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		<id>https://ideawaza.com/index.php?title=Archive:Astrophysics_Source_Code_Library&amp;diff=20699</id>
		<title>Archive:Astrophysics Source Code Library</title>
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		<updated>2007-12-01T18:37:25Z</updated>

		<summary type="html">&lt;p&gt;66.31.39.225: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is a list of professional astrophysics codes.  Many were copied&lt;br /&gt;
from the astrophysics source code library, which hasn&#039;t been updated&lt;br /&gt;
in a while.&lt;br /&gt;
&lt;br /&gt;
== Accretion Disks ==&lt;br /&gt;
&lt;br /&gt;
[http://ascl.net/dusty.html DUSTY] - Radiation transport in a dusty environment Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
== Astrochemistry ==&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
== Astrometry ==&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
== Astronomical Databases: Miscellaneous ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
== Atomic Data ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
== Atomic Processes ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
== Black Hole Physics ==&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
== Circumstellar Matter ==&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
== Cosmic Microwave Background ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
Icosahedron: The Icosahedron Package for Pixelizing the Sphere&lt;br /&gt;
Tegmark, M.&lt;br /&gt;
http://ascl.net/icosahedron.html&lt;br /&gt;
&lt;br /&gt;
== Cosmology: Theory ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
== Cosmology: Large-Scale Structure of Universe ==&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
== Dark Matter ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
== Distance Scale ==&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
== Elementary Particles ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
== Galaxies ==&lt;br /&gt;
&lt;br /&gt;
=== Elliptical ===&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
=== Formation ===&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
=== Halos ===&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
=== Individual ===&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
=== Interactions ===&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
=== Structure ===&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
=== Content ===&lt;br /&gt;
&lt;br /&gt;
BSGMODEL: The Bahcall-Soneira Galaxy Model&lt;br /&gt;
Bahcall, J. N.&lt;br /&gt;
http://ascl.net/bsgmodel.html&lt;br /&gt;
&lt;br /&gt;
=== Structure ===&lt;br /&gt;
&lt;br /&gt;
BSGMODEL: The Bahcall-Soneira Galaxy Model&lt;br /&gt;
Bahcall, J. N.&lt;br /&gt;
http://ascl.net/bsgmodel.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
=== Bursts ===&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
=== Observations ===&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Gravitation ===&lt;br /&gt;
&lt;br /&gt;
NBODY2: A Direct N-Body Integration Code&lt;br /&gt;
Aarseth, S.&lt;br /&gt;
http://ascl.net/nbody2.html&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
== Gravitational Lensing ==&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
LENSKY: Galactic Microlensing Probability&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/lensky.html&lt;br /&gt;
&lt;br /&gt;
== Hydrodynamics ==&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
== Instrumentation ==&lt;br /&gt;
&lt;br /&gt;
=== Adaptive Optics ===&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
=== Detectors ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Interferometric ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
=== Photometers ===&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
=== Spectrographs ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
== ISM ==&lt;br /&gt;
&lt;br /&gt;
=== Abundances ===&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
=== Atoms ===&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
=== Dust ===&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Extinction ===&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Molecules ===&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
== Large-Scale Structure Of The Universe ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
== Line ==&lt;br /&gt;
=== Formation ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
