HEASoft offers an Aladdin?s chest of astronomy software. It is a unified release of FTOOLS and XANADU. OSSBlog hot
INDI is the Instrument-Neutral-Distributed-Interface control protocol. INDI has many advantages including loose coupling between hardware devices and software drivers. Clients that use the device drivers (like KStars) are completely unaware of the device capabilities. In run time, clients communicate with the device drivers and build a completely dynamical GUI based on services provided by the device. Therefore, new device drivers can be written or updated and clients can take full advantage of them without any changes on the client side. hot
abaverify a Python package built on unittest for running verification tests on Abaqus user subroutines.
Airborne Coordinated Conflict Resolution and Detection (ACCoRD) is a framework for the formal specification and verification of state-based conflict detection and resolution algorithms. ACCoRD originates from KB3D, a state-based conflict detection and resolution algorithm.
Apollo-11 is the original Apollo 11 Guidance Computer (AGC) source code for the command and lunar modules.
AstroAviBrowser is a small tool for astronomy imaging capture/treatment. It allows you to open a video file, select the good frames, and save the new sequence in a new video file using the desired codec.
astrofocuser is a very simple tool written with Qt 4.5 to help star focusing in astrophotogaphy. This tool applies an FWHM by transparency on the background window.
astromake is a utility intended to make installations of some common astronomical packages (in binary form) easy. In practice it is a shell script that with the aid of makefiles wraps around rpm's, tarballs and debian packages, currently the three most common package formats.
AstroMD is a visualization package developed in the Cosmo.Lab framework with the specific object of supporting visualization and analysis of astrophysical three dimensional structures. Astrophysical data, in fact, have peculiarities that make them different from data coming from any other kind of simulation or experiment. Therefore they require a specific treatment.
Astropy is a package intended to contain much of the core functionality and some common tools needed for performing astronomy and astrophysics with Python.
Astronomical Python - Promoting the Development & Use of the Python Programming Language in Astronomical Research
Audela is an astrophotography application developed in TCL. The software lets users capture and process images, control telescopes and includes a rather special tool called SpcAudace, which adds advanced spectroscopy. What also sets the software apart is the ability to customize the application using simple scripts, although this involves learning the TCL/Tk language, which may be unfamiliar with many users. OSSBlog
BOTEC is a simple astrophysical and orbital mechanics calculator, including a database of all named Solar System objects.
Colorspec takes as input a digital spectrum ASCII file, space delimited in two columns with wavelength from low to high in Angstroms and relative flux in any units. It produces by default an 800x50 PPM format 24-bit RGB image which can be displayed by most image viewers, and modified as needed or converted to other formats with image processing programs such as Gimp.
The CEOS Data Cube Platform is a data processing platform for Earth science data, with a focus on remote-sensing data.
Desktop Exploration of Remote Terrain (DERT) is a software tool for exploring large Digital Terrain Models (DTM) in 3D. It aids in understanding topography and spatial relationships of terrain features, as well as performing simple analysis tasks relevant to the planetary science community.
dnppy is a collection of functions and classes for download, format, and analysis of NASA satelite data and anciliary NOAA datasets.
EPIC Variability Extraction and Removal for Exoplanet Science Targets: A pipeline for de-trending K2 light curves with pixel level decorrelation and Gaussian processes.
Exoflight is a spaceflight simulator. The player can fly several space vehicles and rockets, travel to the bodies of the solar system, and complete a variety of missions. It includes several spacecraft from history and the future, including the Apollo spacecraft, Saturn V, and Space Shuttle.
fewbody is a software package for doing small-N scattering experiments, licensed under the GNU GPL. "fewbody" can handle an arbitrary number of stars, and understands arbitrarily large hierarchies.
Gimp Astronomy Plugins
Gimp Astronomy Plugins are intended to be useful for astronomical image processing.
glnemo is an interactive visualization program for snapshots, based on the Qt library from Trolltech. You can zoom in/out, rotate, scale, translate, save a screenshot, select different particles and plot them in different blending colors.
Global Village is a GNOME application designed to place a GUI onto the CLI interface of Xplanet.
The General Mission Analysis Tool (GMAT) is an open-source space mission analysis tool for mission analysis and trajectory optimization, estimation, and prediction. The technology can be used to design spacecraft trajectories, optimize maneuvers, perform orbit determination, visualize and communicate mission parameters, and understand a mission's trade space.
Gnome Predict is a satellite tracking program for Gnome.
GoQat is a hardware control and data acquisition program for astronomy on the Linux platform. It has an INDI client to control any device with an INDI driver and has native support for any CCD camera from Quantum Scientific Imaging and any Starlight Xpress USB 2.0 camera. It can also control Starlight Xpress filter wheels.
GRALE is a library to model gravitational lenses and invert gravitational lens systems based on the observed images.
Henry is an educational astrometry utility for performing calculations based on a Hertzsprung-Russel (H-R) diagram, such as spectroscopic parallax for working out the distance to a given star. Unlike many other solutions that use in-built images for their H-R diagrams, Henry plots data directly from the European Space Agency's HIPPARCOS catalog, allowing increased accuracy while also giving students greater room to experiment by exploring the catalogue themselves.
