Search found 1883 matches

by Ada Coda
Wed Sep 29, 2021 10:51 pm
Forum: Astrophysics Source Code Library
Topic: GLoBES: General Long Baseline Experiment Simulator
Replies: 0
Views: 3681

GLoBES: General Long Baseline Experiment Simulator

GLoBES: General Long Baseline Experiment Simulator [/b] Abstract : GLoBES simulates long baseline neutrino oscillation experiments. The package features full incorporation of correlations and degeneracies in the oscillation parameter space, advanced routines for the treatment of arbitrary systemati...
by Ada Coda
Wed Sep 29, 2021 10:50 pm
Forum: Astrophysics Source Code Library
Topic: HTOF: Astrometric solutions for Hipparcos and Gaia intermediate data
Replies: 0
Views: 3712

HTOF: Astrometric solutions for Hipparcos and Gaia intermediate data

HTOF: Astrometric solutions for Hipparcos and Gaia intermediate data [/b] Abstract : HTOF parses the intermediate data from Hipparcos and Gaia and fits astrometric solutions to those data. It computes likelihoods and parameter errors in line with the catalog and can reproduce five, seven, and nine ...
by Ada Coda
Wed Sep 29, 2021 10:50 pm
Forum: Astrophysics Source Code Library
Topic: SkyPy: Simulating the astrophysical sky
Replies: 0
Views: 3686

SkyPy: Simulating the astrophysical sky

SkyPy: Simulating the astrophysical sky [/b] Abstract : SkyPy simulates the astrophysical sky. It provides functions that sample realizations of sources and their associated properties from probability distributions. Simulation pipelines are constructed from these models, while task scheduling and ...
by Ada Coda
Wed Sep 29, 2021 8:00 pm
Forum: Astrophysics Source Code Library
Topic: unpopular: Using CPM detrending to obtain TESS light curves
Replies: 0
Views: 3732

unpopular: Using CPM detrending to obtain TESS light curves

unpopular: Using CPM detrending to obtain TESS light curves [/b] Abstract : unpopular is an implementation of the Causal Pixel Model (CPM) de-trending method to obtain TESS Full-Frame Image (FFI) light curves. The code, written in Python, models the systematics in the light curves of individual pix...
by Ada Coda
Wed Sep 29, 2021 7:59 pm
Forum: Astrophysics Source Code Library
Topic: HSS: The Hough Stream Spotter
Replies: 0
Views: 3711

HSS: The Hough Stream Spotter

HSS: The Hough Stream Spotter [/b] Abstract : The Hough Stream Spotter (HSS) is a stream finding code which transforms individual positions of stars to search for linear structure in discrete data sets. The code requires only the two-dimensional plane of galactic longitude and latitude as input. Cr...
by Ada Coda
Wed Sep 29, 2021 7:59 pm
Forum: Astrophysics Source Code Library
Topic: WimPyDD: WIMP direct–detection rates predictor
Replies: 0
Views: 3697

WimPyDD: WIMP direct–detection rates predictor

WimPyDD: WIMP direct–detection rates predictor [/b] Abstract : WimPyDD calculates accurate predictions for the expected rates in WIMP direct–detection experiments within the framework of Galilean–invariant non–relativistic effective theory. The object–oriented customizable Python code handles diffe...
by Ada Coda
Wed Sep 29, 2021 7:59 pm
Forum: Astrophysics Source Code Library
Topic: STAR-MELT: STellar AccrRtion Mapping with Emission Line Tomography
Replies: 0
Views: 2781

STAR-MELT: STellar AccrRetion Mapping with Emission Line Tomography

STAR-MELT: STellar AccrRetion Mapping with Emission Line Tomography [/b] Abstract : STAR-MELT extracts and identifies emission lines from FITS files by matching to a compiled reference database of lines. Line profiles are fitted and quantified, allowing for calculations of physical properties acros...
by Ada Coda
Wed Sep 29, 2021 6:16 pm
Forum: Astrophysics Source Code Library
Topic: Rubble: Simulating dust size distributions in protoplanetary disks
Replies: 0
Views: 2402

Rubble: Simulating dust size distributions in protoplanetary disks

Rubble: Simulating dust size distributions in protoplanetary disks [/b] Abstract : Rubble implicitly models the local evolution of dust distributions in size, mass, and surface density by solving the Smoluchowski equation (also known as the coagulation-fragmentation equation) under given disk condi...
by Ada Coda
Wed Sep 29, 2021 1:48 am
Forum: Astrophysics Source Code Library
Topic: Frankenstein: Flux reconstructor
Replies: 0
Views: 1107

Frankenstein: Flux reconstructor

Frankenstein: Flux reconstructor [/b] Abstract : Frankenstein (frank) fits the 1D radial brightness profile of an interferometric source given a set of visibilities. It uses a Gaussian process that performs the fit in <1 minute for a typical protoplanetary disc continuum dataset. Frankenstein can p...
by Ada Coda
Wed Sep 29, 2021 1:48 am
Forum: Astrophysics Source Code Library
Topic: pyFFTW: python wrapper around FFTW
Replies: 0
Views: 802

pyFFTW: python wrapper around FFTW

pyFFTW: python wrapper around FFTW [/b] Abstract : pyFFTW is a pythonic wrapper around FFTW (ascl:1201.015), the speedy FFT library. Both the complex DFT and the real DFT are supported, as well as on arbitrary axes of arbitrary shaped and strided arrays, which makes it almost feature equivalent to ...