=== Identification ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Data Analysis ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
Icosahedron: The Icosahedron Package for Pixelizing the Sphere&lt;br /&gt;
Tegmark, M.&lt;br /&gt;
http://ascl.net/icosahedron.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
=== N-Body Simulations ===&lt;br /&gt;
&lt;br /&gt;
NBODY2: A Direct N-Body Integration Code&lt;br /&gt;
Aarseth, S.&lt;br /&gt;
http://ascl.net/nbody2.html&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
=== Numerical ===&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
=== Statistical ===&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
SLstats: Statistics module for the S-Lang interpreter&lt;br /&gt;
Davis, J. E.&lt;br /&gt;
http://space.mit.edu/cxc/software/slang/modules/stats/&lt;br /&gt;
&lt;br /&gt;
== Plasmas ==&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
== Radiation Mechanisms: Non-Thermal ==&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
== Radiation Mechanisms: Thermal ==&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
== Radiative Transfer ==&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
== Radio Continuum: General ==&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
== Radio Lines: General ==&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
== Relativity ==&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
== Scattering ==&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
=== Abundances ===&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== Atmospheres ===&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== Circumstellar Matter ===&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Fundamental Parameters ===&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== General ===&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
=== Imaging ===&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
=== Individual ===&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== Pre-Main-Sequence ===&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Supernovae ===&lt;br /&gt;
&lt;br /&gt;
BOOM: Iron-core collapse supernova simulation&lt;br /&gt;
[[BoomCode]]&lt;br /&gt;
&lt;br /&gt;
=== Variables ===&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
=== Gamma-Rays ===&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Surveys ===&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
== Techniques ==&lt;br /&gt;
=== Image Processing ===&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
=== Interferometric ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
=== Photometric ===&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
=== Radial Velocities ===&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
=== Radar Astronomy ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
=== Spectroscopic ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
== Telescopes ==&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
== Ultraviolet: General ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
== X-Rays ==&lt;br /&gt;
=== General ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
=== Stars ===&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy]]&lt;br /&gt;
[[Category:Software]]&lt;br /&gt;
[[Category:Astrophysics]]&lt;br /&gt;
[[Category:Source code]]&lt;br /&gt;
[[Category:Libraries]]&lt;/div&gt;</summary>
		<author><name>66.31.39.225</name></author>
	</entry>
	<entry>
		<id>https://ideawaza.com/index.php?title=Archive:Astrophysics_Source_Code_Library&amp;diff=20698</id>
		<title>Archive:Astrophysics Source Code Library</title>
		<link rel="alternate" type="text/html" href="https://ideawaza.com/index.php?title=Archive:Astrophysics_Source_Code_Library&amp;diff=20698"/>
		<updated>2007-12-01T18:10:34Z</updated>

		<summary type="html">&lt;p&gt;66.31.39.225: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is a list of professional astrophysics codes.  Many were copied&lt;br /&gt;
from the astrophysics source code library, which hasn&#039;t been updated&lt;br /&gt;
in a while.&lt;br /&gt;
&lt;br /&gt;
== Accretion Disks ==&lt;br /&gt;
&lt;br /&gt;
*[http://ascl.net/dusty.html DUSTY] - Radiation transport in a dusty environment Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
&lt;br /&gt;
*XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
== Astrochemistry ==&lt;br /&gt;
&lt;br /&gt;
*CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
== Astrometry ==&lt;br /&gt;
&lt;br /&gt;
*StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
