Search found 1901 matches

by Ada Coda
Wed Dec 01, 2021 9:00 am
Forum: Astrophysics Source Code Library
Topic: Caustic Mass Estimator for Galaxy Clusters
Replies: 0
Views: 12

Caustic Mass Estimator for Galaxy Clusters

Caustic Mass Estimator for Galaxy Clusters [/b] Abstract : The caustic technique is a powerful method to infer cluster mass profiles to clustrocentric distances well beyond the virial radius, by measuring the escape velocity of the sistem using only galaxy redshift information. This code allows the...
by Ada Coda
Wed Dec 01, 2021 4:11 am
Forum: Astrophysics Source Code Library
Topic: GWToolbox: Gravitational wave observation simulator
Replies: 0
Views: 22

GWToolbox: Gravitational wave observation simulator

GWToolbox: Gravitational wave observation simulator [/b] Abstract : GWToolbox simulates gravitational wave observations for various detectors. The package is composed of three modules, namely the ground-based detectors (and their targets), the space-borne detectors (and their targets) and pulsar ti...
by Ada Coda
Wed Dec 01, 2021 3:24 am
Forum: Astrophysics Source Code Library
Topic: pySYD: Measuring global asteroseismic parameters
Replies: 0
Views: 24

pySYD: Measuring global asteroseismic parameters

pySYD: Measuring global asteroseismic parameters [/b] Abstract : pySYD detects solar-like oscillations and measures global asteroseismic parameters. The code is a python-based implementation of the IDL-based SYD pipeline by Huber et al. (2009), which was extensively used to measure asteroseismic pa...
by Ada Coda
Wed Dec 01, 2021 2:47 am
Forum: Astrophysics Source Code Library
Topic: SteParSyn: Stellar atmospheric parameters using the spectral synthesis method
Replies: 0
Views: 20

SteParSyn: Stellar atmospheric parameters using the spectral synthesis method

SteParSyn: Stellar atmospheric parameters using the spectral synthesis method [/b] Abstract : SteParSyn infers stellar atmospheric parameters (Teff, log g, [Fe/H], and Vbroad) of FGKM-type stars using the spectral synthesis method. The code uses the MCMC sampler emcee (ascl:1303.002) in conjunction...
by Ada Coda
Wed Dec 01, 2021 2:29 am
Forum: Astrophysics Source Code Library
Topic: gCMCRT: 3D Monte Carlo Radiative Transfer for exoplanet atmospheres using GPUs
Replies: 0
Views: 22

gCMCRT: 3D Monte Carlo Radiative Transfer for exoplanet atmospheres using GPUs

gCMCRT: 3D Monte Carlo Radiative Transfer for exoplanet atmospheres using GPUs [/b] Abstract : gCMCRT globally processes 3D atmospheric data, and as a fully 3D model, it avoids the biases and assumptions present when using 1D models to process 3D structures. It is well suited to performing the post...
by Ada Coda
Wed Dec 01, 2021 1:35 am
Forum: Astrophysics Source Code Library
Topic: UniMAP: Unicorn Multi-window Anomaly Detection Pipeline
Replies: 0
Views: 22

UniMAP: Unicorn Multi-window Anomaly Detection Pipeline

UniMAP: Unicorn Multi-window Anomaly Detection Pipeline [/b] Abstract : The data analysis UniMAP (Unicorn Multi-window Anomaly Detection Pipeline) leverages the Temporal Outlier Factor (TOF) method to find anomalies in LVC data. The pipeline requires a target detector and a start and stop GPS time ...
by Ada Coda
Wed Dec 01, 2021 1:12 am
Forum: Astrophysics Source Code Library
Topic: Astrosat: Satellite transit calculator
Replies: 0
Views: 21

Astrosat: Satellite transit calculator

Astrosat: Satellite transit calculator [/b] Abstract : Astrosat calculates which satellites can be seen by a given observer in a given field of view at a given observation time and observation duration. This includes the geometry of the satellite and observer but also estimates the expected apparen...
by Ada Coda
Wed Dec 01, 2021 1:01 am
Forum: Astrophysics Source Code Library
Topic: flatstar: Make 2d intensity maps of limb-darkened stars
Replies: 0
Views: 25

flatstar: Make 2d intensity maps of limb-darkened stars

flatstar: Make 2d intensity maps of limb-darkened stars [/b] Abstract : flatstar is an open-source Python tool for drawing stellar disks as numpy.ndarray objects with scientifically-rigorous limb darkening. Each pixel has an accurate fractional intensity in relation to the total stellar intensity o...
by Ada Coda
Wed Dec 01, 2021 1:01 am
Forum: Astrophysics Source Code Library
Topic: p-winds: Python implementation of Parker wind models for planetary atmospheres
Replies: 0
Views: 23

p-winds: Python implementation of Parker wind models for planetary atmospheres

p-winds: Python implementation of Parker wind models for planetary atmospheres [/b] Abstract : p-winds produces simplified, 1-D models of the upper atmosphere of a planet and performs radiative transfer to calculate observable spectral signatures. The scalable implementation of 1D models allows for...
by Ada Coda
Wed Dec 01, 2021 12:22 am
Forum: Astrophysics Source Code Library
Topic: Nii: Multidimensional posterior distributions framework
Replies: 0
Views: 21

Nii: Multidimensional posterior distributions framework

Nii: Multidimensional posterior distributions framework [/b] Abstract : Nii implements an automatic parallel tempering Markov chain Monte Carlo (APT-MCMC) framework for sampling multidimensional posterior distributions and provides an observation simulation platform for the differential astrometric...