Debian Astro AstroConda packages

• Tody, Doug: The IRAF Data Reduction and Analysis System. Proc.SPIE 627:733 - 748 (1986) (eprint)

• Debian Astro Team
• Ole Streicher

• 2.18.1-2 (sid)
• 2.18.1-2 (forky)
• 2.18.1-2 (trixie)
• 2.17-4 (bookworm)
• 2.16.1+2018.11.01-6 (bullseye)

• 22 regular users
• 17 recent
• 179 total installations (of 284384 submissions)

• iraf-fitsutil
• iraf-mscred
• iraf-rvsao
• iraf-sptable
• iraf-st4gem
• iraf-wcstools
• iraf-xdimsum

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• Matteo Frigo and Steven G. Johnson: The Design and Implementation of FFTW3. 93(2):216–231 (2005) (eprint)

• Debian Science Maintainers
• Gianfranco Costamagna

• 3.3.10-2 (forky)
• 3.3.8-2 (bullseye)
• 3.3.10-2 (sid)
• 3.3.10-1 (bookworm)
• 3.3.10-2 (trixie)
• 3.3.11. (upstream)

devel

library

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devel-lib

• 427 regular users
• 662 recent
• 8579 total installations (of 284384 submissions)

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• Debian Python Team
• Sandro Tosi

• 1.4.4-3 (bookworm)
• 1.4.4-1 (bullseye)

• 227 regular users
• 218 recent
• 12320 total installations (of 284384 submissions)

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• The Astropy Collaboration, A. M. Price-Whelan, B. M. Sipőcz, H. M. Günther, P. L. Lim, S. M. Crawford, S. Conseil, D. L. Shupe, M. W. Craig, N. Dencheva, A. Ginsburg, J. T. VanderPlas, L. D. Bradley, D. Pérez-Suárez, M. de Val-Borro, T. L. Aldcroft, K. L. Cruz, T. P. Robitaille, E. J. Tollerud, C. Ardelean, T. Babej, Y. P. Bach, M. Bachetti, A. V. Bakanov, S. P. Bamford, G. Barentsen, P. Barmby, A. Baumbach, K. L. Berry, F. Biscani, M. Boquien, K. A. Bostroem, L. G. Bouma, G. B. Brammer, E. M. Bray, H. Breytenbach, H. Buddelmeijer, D. J. Burke, G. Calderone, J. L. Cano Rodríguez, M. Cara, J. V. M. Cardoso, S. Cheedella, Y. Copin, L. Corrales, D. Crichton, D. D’Avella, C. Deil, É. Depagne, J. P. Dietrich, A. Donath, M. Droettboom, N. Earl, T. Erben, S. Fabbro, L. A. Ferreira, T. Finethy, R. T. Fox, L. H. Garrison, S. L. J. Gibbons, D. A. Goldstein, R. Gommers, J. P. Greco, P. Greenfield, A. M. Groener, F. Grollier, A. Hagen, P. Hirst, D. Homeier, A. J. Horton, G. Hosseinzadeh, L. Hu, J. S. Hunkeler, Ž. Ivezić, A. Jain, T. Jenness, G. Kanarek, S. Kendrew, N. S. Kern, W. E. Kerzendorf, A. Khvalko, J. King, D. Kirkby, A. M. Kulkarni, A. Kumar, A. Lee, D. Lenz, S. P. Littlefair, Z. Ma, D. M. Macleod, M. Mastropietro, C. McCully, S. Montagnac, B. M. Morris, M. Mueller, S. J. Mumford, D. Muna, N. A. Murphy, S. Nelson, G. H. Nguyen, J. P. Ninan, M. Nöthe, S. Ogaz, S. Oh, J. K. Parejko, N. Parley, S. Pascual, R. Patil, A. A. Patil, A. L. Plunkett, J. X. Prochaska, T. Rastogi, V. Reddy Janga, J. Sabater, P. Sakurikar, M. Seifert, L. E. Sherbert, H. Sherwood-Taylor, A. Y. Shih, J. Sick, M. T. Silbiger, S. Singanamalla, L. P. Singer, P. H. Sladen, K. A. Sooley, S. Sornarajah, O. Streicher, P. Teuben, S. W. Thomas, G. R. Tremblay, J. E. H. Turner, V. Terrón, M. H. van Kerkwijk, A. de la Vega, L. L. Watkins, B. A. Weaver, J. B. Whitmore, J. Woillez and V. Zabalza: The Astropy Project: Building an Open-science Project and Status of the v2.0 Core Package. The Astronomical Journal 156(3):123 (2018) (eprint)

• Debian Astronomy Maintainers
• Ole Streicher

• 7.0.1-3 (trixie)
• 7.2.0-1 (forky)
• 4.2-6 (bullseye)
• 5.2.1-2 (bookworm)
• 7.2.0-1 (sid)
• 8.1.0 (upstream)

• 325 regular users
• 142 recent
• 1566 total installations (of 284384 submissions)

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• Debian Astro Team
• Ole Streicher

• 1.0.3-1 (sid)
• 0.16.1-1 (bullseye)
• 0.18.3-1 (bookworm)
• 0.24.0-1 (trixie)
• 1.0.3-1 (forky)

• 18 regular users
• 20 recent
• 207 total installations (of 284384 submissions)

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• Debian Python Team
• Timo Röhling

• 2.4.4+ds-2 (sid)
• 2.3.5+ds-3 (forky)
• 1.24.2-1+deb12u1 (bookworm)
• 2.2.4+ds-1 (trixie)
• 1.19.5-1 (bullseye)

• 21883 regular users
• 4842 recent
• 52452 total installations (of 284384 submissions)