== Astronomical Databases: Miscellaneous ==&lt;br /&gt;
&lt;br /&gt;
*CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
== Atomic Data ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
== Atomic Processes ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
== Black Hole Physics ==&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
== Circumstellar Matter ==&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
== Cosmic Microwave Background ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
Icosahedron: The Icosahedron Package for Pixelizing the Sphere&lt;br /&gt;
Tegmark, M.&lt;br /&gt;
http://ascl.net/icosahedron.html&lt;br /&gt;
&lt;br /&gt;
== Cosmology: Theory ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
== Cosmology: Large-Scale Structure of Universe ==&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
== Dark Matter ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
== Distance Scale ==&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
== Elementary Particles ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
== Galaxies ==&lt;br /&gt;
&lt;br /&gt;
=== Elliptical ===&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
=== Formation ===&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
=== Halos ===&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
=== Individual ===&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
=== Interactions ===&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
=== Structure ===&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
=== Content ===&lt;br /&gt;
&lt;br /&gt;
BSGMODEL: The Bahcall-Soneira Galaxy Model&lt;br /&gt;
Bahcall, J. N.&lt;br /&gt;
http://ascl.net/bsgmodel.html&lt;br /&gt;
&lt;br /&gt;
=== Structure ===&lt;br /&gt;
&lt;br /&gt;
BSGMODEL: The Bahcall-Soneira Galaxy Model&lt;br /&gt;
Bahcall, J. N.&lt;br /&gt;
http://ascl.net/bsgmodel.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
=== Bursts ===&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
=== Observations ===&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Gravitation ===&lt;br /&gt;
&lt;br /&gt;
NBODY2: A Direct N-Body Integration Code&lt;br /&gt;
Aarseth, S.&lt;br /&gt;
http://ascl.net/nbody2.html&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
== Gravitational Lensing ==&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
LENSKY: Galactic Microlensing Probability&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/lensky.html&lt;br /&gt;
&lt;br /&gt;
== Hydrodynamics ==&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
== Instrumentation ==&lt;br /&gt;
&lt;br /&gt;
=== Adaptive Optics ===&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
=== Detectors ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Interferometric ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
=== Photometers ===&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
=== Spectrographs ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
== ISM ==&lt;br /&gt;
&lt;br /&gt;
=== Abundances ===&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
=== Atoms ===&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
=== Dust ===&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Extinction ===&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Molecules ===&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
== Large-Scale Structure Of The Universe ==&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
== Line ==&lt;br /&gt;
=== Formation ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
=== Identification ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Data Analysis ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
Icosahedron: The Icosahedron Package for Pixelizing the Sphere&lt;br /&gt;
Tegmark, M.&lt;br /&gt;
http://ascl.net/icosahedron.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
=== N-Body Simulations ===&lt;br /&gt;
&lt;br /&gt;
NBODY2: A Direct N-Body Integration Code&lt;br /&gt;
Aarseth, S.&lt;br /&gt;
http://ascl.net/nbody2.html&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
=== Numerical ===&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
=== Statistical ===&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
SLstats: Statistics module for the S-Lang interpreter&lt;br /&gt;
Davis, J. E.&lt;br /&gt;
http://space.mit.edu/cxc/software/slang/modules/stats/&lt;br /&gt;
&lt;br /&gt;
== Plasmas ==&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
