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  1. Random Astro package of the week is skyview-java. SkyView is a "virtual" observatory dynamically generating images of the sky in different wavelength regimes from a static image database. SkyView is intended as a quick look facility to see the heavens.

    This package includes the Java library.

    skyview.gsfc.nasa.gov/

  2. Random Astro package of the week is python3-reproject. This is a package to reproject astronomical images using various techniques via a uniform interface. Reprojection means the re-gridding of images from one world coordinate system to another (for example changing the pixel resolution, orientation, coordinate system). Currently implemented are reprojection of celestial images by interpolation, as well as by finding the exact
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  3. Random Astro package of the week is imagej. It can display, edit, analyze, process, save and print 8-bit, 16-bit and 32-bit images. It can read many image formats including TIFF, GIF, JPEG, BMP, DICOM, FITS and "raw". It supports "stacks", a series of images that share a single window.

    It can calculate area and pixel value statistics of user-defined selections. It can measure distances and angles.
    1/3⤵

  4. Random Astro package of the week is python3-pyavm. PyAVM is a module to represent, read, and write metadata following the Astronomy Visualization Metadata (AVM) standard. With pyavm you can:

    * Parse AVM meta-data from an existing image.
    * Access and Set the metadata.
    * Create an AVM object from scratch.
    * Convert to a WCS object.
    * Initialize from a FITS header.
    * Initialize from a WCS object.
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  5. Random Astro package of the week is python3-ephem. PyEphem provides an ephem Python package for performing high-precision astronomy computations. The underlying numeric routines are coded in C and are the same ones that drive the popular XEphem astronomy application, whose author, Elwood Charles Downey, generously gave permission for their use in PyEphem.

    The name ephem is short for the word ephemeris, which is the traditional
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  6. Random Astro package of the week is gdl-astrolib. The IDL Astronomy Users Library is a central repository for low-level astronomy software written in the GNU Data Language (GDL). The library is not meant to be an integrated package, but rather is a collection of procedures from which users can pick and choose (and possibly modify) for their own use. Submitted procedures are given a cursory testing, but are basically stored
    1/2⤵

  7. Random Astro package of the week is python3-vispy. Vispy is a high-performance interactive 2D/3D data visualization library.

    Vispy leverages the computational power of modern Graphics Processing Units (GPUs) through the OpenGL library to display very large datasets.

    This package provides VisPy for the Python 3 interpreter.

    vispy.org/

  8. Random Astro package of the week is iraf. IRAF is the "Image Reduction and Analysis Facility". The main IRAF distribution includes a good selection of programs for general image processing and graphics.

    Other external or layered packages are available for applications such as data acquisition or handling data from other observatories and wavelength regimes such as the Hubble Space Telescope (optical), EUVE (extreme ultra-violet), or
    1/2⤵

  9. Random Astro package of the week is scamp. SCAMP reads SExtractor catalogs and computes astrometric and photometric solutions for any arbitrary sequence of FITS images in a completely automatic way.

    astromatic.net/software/scamp

  10. Random Astro package of the week is python3-pyraf. PyRAF is a command language for running IRAF tasks in a Python like environment. It works very similar to IRAF CL, but has been updated to allow such things as importing Python modules, GUI parameter editing and help. It can be imported into Python allowing you to run IRAF commands from within a larger script.

    iraf-community.github.io/pyraf

  11. Random Astro package of the week is asdftool. ASDF (Advanced Scientific Data Format) is a proposed next generation interchange format for scientific data. ASDF aims to exist in the same middle ground that made FITS so successful, by being a hybrid text and binary format: containing human editable metadata for interchange, and raw binary data that is fast to load and use. Unlike FITS, the metadata is highly structured and is
    1/2⤵

  12. Random Astro package of the week is python3-asdf. ASDF (Advanced Scientific Data Format) is a proposed next generation interchange format for scientific data. ASDF aims to exist in the same middle ground that made FITS so successful, by being a hybrid text and binary format: containing human editable metadata for interchange, and raw binary data that is fast to load and use. Unlike FITS, the metadata is highly structured and is
    1/2⤵

  13. Random Astro package of the week is python3-drms. The drms module provides an easy-to-use Python interface for accessing HMI, AIA and MDI data with Python. It uses the publicly accessible Joint Science Operations Center (JSOC) server by default, but can also be used with local NetDRMS sites.

