Archive:Astrophysics Source Code Library: Difference between revisions
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Here is a list of professional astrophysics | {{ntnes}} | ||
Here is a list of professional astrophysics codes. Many were copied | |||
from the astrophysics source code library, which hasn't been updated | |||
in a while. | |||
== Accretion Disks == | |||
[http://ascl.net/dusty.html DUSTY] - Radiation transport in a dusty environment Ivezic, Z., Nenkova, M., & Elitzur, M. | [http://ascl.net/dusty.html DUSTY] - Radiation transport in a dusty environment Ivezic, Z., Nenkova, M., & Elitzur, M. | ||
XSTAR: A program for calculating conditions and spectra of photoionized gases | XSTAR: A program for calculating conditions and spectra of photoionized gases | ||
| Line 10: | Line 12: | ||
http://ascl.net/xstar.html | http://ascl.net/xstar.html | ||
== Astrochemistry == | |||
CSENV: A code for the chemistry of CircumStellar ENVelopes | CSENV: A code for the chemistry of CircumStellar ENVelopes | ||
| Line 16: | Line 18: | ||
http://ascl.net/csenv.html | http://ascl.net/csenv.html | ||
== Astrometry == | |||
StarFinder: A code for stellar field analysis | StarFinder: A code for stellar field analysis | ||
| Line 22: | Line 24: | ||
http://ascl.net/starfinder.html | http://ascl.net/starfinder.html | ||
== Astronomical Databases: Miscellaneous == | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 28: | Line 30: | ||
http://ascl.net/chianti.html | http://ascl.net/chianti.html | ||
== Atomic Data == | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 34: | Line 36: | ||
http://ascl.net/chianti.html | http://ascl.net/chianti.html | ||
== Atomic Processes == | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 48: | Line 50: | ||
http://ascl.net/popratio.html | http://ascl.net/popratio.html | ||
== Black Hole Physics == | |||
BHSKY: Visual distortions near a black hole | BHSKY: Visual distortions near a black hole | ||
| Line 54: | Line 56: | ||
http://ascl.net/bhsky.html | http://ascl.net/bhsky.html | ||
== Circumstellar Matter == | |||
CSENV: A code for the chemistry of CircumStellar ENVelopes | CSENV: A code for the chemistry of CircumStellar ENVelopes | ||
| Line 60: | Line 62: | ||
http://ascl.net/csenv.html | http://ascl.net/csenv.html | ||
== Cosmic Microwave Background == | |||
COSMICS: Cosmological initial conditions and microwave anisotropy codes | COSMICS: Cosmological initial conditions and microwave anisotropy codes | ||
| Line 78: | Line 80: | ||
http://ascl.net/icosahedron.html | http://ascl.net/icosahedron.html | ||
== Cosmology: Theory == | |||
COSMICS: Cosmological initial conditions and microwave anisotropy codes | COSMICS: Cosmological initial conditions and microwave anisotropy codes | ||
| Line 100: | Line 102: | ||
http://ascl.net/cmbfast.html | http://ascl.net/cmbfast.html | ||
== Cosmology: Large-Scale Structure of Universe == | |||
MLAPM: Simulating Structure Formation from Collisionless Matter | MLAPM: Simulating Structure Formation from Collisionless Matter | ||
| Line 106: | Line 108: | ||
http://ascl.net/mlapm.html | http://ascl.net/mlapm.html | ||
== Dark Matter == | |||
COSMICS: Cosmological initial conditions and microwave anisotropy codes | COSMICS: Cosmological initial conditions and microwave anisotropy codes | ||
| Line 124: | Line 126: | ||
http://ascl.net/cmbfast.html | http://ascl.net/cmbfast.html | ||
== Distance Scale == | |||
ANGSIZ: A general and practical method for calculating cosmological distances | ANGSIZ: A general and practical method for calculating cosmological distances | ||
| Line 134: | Line 136: | ||
http://ascl.net/slopes.html | http://ascl.net/slopes.html | ||