== Radiation Mechanisms: Non-Thermal ==&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
== Radiation Mechanisms: Thermal ==&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
== Radiative Transfer ==&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
== Radio Continuum: General ==&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
== Radio Lines: General ==&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
== Relativity ==&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
== Scattering ==&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
== Stars ==&lt;br /&gt;
=== Abundances ===&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== Atmospheres ===&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== Circumstellar Matter ===&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Fundamental Parameters ===&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== General ===&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
=== Imaging ===&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
=== Individual ===&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
=== Pre-Main-Sequence ===&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
=== Supernovae ===&lt;br /&gt;
&lt;br /&gt;
BOOM: Iron-core collapse supernova simulation&lt;br /&gt;
[[BoomCode]]&lt;br /&gt;
&lt;br /&gt;
=== Variables ===&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
=== Atmosphere ===&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
=== Gamma-Rays ===&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
=== Surveys ===&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
== Techniques ==&lt;br /&gt;
=== Image Processing ===&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
=== Interferometric ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
=== Photometric ===&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
=== Radial Velocities ===&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
=== Radar Astronomy ===&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
=== Spectroscopic ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
== Telescopes ==&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
== Ultraviolet: General ==&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
== X-Rays ==&lt;br /&gt;
=== General ===&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis&lt;br /&gt;
environment, similar to IDL or matlab, with a strong emphasis on X-ray&lt;br /&gt;
spectral analysis.&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
=== Stars ===&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy]]&lt;br /&gt;
[[Category:Software]]&lt;br /&gt;
[[Category:Astrophysics]]&lt;br /&gt;
[[Category:Source code]]&lt;br /&gt;
[[Category:Libraries]]&lt;/div&gt;</summary>
		<author><name>66.31.39.225</name></author>
	</entry>
	<entry>
		<id>https://ideawaza.com/index.php?title=Archive:Astrophysics_Source_Code_Library&amp;diff=20697</id>
		<title>Archive:Astrophysics Source Code Library</title>
		<link rel="alternate" type="text/html" href="https://ideawaza.com/index.php?title=Archive:Astrophysics_Source_Code_Library&amp;diff=20697"/>
		<updated>2007-12-01T05:55:04Z</updated>

		<summary type="html">&lt;p&gt;66.31.39.225: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;Here is a list of professional astrophysics code copied from the astrophysics source code library which hasn&#039;t been updated in a while.&lt;br /&gt;
&lt;br /&gt;
accretion disks&lt;br /&gt;
*[http://ascl.net/dusty.html DUSTY] - Radiation transport in a dusty environment Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
*XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
*Kallman, T.&lt;br /&gt;
*http://ascl.net/xstar.html&lt;br /&gt;
*astrochemistry&lt;br /&gt;
*CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
*Mamon, G. A.&lt;br /&gt;
*http://ascl.net/csenv.html&lt;br /&gt;
*astrometry&lt;br /&gt;
*StarFinder: A code for stellar field analysis&lt;br /&gt;
*Diolaiti, E. et al.&lt;br /&gt;
*http://ascl.net/starfinder.html&lt;br /&gt;
*Astronomical databases: miscellaneous&lt;br /&gt;
*CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
*CHIANTI Consortium&lt;br /&gt;
*http://ascl.net/chianti.html&lt;br /&gt;
*Atomic data&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
atomic processes&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
black hole physics&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
circumstellar matter&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