    The Helioseismic and Magnetic Imager (HMI) and the Atmospheric Imaging Assembly (AIA) are instruments aboard the Solar Dynamics
    1/2⤵

  14. Random Astro package of the week is python3-montagepy. MontagePy is a toolkit for assembling astronomical images into custom mosaics.

    It uses algorithms that preserve the calibration and positional (astrometric) fidelity of the input images to deliver mosaics that meet user-specified parameters of projection, coordinates, and spatial scale. It supports all projections and coordinate systems in use in
    1/2⤵

  15. Random Astro package of the week is python3-fast-histogram. fast-histogram aims to provide simple and fast histogram functions for regular bins that don't compromise on performance. It doesn't do anything complicated - it just implements a simple histogram algorithm in C and keeps it simple. The aim is to have functions that are fast but also robust and reliable. The result is a 1D histogram function here that is 7-15x faster
    1/2⤵

  16. Random Astro package of the week is python3-healpy. HEALPix is an acronym for Hierarchical Equal Area isoLatitude Pixelization of a sphere. As suggested in the name, this pixelization produces a subdivision of a spherical surface in which each pixel covers the same surface area as every other pixel. It is commonly used to store all-sky astronomical images, most famously maps of the cosmic microwave background.
    1/2⤵

  17. Random Astro package of the week is xplanet-images. Xplanet renders an image of a planet into an X window or a file.

    In order to run xplanet, you'll need at least one map file. This package includes some map files that can be used with xplanet.

    xplanet.sourceforge.net/

  18. Random Astro package of the week is python3-drizzle. The drizzle library is a Python package for combining dithered images into a single image. This library is derived from code used in drizzlepac. Like drizzlepac, most of the code is implemented in the C language. The biggest change from drizzlepac is that this code passes an array that maps the input to output image into the C code, while the drizzlepac code computes the
    1/2⤵

  19. Random Astro package of the week is python3-pysynphot. pysynphot simulates photometric data and spectra as they are observed with the Hubble Space Telescope (HST). Passbands for standard photometric systems are available, and users can incorporate their own filters, spectra, and data. pysynphot user interface allows you to:

    * Construct complicated composite spectra from various grids of model
    1/3⤵

  20. Random Astro package of the week is indi-starbook. This package contains the INDI driver for the Vixen Starbook telescope controllers. It aims for compatibility with first generation Starbook.

    This driver is compatible with any INDI client such as KStars or Xephem.

    github.com/indilib/indi-3rdpar

  21. Random Astro package of the week is libnexstar-dev. This library implements the serial commands supported by the Celestron NexStar hand control (HC) and SkyWatcher/Orion SynScan HC. This applies to the Celestron: NexStar GPS, NexStar GPS-SA, NexStar iSeries, NexStar SE Series, NexStar GT, CPC, SLT, Advanced-VX, Advanced-GT, CGE, CGEM etc. SkyWatcher: EQ5, HEQ5, EQ6 (Pro), AZ-EQ5 GT, AZ-EQ6 GT, EQ8 etc.
    1/2⤵

  22. Random Astro package of the week is fitsh. This software package provides independent binary programs (so called tasks) which performs various steps of astronomical image reduction and data processing. These tasks are designed for execution from a UNIX command line shell or shell script. Each of these tasks performs a specific operation (e.g. transforming an image to another reference frame, search and identifiy stars
    1/3⤵

  23. Random Astro package of the week is libhealpix-cxx-dev. HEALPix is an acronym for Hierarchical Equal Area isoLatitude Pixelization of a sphere. As suggested in the name, this pixelization produces a subdivision of a spherical surface in which each pixel covers the same surface area as every other pixel. It is commonly used to store all-sky astronomical images, most famously maps of the cosmic microwave background.
    1/2⤵

  24. Random Astro package of the week is python3-fitsio. Fitsio provides an easy to use object-oriented API including providing a Numpy interface to FITS files read from CFITSIO. It allows direct access to the columns of a FITS binary table which can be useful for reading large fits files. Compared to astropy.io.fits, this package is closer to the underlying cfitsio library.

    Fitsio also exposes a microlanguage (implemented in
    1/2⤵

  25. Random Astro package of the week is libastro-fits-cfitsio-perl. Astro::Fits::Cfitsio is a Perl interface to William Pence's cfitsio subroutine library. For more information on cfitsio, see heasarc.gsfc.nasa.gov/fitsio.