== Elementary Particles == | |||
COSMICS: Cosmological initial conditions and microwave anisotropy codes | COSMICS: Cosmological initial conditions and microwave anisotropy codes | ||
| Line 140: | Line 142: | ||
http://ascl.net/cosmics.html | http://ascl.net/cosmics.html | ||
== Galaxies == | |||
=== Elliptical === | |||
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | ||
Barkana, R. | Barkana, R. | ||
http://ascl.net/fastell.html | http://ascl.net/fastell.html | ||
=== Formation === | |||
MLAPM: Simulating Structure Formation from Collisionless Matter | MLAPM: Simulating Structure Formation from Collisionless Matter | ||
| Line 156: | Line 159: | ||
http://ascl.net/sph_1d.html | http://ascl.net/sph_1d.html | ||
=== Halos === | |||
MLAPM: Simulating Structure Formation from Collisionless Matter | MLAPM: Simulating Structure Formation from Collisionless Matter | ||
| Line 162: | Line 165: | ||
http://ascl.net/mlapm.html | http://ascl.net/mlapm.html | ||
=== Individual === | |||
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | ||
| Line 168: | Line 171: | ||
http://ascl.net/fastell.html | http://ascl.net/fastell.html | ||
=== Interactions === | |||
SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies | SPH_1D: Hierarchical gravity/SPH treecode for simulations of interacting galaxies | ||
| Line 174: | Line 177: | ||
http://ascl.net/sph_1d.html | http://ascl.net/sph_1d.html | ||
=== Structure === | |||
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | ||
| Line 180: | Line 183: | ||
http://ascl.net/fastell.html | http://ascl.net/fastell.html | ||
=== Content === | |||
BSGMODEL: The Bahcall-Soneira Galaxy Model | BSGMODEL: The Bahcall-Soneira Galaxy Model | ||
| Line 186: | Line 189: | ||
http://ascl.net/bsgmodel.html | http://ascl.net/bsgmodel.html | ||
=== Structure === | |||
BSGMODEL: The Bahcall-Soneira Galaxy Model | BSGMODEL: The Bahcall-Soneira Galaxy Model | ||
| Line 196: | Line 199: | ||
http://ascl.net/extinct.html | http://ascl.net/extinct.html | ||
=== Bursts === | |||
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | ||
| Line 210: | Line 213: | ||
http://ascl.net/block.html | http://ascl.net/block.html | ||
=== Observations === | |||
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | ||
| Line 216: | Line 219: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
=== Gravitation === | |||
NBODY2: A Direct N-Body Integration Code | NBODY2: A Direct N-Body Integration Code | ||
| Line 230: | Line 233: | ||
http://ascl.net/gadget.html | http://ascl.net/gadget.html | ||
== Gravitational Lensing == | |||
FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | FASTELL: Fast calculation of a family of elliptical mass gravitational lens models | ||
| Line 252: | Line 255: | ||
http://ascl.net/lensky.html | http://ascl.net/lensky.html | ||
== Hydrodynamics == | |||
GADGET: A code for cosmological simulations of structure formation | GADGET: A code for cosmological simulations of structure formation | ||
| Line 258: | Line 261: | ||
http://ascl.net/gadget.html | http://ascl.net/gadget.html | ||
== Instrumentation == | |||
=== Adaptive Optics === | |||
StarFinder: A code for stellar field analysis | StarFinder: A code for stellar field analysis | ||
| Line 264: | Line 269: | ||
http://ascl.net/starfinder.html | http://ascl.net/starfinder.html | ||
=== Detectors === | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/cxc/isis/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
CONSKY: Sky CCD Integration Simulation | CONSKY: Sky CCD Integration Simulation | ||
| Line 278: | Line 287: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
=== Interferometric === | |||