cosmic microwave background&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
Icosahedron: The Icosahedron Package for Pixelizing the Sphere&lt;br /&gt;
Tegmark, M.&lt;br /&gt;
http://ascl.net/icosahedron.html&lt;br /&gt;
&lt;br /&gt;
cosmology: theory&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
cosmology: large-scale structure of universe&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
dark matter&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
distance scale&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
elementary particles&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
galaxies: elliptical&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
galaxies: formation&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
galaxies: halos&lt;br /&gt;
&lt;br /&gt;
MLAPM: Simulating Structure Formation from Collisionless Matter&lt;br /&gt;
Knebe, A., Green, A. &amp;amp; Binney, J.&lt;br /&gt;
http://ascl.net/mlapm.html&lt;br /&gt;
&lt;br /&gt;
galaxies: individual&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
galaxies: interactions&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
galaxies: structure&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
Galaxy: stellar content&lt;br /&gt;
&lt;br /&gt;
BSGMODEL: The Bahcall-Soneira Galaxy Model&lt;br /&gt;
Bahcall, J. N.&lt;br /&gt;
http://ascl.net/bsgmodel.html&lt;br /&gt;
&lt;br /&gt;
Galaxy: structure&lt;br /&gt;
&lt;br /&gt;
BSGMODEL: The Bahcall-Soneira Galaxy Model&lt;br /&gt;
Bahcall, J. N.&lt;br /&gt;
http://ascl.net/bsgmodel.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
gamma-rays: bursts&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
gamma-rays: observations&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
gravitation&lt;br /&gt;
&lt;br /&gt;
NBODY2: A Direct N-Body Integration Code&lt;br /&gt;
Aarseth, S.&lt;br /&gt;
http://ascl.net/nbody2.html&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
gravitational lensing&lt;br /&gt;
&lt;br /&gt;
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models&lt;br /&gt;
Barkana, R.&lt;br /&gt;
http://ascl.net/fastell.html&lt;br /&gt;
&lt;br /&gt;
ANGSIZ: A general and practical method for calculating cosmological distances&lt;br /&gt;
Helbig, P., Kayser, R., &amp;amp; Schramm, T.&lt;br /&gt;
http://ascl.net/angsiz.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
LENSKY: Galactic Microlensing Probability&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/lensky.html&lt;br /&gt;
&lt;br /&gt;
hydrodynamics&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
instrumentation: adaptive optics&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
instrumentation: detectors&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
instrumentation: interferometric&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
instrumentation: photometers&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
instrumentation: spectrographs&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
ISM: abundances&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
ISM: atoms&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
ISM: dust&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
ISM: extinction&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
EXTINCT: A Computerized Model of Large-Scale Visual Interstellar Extinction&lt;br /&gt;
Hakkila, J., Myers, J. M., Stidman, B. J., Hartmann, D. H.&lt;br /&gt;
http://ascl.net/extinct.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
ISM: molecules&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
CSENV: A code for the chemistry of CircumStellar ENVelopes&lt;br /&gt;
Mamon, G. A.&lt;br /&gt;
http://ascl.net/csenv.html&lt;br /&gt;
&lt;br /&gt;
large-scale structure of the universe&lt;br /&gt;
&lt;br /&gt;
COSMICS: Cosmological initial conditions and microwave anisotropy codes&lt;br /&gt;
Bertschinger, E.&lt;br /&gt;
http://ascl.net/cosmics.html&lt;br /&gt;
&lt;br /&gt;
PMcode: Particle-Mesh code for cosmological simulations&lt;br /&gt;
Klypin, A. &amp;amp; Holtzman, J.&lt;br /&gt;
http://ascl.net/pmcode.html&lt;br /&gt;
&lt;br /&gt;
CMBFAST: A microwave anisotropy code&lt;br /&gt;
Seljak, U. &amp;amp; Zaldarriaga, M.&lt;br /&gt;
http://ascl.net/cmbfast.html&lt;br /&gt;
&lt;br /&gt;
line: formation&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
line: identification&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
methods: data analysis&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
