ASCL.net

Spectractor: spectrum extraction tool for slitless spectrophotometry [/b] Abstract : The goal of Spectractor is to extract spectra from slitless spectrophotometric images, and then to measure the atmospheric transmission on the line of sight if standard stars are targetted. It has been optimized on...

Hilal-Obs: Authentication agorithm for new moon visibility report [/b] Abstract : Hilal-Obs authenticates lunar crescent first visibility reports. The code, written in Python, uses PyEphem (ascl:1112.014) for astrometrics, and takes into account all the factors that affect lunar crescent visibility...

Librarian: The HERA Librarian [/b] Abstract : The HERA Librarian system keeps track of all the primary data products for the telescope at a given site. The Librarian supports large data volumes and automated data processing capabilities. A web-based application handles human user and automatic requ...

hera_opm: The HERA Online Processing Module [/b] Abstract : The hera_opm package provides a convenient and flexible framework for developing data analysis pipelines for operating on a sequence of input files. Though developed for application to the Hydrogen Epoch of Reionization Array (HERA), it is...

CARTA: Cube Analysis and Rendering Tool for Astronomy [/b] Abstract : CARTA (Cube Analysis and Rendering Tool for Astronomy) is a image visualization and analysis tool designed for the ALMA, VLA, SKA pathfinders, and the ngVLA. If offers catalog support, shared region analytics, profile smoothing, ...

DIAPHANE: Library for radiation and neutrino transport in hydrodynamical simulations [/b] Abstract : DIAPHANE provides a common platform for application-independent radiation and neutrino transport in astrophysical simulations. The library contains radiation and neutrino transport algorithms for mo...

SparseBLS: Box-Fitting Least Squares implementation for sparse data [/b] Abstract : SparseBLS uses the Box-fitting Least Squares (BLS) algorithm to detect transiting exoplanets in photometric data. SparseBLS does not bin data into phase bins and does not use a phase grid. Because its detection effi...

Astro-Fix: Correcting astronomical bad pixels in Python [/b] Abstract : astrofix is an astronomical image correction algorithm based on Gaussian Process Regression. It trains itself to apply the optimal interpolation kernel for each image, performing multiple times better than median replacement an...

GalLenspy: Reconstruction of mass profile in disc-like galaxies from the gravitational lensing effect [/b] Abstract : Gallenspy uses the gravitational lensing effect (GLE) to reconstruct mass profiles in disc-like galaxies. The algorithm inverts the lens equation for gravitational potentials with s...

PyPion: Post-processing code for PION simulation data [/b] Abstract : PyPion reads in Silo (ascl:2103.025) data files from PION (ascl:2103.024) simulations and plots the data. This library works for 1D, 2D, and 3D data files and for any amount of nested-grid levels. The scripts contained in PyPion ...