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This package provides a Square Kilometre Array (SKA) Science Data Processor (SDP) function library for radio astronomy.
Event reconstruction framework for Imaging Atmospheric Cherenkov Telescopes developed for CTAO.
AOFlagger is a tool that can find and remove radio-frequency interference (RFI) in radio astronomical observations. It can make use of Lua scripts to make flagging strategies flexible, and the tools are applicable to a wide set of telescopes.
Provides DataModel, which is the base class for data models implemented in the JWST and Roman calibration software.
The Python-based Space Physics Environment Data Analysis Software (PySPEDAS) framework supports multi-mission, multi-instrument retrieval, analysis, and visualization of heliophysics time series data.
The FITS "World Coordinate System" (WCS) standard defines keywords and usage that provide for the description of astronomical coordinate systems in a FITS (Flexible Image Transport System) image header.
This package implements a functionality to read and analyze halo/galaxy catalogs (generated from Rockstar or AHF) and merger trees (generated from ConsistentTrees).
This package provides a CIANNA - a general-purpose deep learning framework primarily developed and used for astronomical data analysis.
Pynbody is an analysis framework for N-body and hydrodynamic astrophysical simulations supporting PKDGRAV/Gasoline, Gadget, Gadget4/Arepo, N-Chilada and RAMSES AMR outputs.
This package provides tools for COS.
This package implements a functionality for calibration of science observations from the Nancy Grace Roman Space Telescope.
This package provides an way to compute dendrograms of observed or simulated Astronomical data in Python.
HEALPix of a sphere produces a subdivision of a spherical surface in which each pixel covers the same surface area as every other pixel. This package provides the dynamic library for the C++ language implementation of HEALPix.
CalcMySky is a software package that simulates scattering of light by the atmosphere to render daytime and twilight skies (without stars). Its primary purpose is to enable realistic view of the sky in applications such as planetaria. Secondary objective is to make it possible to explore atmospheric effects such as glories, fogbows etc., as well as simulate unusual environments such as on Mars or an exoplanet orbiting a star with a non-solar spectrum of radiation.
This package consists of three parts:
calcmyskyutility that does the precomputation of the atmosphere model to enable rendering.libShowMySkylibrary that lets the applications render the atmosphere model.ShowMySkypreview GUI that makes it possible to preview the rendering of the atmosphere model and examine its properties.
uranimator is a CLI tool that works with your existing (code uraniborg) install to create animations. See how the sky evolves over a million years or what traveling to a star 100 light years away looks like.
ADARI (Astronomical DAta Reporting Infrastructure) is a system designed for creating graphical reports of astronomical data so that the quality of these products can be assessed. It has been designed from the ground up to be backend-agnostic, meaning the same ADARI code can be sent to a web plotting API, or a code-based plotting API, with no alteration.
pyregion is a python module to parse ds9 region files. It also supports ciao region files. Features:
ds9 and ciao region files.
(physical, WCS) coordinate conversion to the image coordinate.
convert regions to matplotlib patches.
convert regions to spatial filter (i.e., generate mask images)
qfits is a C library giving access to FITS file internals, both for reading and writing.
The Advanced Scientific Data Format (ASDF) is a next-generation interchange format for scientific data. This package contains the Python implementation of the ASDF Standard.
Astroquery is a package that contains a collection of tools to access online Astronomical data. Each web service has its own sub-package.
Python package of utility functions that are useful in analyzing various datasets, in particular, catalogs of particles or galaxies/halos from cosmological simulations.
sbpy is a package for small-body planetary astronomy. It is meant to supplement functionality provided by astropy with functions and methods that are frequently used in the context of planetary astronomy with a clear focus on asteroids and comets. Features:
observation planning tools tailored to moving objects
photometry models for resolved and unresolved observations
wrappers and tools for astrometry and orbit fitting
spectroscopy analysis tools and models for reflected solar light and emission from gas
cometary gas and dust coma simulation and analysis tools
asteroid thermal models for flux estimation and size/albedo estimation
image enhancement tools for comet comae and PSF subtraction tools
lightcurve and shape analysis tools
access tools for various databases for orbital and physical data, as well as ephemerides services
Skyfield computes positions for the stars, planets, and satellites in orbit around the Earth.
Portable library and tools for manipulating extended attributes.