AIPS: Astronomical Image Processing System | AIPS: Astronomical Image Processing System | ||
| Line 284: | Line 293: | ||
http://ascl.net/aips.html | http://ascl.net/aips.html | ||
=== Photometers === | |||
IRAF: Image Reduction and Analysis Facility | IRAF: Image Reduction and Analysis Facility | ||
| Line 290: | Line 299: | ||
http://ascl.net/iraf.html | http://ascl.net/iraf.html | ||
=== Spectrographs === | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
IRAF: Image Reduction and Analysis Facility | IRAF: Image Reduction and Analysis Facility | ||
| Line 304: | Line 317: | ||
http://ascl.net/rvsao.html | http://ascl.net/rvsao.html | ||
ISM | == ISM == | ||
=== Abundances === | |||
CLOUDY: Numerical simulation of plasmas and their spectra | CLOUDY: Numerical simulation of plasmas and their spectra | ||
| Line 310: | Line 325: | ||
http://ascl.net/cloudy.html | http://ascl.net/cloudy.html | ||
=== Atoms === | |||
CLOUDY: Numerical simulation of plasmas and their spectra | CLOUDY: Numerical simulation of plasmas and their spectra | ||
| Line 316: | Line 331: | ||
http://ascl.net/cloudy.html | http://ascl.net/cloudy.html | ||
=== Dust === | |||
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | ||
| Line 330: | Line 345: | ||
http://ascl.net/dusty.html | http://ascl.net/dusty.html | ||
=== Extinction === | |||
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | ||
| Line 344: | Line 359: | ||
http://ascl.net/dusty.html | http://ascl.net/dusty.html | ||
=== Molecules === | |||
RATRAN: Radiative transfer and molecular excitation in one and two dimensions | RATRAN: Radiative transfer and molecular excitation in one and two dimensions | ||
| Line 354: | Line 369: | ||
http://ascl.net/csenv.html | http://ascl.net/csenv.html | ||
== Large-Scale Structure Of The Universe == | |||
COSMICS: Cosmological initial conditions and microwave anisotropy codes | COSMICS: Cosmological initial conditions and microwave anisotropy codes | ||
| Line 368: | Line 383: | ||
http://ascl.net/cmbfast.html | http://ascl.net/cmbfast.html | ||
== Line == | |||
=== Formation === | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
CLOUDY: Numerical simulation of plasmas and their spectra | CLOUDY: Numerical simulation of plasmas and their spectra | ||
| Line 390: | Line 410: | ||
http://ascl.net/popratio.html | http://ascl.net/popratio.html | ||
=== Identification === | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | ||
| Line 400: | Line 424: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
=== Data Analysis === | |||
AIPS: Astronomical Image Processing System | AIPS: Astronomical Image Processing System | ||
| Line 413: | Line 437: | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
StarFinder: A code for stellar field analysis | StarFinder: A code for stellar field analysis | ||
| Line 454: | Line 482: | ||
http://ascl.net/saoimage.html | http://ascl.net/saoimage.html | ||
=== N-Body Simulations === | |||
NBODY2: A Direct N-Body Integration Code | NBODY2: A Direct N-Body Integration Code | ||
| Line 464: | Line 492: | ||
http://ascl.net/gadget.html | http://ascl.net/gadget.html | ||
=== Numerical === | |||
RATRAN: Radiative transfer and molecular excitation in one and two dimensions | RATRAN: Radiative transfer and molecular excitation in one and two dimensions | ||
| Line 478: | Line 506: | ||
http://ascl.net/block.html | http://ascl.net/block.html | ||
=== Statistical === | |||
ISIS: A method for optimal image subtraction | ISIS: A method for optimal image subtraction | ||
| Line 496: | Line 524: | ||
http://ascl.net/block.html | http://ascl.net/block.html | ||
SLstats: Statistics module for the S-Lang interpreter | |||
Davis, J. E. | |||
http://space.mit.edu/cxc/software/slang/modules/stats/ | |||
