Astronomy Software

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Astronomy Software

  • Find out what (or who) is slowing down your network Find out what (or who) is slowing down your network Icon
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  • Perl Data Language Icon

    Perl Data Language

    The PDL module gives standard perl the ability to COMPACTLY store and SPEEDILY manipulate the large N-dimensional data sets that are the bread and butter of scientific computing.

  • HEALPix Icon

    HEALPix

    Data Analysis, Simulations and Visualization on the Sphere

    Software for pixelization, hierarchical indexation, synthesis, analysis, and visualization of data on the sphere. Please acknowledge HEALPix by quoting the web page http://healpix.sourceforge.net and publication: K.M. Gorski et al., 2005, Ap.J., 622, p.759 Full software documentation available at http://healpix.sf.net/documentation.php Wiki Pages: https://sourceforge.net/p/healpix/wiki/Home GDL users should read https://sourceforge.net/p/healpix/wiki/HEALPix%20and%20GDL/

  • mesa Icon

    mesa

    MESA: Modules for Experiments in Stellar Astrophysics -- a set of thread-safe fortran 95 libraries for stellar astrophysics, including physics (e.g., eos, opacities, nuclear nets) and algorithms (e.g., ODE solvers). Available by svn checkout or as zip file. See project webpage (http://mesa.sourceforge.net/).

  • gnuplotfortran

    This library is a Fortran 95 gnuplot interface for some Unix like OS'es. This provides some routines that enables direct access of a child gnuplot session from a Fortran 95 program. You will need a copy of fortranposix to make this work.

  • FreeEOS

    FreeEOS is a Fortran library for calculating the equation of state using an efficient free-energy minimization technique that is suitable for physical conditions in stellar interiors.

  • MieConScat Icon

    MieConScat

    MieConScat is a GUI/Console program for generating MIE SCATtering data as a table of cross sections. It can generate scattering cross sections over specified angular ranges and total absorption cross sections. It was initially developed to aid work with optical particle counters (OPC) especially when CONverting data between cross section and diameter space. These methods are described in Rosenberg et al. 2012, Particle sizing calibration with refractive index correction for light scattering optical particle counters and impacts upon PCASP and CDP data collected during the Fennec campaign and CDP data collected during the Fennec campaign, http://www.atmos-meas-tech.net/5/1147/2012/amt-5-1147-2012.html

  • Time Ephemerides

    Calculate time ephemerides in convenient form

    Project to calculate and distribute the general relativistic corrections to clock rates for the surfaces of various solar system bodies. These corrections are also known as time ephemerides.

  • rochePlot Icon

    rochePlot

    Schematically plot the evolution of binary stars

    RochePlot is a Fortran code using PGPlot to plot a series of binaries to illustrate the key stages in the evolution of a binary star

    Downloads: 0 This Week Last Update: See Project
  • bagemass

    Bayesian age and mass estimates for transiting planet host stars

    Source code, makefile and README for installation of software used for the analysis in Maxted, Serenelli & Southworth, "Bayesian mass and age estimates for transiting exoplanet host stars", A&A 575, 36, 2015.

    Downloads: 0 This Week Last Update: See Project
  • Planck Level-S

    Sources of the simulations package for the Planck satellite project

    This project contains the sources for the simulation codes used within ESA's Planck mission (http://sci.esa.int/planck/)

    Downloads: 2 This Week Last Update: See Project
  • GPU-BH Treesolver

    The GPU-BH tree solver is a FLASH4 module to calculate the gravitational potential using a CUDA device.

    Downloads: 0 This Week Last Update: See Project
  • Morpheus Icon

    Morpheus

    MORPHEUS is a 3D MPI-OPENMP hydrodynamic simulation code

    Manchester Omni-geometRical Program for Hydrodynamical EUlerian Simulations Copyright © N. Vaytet & T. O'Brien (2008-2014) The University of Manchester Current version 1.33 - 07/2014 MORPHEUS is a 3D MPI-OPENMP Eulerian second-order Godunov hydrodynamic simulation code in cartesian, spherical and cylindrical coordinates which includes radiative cooling and gravity.

