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 glue-astronomy plugin for glue provides a collection of astronomy-specific functionality
Weightwatcher is a program hat combines weight-maps, flag-maps and polygon data in order to produce control maps which can directly be used in astronomical image-processing packages like Drizzle, Swarp or SExtractor.
This package provides ALFA, which can identify and fit hundreds of lines in emission line spectra in just a few seconds with following features:
A population of synthetic spectra is generated using a reference line catalogue.
The goodness of fit for each synthetic spectrum is calculated. The best sets of parameters are retained and the rest discarded.
A new population of synthetic spectra is obtained by averaging pairs of the best performers.
A small fraction of the parameters of the lines in the new generation are randomly altered.
The process repeats until a good fit is obtained.
SunPy is package for solar physics and is meant to be a free alternative to the SolarSoft data analysis environment.
Astro-SCRAPPY is designed to detect cosmic rays in images (numpy arrays), based on Pieter van Dokkum's L.A.Cosmic algorithm. Much of this was originally adapted from cosmics.py written by Malte Tewes. This is designed to be as fast as possible so some of the readability has been sacrificed, specifically in the C code.
pixell is a library for loading, manipulating and analyzing maps stored in rectangular pixelization. It is mainly intended for use with maps of the sky (e.g. CMB intensity and polarization maps, stacks of 21 cm intensity maps, binned galaxy positions or shear) in cylindrical projection, but its core functionality is more general.
STPSF produces simulated PSFs for the James Webb Space Telescope, NASA's flagship infrared space telescope. STPSF can simulate images for any of the four science instruments plus the fine guidance sensor, including both direct imaging, coronagraphic, and spectroscopic modes.
Python Tools for HST ACS (Advanced Camera for Surveys) Data.
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.
EsoRex is the European Southern Observatory Recipe Execution Tool. It can list, configure and execute Common Pipeline Library-based recipes from the command line.
Python read-only implementation of the EventIO file format.
European Southern Observatory Data Processing System EDPS is a system to automatically organise data from ESO instruments for pipeline processing and running the pipeline on these data. It is used for quality control at ESO. The current public release is a beta version without a GUI. A GUI is being developed and the system is meant to eventually replace the older EsoReflex environment.
Glue is a python project to link visualizations of scientific datasets across many files.
Multidimensional data visualization across files.
This package provides ASDF schemas for validating transform tags. Users should not need to install this directly; instead, install an implementation package such as asdf-astropy.
Halotools is a specialized python package for building and testing models of the galaxy-halo connection, and analyzing catalogs of dark matter halos. The core feature of Halotools is a modular platform for creating mock universes of galaxies starting from a catalog of dark matter halos obtained from a cosmological simulation.
Radio Beam is a simple toolkit for reading beam information from FITS headers and manipulating beams. Some example applications include:
Convolution and deconvolution
Unit conversion (Jy to/from K)
Handle sets of beams for spectral cubes with varying resolution between channels
Find the smallest common beam from a set of beams
Add the beam shape to a matplotlib plot
PyCPL provides Python3 language bindings for the complete programming API of the European Southern Observatory Common Pipeline Library toolkit, including the CPL plugin interface.
This package contains FIT and CSV files required for WebbPSF installation and distributed separately from it.
This package provides HEALPix to the Astropy project.
CFITSIO provides simple high-level routines for reading and writing Flexible Image Transport System files that insulate the programmer from the internal complexities of the FITS format. CFITSIO also provides many advanced features for manipulating and filtering the information in FITS files.
Python package for making visuals of gravitational wave signals, specifically pulsar timing array signals.
This package provides ASDF schemas for validating coordinates tags. Users should not need to install this directly; instead, install an implementation package such as asdf-astropy.
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.