== Plasmas == | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
CLOUDY: Numerical simulation of plasmas and their spectra | CLOUDY: Numerical simulation of plasmas and their spectra | ||
| Line 518: | Line 554: | ||
http://ascl.net/popratio.html | http://ascl.net/popratio.html | ||
== Radiation Mechanisms: Non-Thermal == | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | ||
| Line 528: | Line 568: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
== Radiation Mechanisms: Thermal == | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
CLOUDY: Numerical simulation of plasmas and their spectra | CLOUDY: Numerical simulation of plasmas and their spectra | ||
| Line 546: | Line 590: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
== Radiative Transfer == | |||
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | ||
| Line 564: | Line 608: | ||
http://ascl.net/dusty.html | http://ascl.net/dusty.html | ||
== Radio Continuum: General == | |||
AIPS: Astronomical Image Processing System | AIPS: Astronomical Image Processing System | ||
| Line 570: | Line 614: | ||
http://ascl.net/aips.html | http://ascl.net/aips.html | ||
== Radio Lines: General == | |||
AIPS: Astronomical Image Processing System | AIPS: Astronomical Image Processing System | ||
| Line 576: | Line 620: | ||
http://ascl.net/aips.html | http://ascl.net/aips.html | ||
== Relativity == | |||
BHSKY: Visual distortions near a black hole | BHSKY: Visual distortions near a black hole | ||
| Line 582: | Line 626: | ||
http://ascl.net/bhsky.html | http://ascl.net/bhsky.html | ||
== Scattering == | |||
DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | DDSCAT: The Discrete Dipole approximation for Scattering and absorption of light by irregular particles | ||
| Line 588: | Line 632: | ||
http://ascl.net/ddscat.html | http://ascl.net/ddscat.html | ||
== Stars == | |||
=== Abundances === | |||
SPECTRUM: A stellar spectral synthesis program | SPECTRUM: A stellar spectral synthesis program | ||
| Line 594: | Line 639: | ||
http://ascl.net/spectrum.html | http://ascl.net/spectrum.html | ||
=== Atmospheres === | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 604: | Line 649: | ||
http://ascl.net/spectrum.html | http://ascl.net/spectrum.html | ||
=== Circumstellar Matter === | |||
DUSTY: Radiation transport in a dusty environment | DUSTY: Radiation transport in a dusty environment | ||
| Line 610: | Line 655: | ||
http://ascl.net/dusty.html | http://ascl.net/dusty.html | ||
=== Fundamental Parameters === | |||
SPECTRUM: A stellar spectral synthesis program | SPECTRUM: A stellar spectral synthesis program | ||
| Line 616: | Line 661: | ||
http://ascl.net/spectrum.html | http://ascl.net/spectrum.html | ||
=== General === | |||
CONSKY: Sky CCD Integration Simulation | CONSKY: Sky CCD Integration Simulation | ||
| Line 622: | Line 667: | ||
http://ascl.net/consky.html | http://ascl.net/consky.html | ||
=== Imaging === | |||
StarFinder: A code for stellar field analysis | StarFinder: A code for stellar field analysis | ||
| Line 628: | Line 673: | ||
http://ascl.net/starfinder.html | http://ascl.net/starfinder.html | ||
=== Individual === | |||
SPECTRUM: A stellar spectral synthesis program | SPECTRUM: A stellar spectral synthesis program | ||
| Line 634: | Line 679: | ||
http://ascl.net/spectrum.html | http://ascl.net/spectrum.html | ||
=== Pre-Main-Sequence === | |||
DUSTY: Radiation transport in a dusty environment | DUSTY: Radiation transport in a dusty environment | ||
| Line 640: | Line 685: | ||
http://ascl.net/dusty.html | http://ascl.net/dusty.html | ||
=== Supernovae === | |||
BOOM: Iron-core collapse supernova simulation | BOOM: Iron-core collapse supernova simulation | ||