    Downloads: 1 This Week Last Update: See Project
  • Sextant

    Manuel, tables et logiciels de navigation astronomique

    Downloads: 0 This Week Last Update: See Project
  • astronx

    simulation of objects in space with classical mechanics

    astronx simulates the motion of mass-centres in cartesian space. The mass-centres interact solely through gravity. astronx uses the Bulirsch-Stoer extrapolation algorithm with adaptive stepsize to integrate the newtonian equations of motion.

    Downloads: 1 This Week Last Update: See Project
  • Sloan Digital Sky Survey: DR5 Clustering

    Data, catalogues and code for analyzing the Sloan Digital Sky Survey (SDSS) Quasar data. The resources presented here were published by Ross et al. in the Astrophysical Journal, 2009, Vol. , / .

    Downloads: 0 This Week Last Update: See Project
  • Numerical codes in stellar evolution

    Working group working in the compilation and development of tools for stellar evolution

    Downloads: 0 This Week Last Update: See Project
  • OpenSky

    A user community and inclusive package of compatible routines available to diverse astronomy users. Application services to include astronomical lab control, image processing and amateur exploration that continues to adapt to meet a wide range of needs.

    Downloads: 0 This Week Last Update: See Project
  • Easy-FITS

    The aim of this project is to provide amateur astronomers with a minimalistic set of commands to analyze FITS files.

    Downloads: 0 This Week Last Update: See Project
  • SIGPROC

    SIGPROC - a collection of signal processing programs developed for pulsar data reduction has been developed and maintained since 1999. The package is used to search for and visualize the presence of pulsed signals in noisy radio astronomy data.

    Downloads: 13 This Week Last Update: See Project
  • PSRPOP

    PSRPOP - a package to simulate radio pulsar populations has been undergoing development and use since 2003. The package is used to infer the underlying properties of pulsars and help make predictions for future surveys.

    Downloads: 0 This Week Last Update: See Project
  • ISS project

    This is a project to prove the existence of space travel by observing the international space station. This will include some history about non-believers, maths and a program to calculate the heigth and velocity of the ISS.

    Downloads: 0 This Week Last Update: See Project
  • LibppGam

    pp->gamma cross sections parametrization

    This library contains the parametrization of pp->gamma cross section functions based on Phys.Rev. D90 (2014) 12, 123014 (astro-ph/1406.7369) work. The functions are written in Python, Fortran and Matlab. Please, if you use this library DO NOT reference to this webpage, instead reference to Phys.Rev. D90 (2014) 12, 123014 (astro-ph/1406.7369), "Parametrization of gamma-ray production cross-sections for pp interactions in a broad proton energy range from the kinematic threshold to PeV energies" by Ervin Kafexhiu, Felix Aharonian, Andrew M. Taylor, Gabriela S. Vila

    Downloads: 0 This Week Last Update: See Project
  • RT: Radiative Transfer

    RT is the world's fastest and most accurate simulation of astrophysical radiative transfer. RT includes C++ implementations of the Mersenne Twister and R250/521 RNGs, and the best-known BSP traversal algorithm.

    Downloads: 0 This Week Last Update: See Project
  • Digest2 Statistical Ranging

    Note: This project is no longer maintained. A newer version of the program is at https://code.google.com/p/digest2/. Statistical ranging for short arc moving object astrometry. Accepts atstrometry in MPC 80 charcater observation format, rates objects on likelyhood that they are yet-unknown near Earth objects.

    Downloads: 1 This Week Last Update: See Project
  • PARAMESH

    PARAMESH is a package of Fortran 90 subroutines designed to provide an application developer with an easy route to extend an existing serial code which uses a logically cartesian structured mesh into a parallel code with adaptive mesh refinement(AMR).

    Downloads: 4 This Week Last Update: See Project
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