Enter the query into the form above. You can look for specific version of a package by using @ symbol like this: gcc@10.
API method:
GET /api/packages?search=hello&page=1&limit=20
where search is your query, page is a page number and limit is a number of items on a single page. Pagination information (such as a number of pages and etc) is returned
in response headers.
If you'd like to join our channel webring send a patch to ~whereiseveryone/toys@lists.sr.ht adding your channel as an entry in channels.scm.
The ccdproc package provides many of the necessary tools for processing of CCD images built on a framework to provide error propagation and bad pixel tracking throughout the reduction process.
The concept of the pvextractor package is simple - given a path defined in sky coordinates, and a spectral cube, extract a slice of the cube along that path, and along the spectral axis, producing a position-velocity or position-frequency slice.
Glue is a python project to link visualizations of scientific datasets across many files.
This package provides ASDF schemas for validating FITS tags.
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.
This package implement functionality for computation of non-thermal radiation from relativistic particle populations. It includes tools to perform MCMC fitting of radiative models to X-ray, GeV, and TeV spectra using emcee, an affine-invariant ensemble sampler for Markov Chain Monte Carlo.
This package provides shared libraries to interface Pascal program with standard astronomy libraries:
libpasgetdss.so: Interface with GetDSS to work with DSS images.libpasplan404.so: Interface with Plan404 to compute planets position.libpaswcs.so: Interface with libwcs to work with FITS WCS.libpasspice.so: To work with NAIF/SPICE kernel.
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.
This package provides data content for Celestia.
Scientific Data Base
Texture maps
3D Models
SPLASH is visualisation tool for Smoothed Particle Hydrodynamics (SPH) simulations in one, two and three dimensions, developed mainly for astrophysics. It uses a command-line menu but data can be manipulated interactively in the plotting window.
qfits is a C library giving access to FITS file internals, both for reading and writing.
The DKIST package aims to help you search, obtain and use DKIST data as part of your Python software.
radiospectra provides support for some type of radio spectra in solar physics.
This package contains FIT and CSV files required for WebbPSF installation and distributed separately from it.
LibXISF is C++ library that can read and write XISF files produced by PixInsight. It implements XISF 1.0 specification.
PyVO is a package providing access to remote data and services of the Virtual observatory (VO) using Python.
EsoRex is the European Southern Observatory Recipe Execution Tool. It can list, configure and execute Common Pipeline Library-based recipes from the command line.
Astrocut provides tools for making cutouts from sets of astronomical images with shared footprints. It is under active development.
Three main areas of functionality are included:
solving the specific problem of creating image cutouts from sectors of Transiting Exoplanet Survey Satellite full-frame images
general fits file cutouts including from single images and sets of images with the shared WCS/pixel scale
cutout post-processing functionality, including centering cutouts along a path (for moving targets) and combining cutouts
UNSIO provides an API for performing input and output operations on different kinds of n-body file formats (nemo, Gadget binaries 1 and 2, Gadget hdf5, Ramses).
PHD2 is the enhanced,second generation version of the PHD guiding software from Stark Labs.
PyEsoRex is a command line tool which can serve as a drop-in replacement of EsoRex, which can execute both, existing pipeline recipes implemented using the Common Pipeline Library C API, and recipes implemented using the PyCPL Python API.
APLpy is a Python module aimed at producing publication-quality plots of astronomical imaging data in FITS format. The module uses matplotlib, a powerful and interactive plotting package. It is capable of creating output files in several graphical formats, including EPS, PDF, PS, PNG, and SVG.
Main features:
Make plots interactively or using scripts
Show grayscale, colorscale, and 3-color RGB images of FITS files
Generate co-aligned FITS cubes to make 3-color RGB images
Make plots from FITS files with arbitrary WCS (e.g. position-velocity)
Slice multi-dimensional FITS cubes
Overlay any number of contour sets
Overlay markers with fully customizable symbols
Plot customizable shapes like circles, ellipses, and rectangles
Overlay ds9 region files
Overlay coordinate grids
Show colorbars, scalebars, and beams
Customize the appearance of labels and ticks
Hide, show, and remove different contour and marker layers
Pan, zoom, and save any view as a full publication-quality plot
Save plots as EPS, PDF, PS, PNG, and SVG
The package statmorph implements functionality of calculating non-parametric morphological diagnostics of galaxy images (e.g., Gini-M_20 and CAS statistics), as well as fitting 2D Sérsic profiles.