    This module attempts to provide a wrapper for nearly every cfitsio routine, while retaining as much cfitsio behavior as possible. As such, one should be aware that it is still somewhat
    1/2⤵

  26. Random Astro package of the week is libccfits-dev. CCfits is an object oriented interface to the cfitsio library. It is designed to make the capabilities of cfitsio available to programmers working in C++. It is written in ANSI C++ and implemented using the C++ Standard Library with namespaces, exception handling, and member template functions.

    This package contains what you need for compiling sources that use
    1/2⤵

  27. Random Astro package of the week is python3-numpy. NumPy contains a powerful N-dimensional array object, sophisticated (broadcasting) functions, tools for integrating C/C++ and Fortran code, and useful linear algebra, Fourier transform, and random number capabilities.

    This package installs NumPy for Python 3.

    numpy.org/

  28. Random Astro package of the week is casacore-dev. The casacore package contains the core libraries of the old AIPS++/CASA (Common Astronomy Software Applications) package. This split was made to get a better separation of core libraries and applications.

    This package contains the files for application development.

    casacore.github.io/casacore

  29. Random Astro package of the week is gdl-mpfit. These GDL routines provide a robust and relatively fast way to perform least-squares curve and surface fitting. The algorithms are translated from MINPACK-1, which is a rugged minimization routine found on Netlib, and distributed with permission. This algorithm is more desirable than CURVEFIT because it is generally more stable and less likely to crash than the brute-force
    1/3⤵

  30. Random Astro package of the week is libgsl-dev. The GNU Scientific Library (GSL) is a collection of routines for numerical analysis. The routines are written from scratch by the GSL team in C, and present a modern API for C programmers, while allowing wrappers to be written for very high level languages.

    This package contains the header files, static libraries and symbolic links that developers using GNU GSL will
    1/2⤵

  31. Random Astro package of the week is python3-astroml. AstroML is a Python 3 module for machine learning and data mining built on numpy, scipy, scikit-learn, and matplotlib. It contains a growing library of statistical and machine learning routines for analyzing astronomical data in Python, loaders for several open astronomical datasets, and a large suite of examples of analyzing and visualizing astronomical datasets.
    1/2⤵

  32. Random Astro package of the week is planetary-system-stacker. This package contrains software to produce a sharp image of a planetary system object (moon, sun, planets) from many seeing-affected frames using the "lucky imaging" technique._

    The program is mainly targeted at extended objects (moon, sun), but it works as well for planets. Results obtained in many tests show at least the same image quality as with the
    1/5⤵

  33. Random Astro package of the week is python3-unyt. Often writing code that deals with data that has units can be confusing. A function might return an array but at least with plain NumPy arrays, there is no way to easily tell what the units of the data are without somehow knowing a priori.

    The unyt package (pronounced like “unit”) provides a subclass of NumPy’s ndarray class that knows about units.
    1/2⤵

  34. Random Astro package of the week is skyview. SkyView is a "virtual" observatory dynamically generating images of the sky in different wavelength regimes from a static image database. SkyView is intended as a quick look facility to see the heavens.

    This package includes the executable.

    skyview.gsfc.nasa.gov/

  35. Random Astro package of the week is libccfits-dev. CCfits is an object oriented interface to the cfitsio library. It is designed to make the capabilities of cfitsio available to programmers working in C++. It is written in ANSI C++ and implemented using the C++ Standard Library with namespaces, exception handling, and member template functions.

    This package contains what you need for compiling sources that use
    1/2⤵

  36. Random Astro package of the week is libstarlink-pal-dev. This library is a collection of code designed to aid in replacing the SLA library with code from NOVAS and ERFA.

    Where possible the API is similar to the C SLA API except for the use of a "pal" prefix.

    This package contains the development files.

    starlink.eao.hawaii.edu/starli

  37. Random Astro package of the week is ser-player. The SER file format can be used to store data from fast frame rate astronomy cameras instead of using the AVI file format. This application enables users to review SER files in the same way that AVI files are reviewed with a video player.

    github.com/cgarry/ser-player

  38. Random Astro package of the week is python3-astropy-affiliated. A major part of the Astropy project is the concept of “Affiliated Packages”. An affiliated package is an astronomy-related Python package that is not part of the astropy core package, but has requested to be included as part of the Astropy project’s community. These packages are expressing an interest in Astropy’s goals of improving reuse, interoperability, and
    1/2⤵

  39. Random Astro package of the week is python3-astroalign. Astroalign is a Python module that will try to align two stellar astronomical images, especially when there is no WCS information available.

    It does so by finding similar 3-point asterisms (triangles) in both images and deducing the affine transformation between them.