[[BoomCode]] | [[BoomCode]] | ||
=== Variables === | |||
CONSKY: Sky CCD Integration Simulation | CONSKY: Sky CCD Integration Simulation | ||
| Line 651: | Line 696: | ||
http://ascl.net/consky.html | http://ascl.net/consky.html | ||
=== Atmosphere === | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 657: | Line 702: | ||
http://ascl.net/chianti.html | http://ascl.net/chianti.html | ||
=== Gamma-Rays === | |||
WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | WINGSPAN: A WINdows Gamma-ray SPectral Analysis program | ||
| Line 663: | Line 708: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
=== Surveys === | |||
CONSKY: Sky CCD Integration Simulation | CONSKY: Sky CCD Integration Simulation | ||
| Line 669: | Line 714: | ||
http://ascl.net/consky.html | http://ascl.net/consky.html | ||
== Techniques == | |||
=== Image Processing === | |||
ISIS: A method for optimal image subtraction | ISIS: A method for optimal image subtraction | ||
| Line 683: | Line 729: | ||
http://ascl.net/ftools.html | http://ascl.net/ftools.html | ||
=== Interferometric === | |||
AIPS: Astronomical Image Processing System | AIPS: Astronomical Image Processing System | ||
| Line 689: | Line 735: | ||
http://ascl.net/aips.html | http://ascl.net/aips.html | ||
=== Photometric === | |||
StarFinder: A code for stellar field analysis | StarFinder: A code for stellar field analysis | ||
| Line 707: | Line 753: | ||
http://ascl.net/saoimage.html | http://ascl.net/saoimage.html | ||
=== Radial Velocities === | |||
RVSAO: Digital redshifts and radial velocities | RVSAO: Digital redshifts and radial velocities | ||
| Line 713: | Line 759: | ||
http://ascl.net/rvsao.html | http://ascl.net/rvsao.html | ||
=== Radar Astronomy === | |||
AIPS: Astronomical Image Processing System | AIPS: Astronomical Image Processing System | ||
| Line 719: | Line 765: | ||
http://ascl.net/aips.html | http://ascl.net/aips.html | ||
=== Spectroscopic === | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 745: | Line 795: | ||
http://ascl.net/wingspan.html | http://ascl.net/wingspan.html | ||
== Telescopes == | |||
CONSKY: Sky CCD Integration Simulation | CONSKY: Sky CCD Integration Simulation | ||
| Line 751: | Line 801: | ||
http://ascl.net/consky.html | http://ascl.net/consky.html | ||
== Ultraviolet: General == | |||
CHIANTI: A database for astrophysical emission line spectroscopy | CHIANTI: A database for astrophysical emission line spectroscopy | ||
| Line 765: | Line 815: | ||
http://ascl.net/saoimage.html | http://ascl.net/saoimage.html | ||
X- | == X-Rays == | ||
=== General === | |||
XSPEC: An X-ray spectral fitting package | XSPEC: An X-ray spectral fitting package | ||
Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | Arnaud, K., Shafer, R., Haberl, F. & Tennant, A. | ||
http://ascl.net/xspec.html | http://ascl.net/xspec.html | ||
[http://space.mit.edu/ASC/ISIS/ ISIS] - A programmable data analysis | |||
environment, similar to IDL or matlab, with a strong emphasis on X-ray | |||
spectral analysis. | |||
FTOOLS: A general package of software to manipulate FITS files | FTOOLS: A general package of software to manipulate FITS files | ||
| Line 779: | Line 834: | ||
http://ascl.net/xstar.html | http://ascl.net/xstar.html | ||
=== Stars === | |||
XSTAR: A program for calculating conditions and spectra of photoionized gases | XSTAR: A program for calculating conditions and spectra of photoionized gases | ||
| Line 786: | Line 841: | ||
[[Category: Astronomy]] | [[Category:Astronomy]] | ||
[[Category: Software]] | [[Category:Software]] | ||
[[Category:Astrophysics]] | |||
[[Category:Source code]] | |||
[[Category:Libraries]] | |||