#AstroDatareduction #AstronomySoftware #ScienceSoftware
Random #Debian 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.
#IRAF #AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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.
#AstroTools #AstronomySoftware #ScienceSoftware
Random #Debian 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
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#AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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
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#AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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
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#SciencePublication #AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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
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#AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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
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#AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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.
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#DebianEdu #AstronomySoftware #ScienceSoftware
Random #Debian 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.
#AstroPython #AstronomySoftware #ScienceSoftware
Random #Debian 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
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Debian Astro