MILLISEARCH: A Search for Millilensing in BATSE GRB Data&lt;br /&gt;
Nemiroff, Robert J.&lt;br /&gt;
http://ascl.net/millisearch.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
Icosahedron: The Icosahedron Package for Pixelizing the Sphere&lt;br /&gt;
Tegmark, M.&lt;br /&gt;
http://ascl.net/icosahedron.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
methods: N-body simulations&lt;br /&gt;
&lt;br /&gt;
NBODY2: A Direct N-Body Integration Code&lt;br /&gt;
Aarseth, S.&lt;br /&gt;
http://ascl.net/nbody2.html&lt;br /&gt;
&lt;br /&gt;
GADGET: A code for cosmological simulations of structure formation&lt;br /&gt;
Springel, V. &amp;amp; Yoshida, N.&lt;br /&gt;
http://ascl.net/gadget.html&lt;br /&gt;
&lt;br /&gt;
methods: numerical&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies&lt;br /&gt;
Olson, K.&lt;br /&gt;
http://ascl.net/sph_1d.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
methods: statistical&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
SLOPES: least-squares linear regression lines for bivariate datasets&lt;br /&gt;
Feigelson, E.&lt;br /&gt;
http://ascl.net/slopes.html&lt;br /&gt;
&lt;br /&gt;
RADPACK: A RADical compression analysis PACKage for fitting to the CMB&lt;br /&gt;
Knox, L.&lt;br /&gt;
http://ascl.net/radpack.html&lt;br /&gt;
&lt;br /&gt;
BLOCK: A Bayesian block method to analyze structure in photon counting data&lt;br /&gt;
Scargle, J. D.&lt;br /&gt;
http://ascl.net/block.html&lt;br /&gt;
&lt;br /&gt;
SLstats: Statistics module for the S-Lang interpreter&lt;br /&gt;
Davis, J. E.&lt;br /&gt;
http://space.mit.edu/cxc/software/slang/modules/stats/&lt;br /&gt;
&lt;br /&gt;
plasmas&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
PopRatio: A program to calculate atomic level populations in astrophysical plasmas&lt;br /&gt;
Silva, A. I. &amp;amp; Viegas, S. M.&lt;br /&gt;
http://ascl.net/popratio.html&lt;br /&gt;
&lt;br /&gt;
radiation mechanisms: non-thermal&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
radiation mechanisms: thermal&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
radiative transfer&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
CLOUDY: Numerical simulation of plasmas and their spectra&lt;br /&gt;
Ferland, G. et al.&lt;br /&gt;
http://ascl.net/cloudy.html&lt;br /&gt;
&lt;br /&gt;
RATRAN: Radiative transfer and molecular excitation in one and two dimensions&lt;br /&gt;
Hogerheijde, Michiel &amp;amp; van der Tak, Floris&lt;br /&gt;
http://ascl.net/ratran.html&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
radio continuum: general&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
radio lines: general&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
relativity&lt;br /&gt;
&lt;br /&gt;
BHSKY: Visual distortions near a black hole&lt;br /&gt;
Nemiroff, R. J.&lt;br /&gt;
http://ascl.net/bhsky.html&lt;br /&gt;
&lt;br /&gt;
scattering&lt;br /&gt;
&lt;br /&gt;
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles&lt;br /&gt;
Draine, B. T. &amp;amp; Flatau, Piotr J.&lt;br /&gt;
http://ascl.net/ddscat.html&lt;br /&gt;
&lt;br /&gt;
stars: abundances&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
stars: atmospheres&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
stars: circumstellar matter&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
stars: fundamental parameters&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
stars: general&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
stars: imaging&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
stars: individual&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
stars: pre-main-sequence&lt;br /&gt;
&lt;br /&gt;
DUSTY: Radiation transport in a dusty environment&lt;br /&gt;
Ivezic, Z., Nenkova, M., &amp;amp; Elitzur, M.&lt;br /&gt;
http://ascl.net/dusty.html&lt;br /&gt;
&lt;br /&gt;
stars: supernovae&lt;br /&gt;
&lt;br /&gt;
BOOM: Iron-core collapse supernova simulation&lt;br /&gt;
[[BoomCode]]&lt;br /&gt;
&lt;br /&gt;
stars: variables&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
Sun: atmosphere&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
Sun: gamma-rays&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
surveys&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
techniques: image processing&lt;br /&gt;
&lt;br /&gt;
ISIS: A method for optimal image subtraction&lt;br /&gt;
Alard, C. &amp;amp; Lupton, R.&lt;br /&gt;
http://ascl.net/isis.html&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