• python3-shapely

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• Debian Astronomy Team
• Alexandre Detiste

• 1.8.1-7 (sid)
• 1.8.1-5 (bullseye)
• 1.8.1-5 (bookworm)
• 1.8.1-7 (trixie)
• 1.8.1-7 (forky)

• 50 regular users
• 17 recent
• 187 total installations (of 284384 submissions)

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• Debian Astro Team
• Ole Streicher

• 2.2.4-1 (sid)
• 2.2.2-4~deb13u1 (trixie)
• 2.1.15-2 (bullseye)
• 2.2.1-1 (bookworm)
• 2.2.4-1 (forky)

• 16 regular users
• 18 recent
• 154 total installations (of 284384 submissions)

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• P. L. Lim, R. I. Diaz and V. Laidler: PySynphot User’s Guide. (2015)

• Debian Astronomy Team
• Alexandre Detiste

• 2.0.0+dfsg-3 (sid)
• 1.0.0+dfsg-1 (bullseye)
• 2.0.0+dfsg-1 (bookworm)
• 2.0.0+dfsg-3 (trixie)
• 2.0.0+dfsg-3 (forky)

• 11 regular users
• 18 recent
• 169 total installations (of 284384 submissions)

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• Debian Python Team
• Drew Parsons

• 1.17.1-1exp2 (experimental)
• 1.16.3-4 (sid)
• 1.16.3-4 (forky)
• 1.15.3-1 (trixie)
• 1.10.1-2 (bookworm)
• 1.6.0-2 (bullseye)
• 1.17.1 (upstream)

• 3217 regular users
• 2144 recent
• 30408 total installations (of 284384 submissions)

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• William Desportes

• 2.1.6-1.2 (bullseye)
• 2.1.8-4 (sid)
• 2.1.8-3 (bookworm)
• 2.1.8-4 (forky)
• 2.1.8-4 (trixie)

• 16 regular users
• 14 recent
• 219 total installations (of 284384 submissions)

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This package provides a selection of tools for FITS and WCS handling image handling, and data analysis, used by other STScI packages.

• Debian Astro Team
• Ole Streicher

• 4.0.1-3 (bookworm)
• 3.6.0-1 (bullseye)
• 4.2.0-1 (trixie)
• 4.3.0-1 (forky)
• 4.3.0-1 (sid)

• 1 regular users
• 1 recent
• 33 total installations (of 284384 submissions)

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Advanced Scientific Data Format is a proposed replacement to the FITS standard for astronomical images and other astronomical data. The Metadata is contained in a YAML header followed by binary or ascii data.

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This package aims to provide much of the IDL "astron" functionality that pertains to coordinate manipulations in an OO framework. Our target user is a typical astronomer who needs to analyze data, work with catalogs, prepare observing proposals, and prepare for observing runs.

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This packages is obsolete and replaced by astrolib.coordinates.

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DrizzlePac allows users to easily and accurately align and combine HST images taken at multiple epochs, and even with different instruments. It is a suite of supporting tasks for AstroDrizzle which includes:astrodrizzle to align and combine imagestweakreg and tweakback for aligning images in different visitspixtopix transforms an X,Y pixel position to its pixel position after distortion correctionsskytopix transforms sky coordinates to X,Y pixel positions. A reverse transformation can be done using the task pixtosky.

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Depends on stsci.tools, stsci.convolve, stsci.image, stsci.imagemanip, stsci.imagestats, stsci.ndimage, stsci.stimage, nictools, stwcs, fitsblender, and astrolib.coords.

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POPPY (Physical Optics Propagation in PYthon) simulates physical optical propagation including diffraction. It implements a flexible framework for modeling Fraunhofer and Fresnel diffraction and point spread function formation, particularly in the context of astronomical telescopes. POPPY provides the optical modeling framework for WebbPSF (ascl:1504.007) and was developed as part of a simulation package for JWST, but is available separately and is broadly applicable to many kinds of imaging simulations.

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RELIC stands for "Release I Control". This software attempts to automatically maintain a git project's version information without the need for hardcoded values in the source code. It is designed primarily for hardcore build maintainers, and is best used with continuous integration services (i.e Travis-CI, etc).

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Specview is a tool for 1-D spectral visualization and analysis of astronomical spectrograms. Written in Java, it is capable of reading all the Hubble Space Telescope spectral data formats as well as data from several other instruments (such as IUE, FUSE, ISO, FORS and SDSS), preview spectra from MAST, and data from generic FITS and ASCII tables. It can read data from Virtual Observatory servers, and read and write spectrogram data in Virtual Observatory SED format. It can also read files in the SPC Galactic format used in the chemistry field. Once ingested, data can be plotted and examined with a large selection of custom settings. Specview supports instrument-specific data quality handling, flexible spectral units conversions, custom plotting attributes, plot annotations, tiled plots, hardcopy to JPEG files and PostScript file or printer, etc. Specview can be used to build wide-band SEDs, overplotting or combining data from the same astronomical source taken with different instruments and/or spectral bands. Data can be further processed with averaging, splicing, detrending, and Fourier filtering tools. Specview has a spectral model fitting capability that enables the user to work with multi-component models (including user- defined models) and fit models to data.

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Package is outdated and replaced by Scipy

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Package is outdated and replaced by Scipy

Visualize numpy array objects using image display tools like ds9 and ximtool

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Package is outdated and may be replaced by pyds9.

Python package for handling spherical polygons that represent arbitrary regions of the sky.sphere

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Package is outdated and replaced by Scipy

Recomputes the WCS of an HST observation and puts all distortion corrections in the headers.

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