    Generic registration routines try to match feature points, using corner detection routines to make the
    1/2⤵

  40. Random Astro package of the week is iraf-dev. IRAF is the "Image Reduction and Analysis Facility". The main IRAF distribution includes a good selection of programs for general image processing and graphics, plus a large number of programs for the reduction and analysis of optical and IR astronomy data.

    This package contains the IMFORT Fortran/C programming interface, and the full SPP/VOS programming environment in which the portable
    1/2⤵

  41. Random Astro package of the week is python3-pygnuplot. PyGnuplot works as a Python pipe for Gnuplot allowing to pipe commands to Gnuplot command prompt, plot, save data files, create postscript and PDF files

    This package installs the library for Python 3.

    github.com/benschneider/PyGnup

  42. Random Astro package of the week is python3-astlib. astLib is a set of Python3 modules that provides some tools for research astronomers. It can be used for astronomical plots, some statistics, common calculations, coordinate conversions, and manipulating FITS images with World Coordinate System (WCS) information through PyWCSTools - a simple wrapping of WCSTools by Jessica Mink. PyWCSTools is distributed (and developed) as
    1/2⤵

  43. Random Astro package of the week is python3-cmyt. This package provides several colormaps for the scientific use with matplotlib. It contains perceptually uniform sequential colormaps (abre, dusk, kepl, octarine), monochromatic sequential colormaps (blue, green, red) and other (algae, pastel and xray).

    github.com/yt-project/cmyt

  44. Random Astro package of the week is libstarlink-ast-dev. AST implements an object oriented model for describing physical coordinate systems, and the transformations that exist between them.

    It provides a comprehensive range of facilities for attaching world coordinate systems (WCS) to astronomical data and for retrieving and manipulating that information.

    It has built-in intelligence for identifying types of
    1/2⤵

  45. #IRAF #AstronomySoftware #ScienceSoftware

    Random #Debian Astro package of the week is iraf-xdimsum. XDIMSUM is a package for creating accurate sky subtracted images from sets of dithered observations. While the observations need not be in the infrared, the dominance of the variable sky background in infrared data requires the dithering and recombination of many short carefully sky subtracted exposures to produce deep images.

    github.com/iraf-community/iraf

  46. #IRAF #AstronomySoftware #ScienceSoftware

    Random #Debian Astro package of the week is iraf-wcstools. WCSTools is a set of software utilities, written in C, which create, display and manipulate the world coordinate system of a FITS or IRAF image, using specific keywords in the image header which relate pixel position within the image to position on the sky. Auxiliary programs search star catalogs and manipulate images.

    This package contains the IRAF package.
    1/2⤵

  47. #DebianEdu #AstronomySoftware #ScienceSoftware

    Random #Debian Astro package of the week is gpredict. Gpredict is a real time satellite tracking and orbit prediction program for the Linux desktop. It uses the SGP4/SDP4 propagation algorithms together with NORAD two-line element sets (TLE).

    Some core features of Gpredict include:

    * Tracking of a large number of satellites only limited by the physical
    memory and processing power of the computer
    1/3⤵

  48. #AstroDatareduction #AstronomySoftware #ScienceSoftware

    Random #Debian Astro package of the week is esorex. EsoRex is the European Southern Observatory (ESO) Recipe Execution Tool. It can list, configure and execute CPL-based recipes from the command line.

    The Common Pipeline Library (CPL) comprises a set of ISO-C libraries that provide a comprehensive, efficient and robust software toolkit. It forms a basis for the creation of automated astronomical data-reduction tasks.
    1/2⤵

  49. #VirtualObservatory #AstronomySoftware #ScienceSoftware

    Random #Debian Astro package of the week is jython-stilts. The STIL Tool Set is a set of command-line tools based on STIL, the Starlink Tables Infrastructure Library. It deals with the processing of tabular data; the package has been designed for, but is not restricted to, astronomical tables such as object catalogues. Some of the tools are generic and can work with multiple formats (including FITS, VOTable, CDF, CSV, SQL and
    1/2⤵

  50. #AstroPython #AstronomySoftware #ScienceSoftware

    Random #Debian Astro package of the week is python3-specreduce. The specreduce package aims to provide a data reduction toolkit for optical and infrared spectroscopy, on which applications such as pipeline processes for specific instruments can be built.

    The scope of its functionality is limited to basic spectroscopic reduction, with basic image processing steps (such as bias subtraction) instead covered by ccdproc and other packages,
    1/2⤵