techniques: interferometric&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
techniques: photometric&lt;br /&gt;
&lt;br /&gt;
StarFinder: A code for stellar field analysis&lt;br /&gt;
Diolaiti, E. et al.&lt;br /&gt;
http://ascl.net/starfinder.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
techniques: radial velocities&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
techniques: radar astronomy&lt;br /&gt;
&lt;br /&gt;
AIPS: Astronomical Image Processing System&lt;br /&gt;
AIPS Team&lt;br /&gt;
http://ascl.net/aips.html&lt;br /&gt;
&lt;br /&gt;
techniques: spectroscopic&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
SPECTRUM: A stellar spectral synthesis program&lt;br /&gt;
Gray, R. O.&lt;br /&gt;
http://ascl.net/spectrum.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
RVSAO: Digital redshifts and radial velocities&lt;br /&gt;
Kurtz, M. J. &amp;amp; Mink, D. J.&lt;br /&gt;
http://ascl.net/rvsao.html&lt;br /&gt;
&lt;br /&gt;
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program&lt;br /&gt;
Preece, R. D., Briggs, M. S., Mallozzi R. S., &amp;amp; Brock, M. N.&lt;br /&gt;
http://ascl.net/wingspan.html&lt;br /&gt;
&lt;br /&gt;
telescopes&lt;br /&gt;
&lt;br /&gt;
CONSKY: Sky CCD Integration Simulation&lt;br /&gt;
Nemiroff, R. J. &amp;amp; Rafert, J. B.&lt;br /&gt;
http://ascl.net/consky.html&lt;br /&gt;
&lt;br /&gt;
ultraviolet: general&lt;br /&gt;
&lt;br /&gt;
CHIANTI: A database for astrophysical emission line spectroscopy&lt;br /&gt;
CHIANTI Consortium&lt;br /&gt;
http://ascl.net/chianti.html&lt;br /&gt;
&lt;br /&gt;
IRAF: Image Reduction and Analysis Facility&lt;br /&gt;
IRAF Team&lt;br /&gt;
http://ascl.net/iraf.html&lt;br /&gt;
&lt;br /&gt;
SAOimage: A utility for displaying astronomical images in the X11 window environment&lt;br /&gt;
VanHilst, M. &amp;amp; Mink, D.&lt;br /&gt;
http://ascl.net/saoimage.html&lt;br /&gt;
&lt;br /&gt;
X-rays: general&lt;br /&gt;
&lt;br /&gt;
XSPEC: An X-ray spectral fitting package&lt;br /&gt;
Arnaud, K., Shafer, R., Haberl, F. &amp;amp; Tennant, A.&lt;br /&gt;
http://ascl.net/xspec.html&lt;br /&gt;
&lt;br /&gt;
ISIS: An extensible programmable data and X-ray spectral analysis environment&lt;br /&gt;
Houck, J. C.&lt;br /&gt;
http://space.mit.edu/ASC/ISIS/&lt;br /&gt;
&lt;br /&gt;
FTOOLS: A general package of software to manipulate FITS files&lt;br /&gt;
FTOOLS Team&lt;br /&gt;
http://ascl.net/ftools.html&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
X-rays: stars&lt;br /&gt;
&lt;br /&gt;
XSTAR: A program for calculating conditions and spectra of photoionized gases&lt;br /&gt;
Kallman, T.&lt;br /&gt;
http://ascl.net/xstar.html&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
[[Category:Astronomy]]&lt;br /&gt;
[[Category:Software]]&lt;br /&gt;
[[Category:Astrophysics]]&lt;br /&gt;
[[Category:Source code]]&lt;br /&gt;
[[Category:Libraries]]&lt;/div&gt;</summary>
		<author><name>66.31.39.225</name></author>
	</entry>
	<entry>
		<id>https://ideawaza.com/index.php?title=Instance_dungeon&amp;diff=72104</id>
		<title>Instance dungeon</title>
		<link rel="alternate" type="text/html" href="https://ideawaza.com/index.php?title=Instance_dungeon&amp;diff=72104"/>
		<updated>2007-10-22T00:18:57Z</updated>

		<summary type="html">&lt;p&gt;66.31.197.38: &lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;{{Unreferenced|date= May 2007}}&lt;br /&gt;
In [[MMORPG]]s, an &#039;&#039;&#039;instance dungeon&#039;&#039;&#039; is a special area, typically a [[dungeon (games)|dungeon]], that generates a new copy, or instance, of the dungeon map for each group that enters the area. This saves server work and ensures that there will never be competition ([[kill stealing]], [[spawn camping]]) over resources such as [[mob (computer gaming)|mobs]] within the instance and that [[player character]]s experience minimum [[lag]]. &lt;br /&gt;
&lt;br /&gt;
This also preserves the gaming experience, since some gaming scenarios do not work if the player is continually surrounded by other players, as in a multiplayer setting. Instance dungeons may contain stronger than usual mobs and rare, sought-after equipment. They also may include level restrictions and/or restrict the number of players allowed in each instance to balance gameplay.&lt;br /&gt;
&lt;br /&gt;
Instances were first proposed by [[Richard Garriott]] in the late 1990&#039;s as a way to solve a set of related problems which had become obvious in [[Ultima Online]]. The problem is simple to state: everyone wants to be &amp;quot;A Hero&amp;quot; and slay &amp;quot;The Monster&amp;quot;, rescue &amp;quot;The Princess&amp;quot; and obtain &amp;quot;The Magic Sword&amp;quot;. When there are 2,000 and more players all playing the same game, clearly not everyone can be a hero. The problem of everyone wanting to kill the same monster and gain the best treasure was terribly obvious in the game [[EverQuest]]. The creation of instances largely solves this set of problems. There are few examples of boss camping and kill stealing in [[World of Warcraft]] - because a copy of the dungeon (instance) is always created on demand for you or your party.&lt;br /&gt;
&lt;br /&gt;
Games that have been known to use instancing include:&lt;br /&gt;
*&#039;&#039;[[Anarchy Online]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[City of Heroes]]&#039;&#039;/&#039;&#039;[[City of Villains]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Dark Age of Camelot]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Dungeon Runners]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Runescape]]&#039;&#039; (only for numerous &#039;minigames&#039;)&lt;br /&gt;
*&#039;&#039;[[EverQuest]]&#039;&#039; (instances added in 2003)&lt;br /&gt;
*&#039;&#039;[[EverQuest 2]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Final Fantasy XI]]&#039;&#039; (instances added with the Treasures of Aht Urghan expansion)&lt;br /&gt;
*&#039;&#039;[[Granado Espada]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Guild Wars]]&#039;&#039; (uses instancing for every area where monsters must be fought.)&lt;br /&gt;
*&#039;&#039;[[Myst Online: Uru Live]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[The Realm Online]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[World of Warcraft]]&#039;&#039;; see [[Instance (World of Warcraft)]]&lt;br /&gt;
*&#039;&#039;[[The Lord of the Rings Online: Shadows of Angmar]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Tabula Rasa (game)|Tabula Rasa]]&#039;&#039;&lt;br /&gt;
*&#039;&#039;[[Auto Assault]]&#039;&#039;&lt;br /&gt;
One game known for not using instance dungeons is &#039;&#039;[[EVE Online]]&#039;&#039;. Because of the vast amount of space available in the EVE universe, missions for players are created in real space, which any other player could in theory travel to. This allows multiple players to perform the same mission at the same time (in the same manner as an instanced dungeon) but also allows other players to view or participate in the mission, if they discover the location, or if invited to assist by the player who was initially given the mission.&lt;br /&gt;
&lt;br /&gt;
&#039;&#039;[[Vanguard: Saga of Heroes]]&#039;&#039; is another game that does not use instance dungeons. However, it is envisioned that, through the Advanced Encounter System (AES), certain &amp;quot;boss&amp;quot; NPCs can be triggered when a group enters an area; this NPC would then be &amp;quot;tagged&amp;quot; to that group, meaning no other players could attack or interact with it. AES was not implemented in the commercial release of &#039;&#039;V:SoH&#039;&#039;, but Sigil programmers are reportedly working on it and are planning to release it in a future patch.&lt;br /&gt;
&lt;br /&gt;
In [[RuneScape]], instance dungeons are used mostly in quests, so that other players cannot interfere with the player who is doing the quest, such as battling boss [[NPC]]&#039;s or having to accomplish a special task.&lt;br /&gt;
&lt;br /&gt;
Several games use instancing to scale the [[mob (computer gaming)|mobs]] to the players&#039; levels, and/or the number of players present.&lt;br /&gt;
&lt;br /&gt;
[[Category:Video game gameplay]]&lt;br /&gt;
[[Category:Massively multiplayer online role-playing games]]&lt;br /&gt;
[[Category:Competitive video gaming]]&lt;br /&gt;
&lt;br /&gt;
[[de:Instanz (Computerspiel)]]&lt;br /&gt;
[[fr:Donjon instancié]]&lt;/div&gt;</summary>
		<author><name>66.31.197.38</name></author>
	</entry>
	<entry>
		<id>https://ideawaza.com/index.php?title=Archive:Aquamarine&amp;diff=26050</id>
		<title>Archive:Aquamarine</title>
		<link rel="alternate" type="text/html" href="https://ideawaza.com/index.php?title=Archive:Aquamarine&amp;diff=26050"/>
		<updated>2007-02-04T00:45:13Z</updated>

		<summary type="html">&lt;p&gt;66.31.29.120: ←Blanked the page&lt;/p&gt;
&lt;hr /&gt;
&lt;div&gt;&lt;/div&gt;</summary>
		<author><name>66.31.29.120</name></author>
	</entry>
</feed>