ICAROUS (Integrated Configurable Algorithms for Reliable Operations of Unmanned Systems) is a software architecture that enables the robust integration of mission specific software modules and highly assured core software modules for building safety-centric autonomous unmanned aircraft applications.
K2 Planet search
K2 Planet search (k2ps) searches for transit-like signals from the k2sc-detrended light curves.
K2ephem is a Python package that allows to check whether a Solar System body, i.e. a moving asteroid or comet, falls within the field of view of a K2 campaign.
K2fov checks whether targets are in the field of view of NASA's K2 mission.
Kadenza converts raw cadence data from the Kepler spacecraft into astronomer-friendly FITS files. Kadenza allows the raw cadence pixel data from the Kepler space telescope to be inspected as soon as they arrive on Earth; bypassing the (time-consuming) standard pipeline processing to enable time-critical data analyses to be carried out quickly.
KAstrometry is for the KDE Desktop Environment. It is written in Python. It aims to be a good tool to make measurements of objects in space from images taken by CCD cameras. Such measurements might be used to find orbits of astroids or record the brightness of variables stars.
ketu helps the search for transiting exoplanets.
kplr is a Python interface to the Kepler data.
ktransit is a simple exoplanet transit modeling tool in Python. It contains routines to create and/or fit a transiting planet model.
Lxnstack is a program designed to align and stack astronomical images (both planetary and deep-sky).
The Memory Manager application (MM) is a core Flight System (cFS) application that is a plug in to the Core Flight Executive (cFE) component of the cFS.
Moon Tool displays information about the current state of the moon and sun.
moontool displays an icon with the current phase of the Moon on an OpenLook or SunView screen.
The Neo-Geography Toolkit (NGT) is a collection of tools for automated processing of geospatial data, including images and maps. It is capable of processing raw raster data from remote sensing instruments and transforming it into useful cartographic products, such as visible image base maps and topographic models. Components of the NGT can perform data processing on extremely large geospatial data sets (up to several tens of terabytes) via parallel processing pipelines.
OnEarth is a software package consisting of image formatting and serving modules which facilitate the deployment of a web service capable of efficiently serving standards-based requests for georeferenced raster imagery at multiple spatial resolutions including, but not limited to, full spatial resolution.
partiview is a program that enables you to visualize and animate particle data. partiview runs on relatively simple desktops and laptops, but is mostly compatible with its big brother VirDir.
PHD2 is a telescope guiding software tool for astro-photographers. It is a well-polished application and has both beginner and experienced friendly features combined with a good set of visualization tools. OSSBlog
pngphoon is intended as a successor to xphoon. It draws the actual phase of the moon into a png file for desktop integration.
PolyCARP (Algorithms and Software for Computations with Polygons) is a package of algorithms, implemented in Java, C++, and Python, for computing containment, collision, resolution, and recovery information for polygons.
PyKE ia a suite of Python/PyRAF tools to analyze Kepler data.
PyNOVAS offers a collection of functions and applications for calculating the positions of the sun, moon, planets and other celestial objects.
radial calculates the radial velocities of both stars in a binary system.
SAOimage is a utility for displaying astronomical images in the X11 window environment. It was written at the Smithsonian Astrophysical Observatory by Mike Van Hilst in 1990 and is now maintained by Doug Mink. Image files can be read directly, or image data may be passed through a named pipe (Unix) or a mailbox (VMS) from IRAF display tasks.
Satellitarium is a graphical application that predicts the position of artificial satellites and displays them against the sky background.
Siril is an image processing tool specially tailored for noise reduction and improving the signal/noise ratio of an image from multiple captures, as required in astronomy. Siril can align, stack and enhance pictures from various file formats, even image sequences (movies and SER files). OSSBlog
SkyDome is a tool to demonstrate the location of stars, planets, constellations, and the Milky Way during Earth's rotation. Besides the optical view, various other star maps are incorporated from satellites like COBE, EGRET, and IUE, making the multi-wavelength Milky Way visible to the user.
SkyViewer is an OpenGL-based program written by Nicholas Phillips to display HEALPix-based sky maps from FITS format files. The program will display sky maps on a 3D sphere or a 2D Mollweide projection. Real time panning and zooming are supported, as are rotations of the 3D sphere (if you have a fast graphics card).
Solar reads a line list from the Moore Tables of the Rowland Atlas of the Sun and creates a spectrum based on the wavelength and equivalent width of the tabulated features. It is useful for creating illustrations of spectra that have selected lines.
SolarBeam is a desktop application for drawing solar diagrams. You supply the geographical position, and it draws a diagram showing the Sun's trajectory over your location at various times of the year. It also shows the times of sunrise and sunset.
Starbase is a set of filter programs and an ascii table format for UNIX. The current release contains over 95 programs for manipulating data tables.
Starblinker allows you to easily search for new stars in your astronomical photos.
SunSky uses the Utah sun/sky model to draw plots
of the entire sky, or a specific window of the sky, for a given location, time, and view
The TABLES package sits alongside STSDAS and provides tools and libraries for working with tabular data.
TRIP is a general computer algebra system dedicated to celestial mechanics. It includes a numerical kernel and has interfaces to gnuplot and xmgrace.
Visual Environment for Remote Virtual Exploration (VERVE) is a collection of software components for visualizing, monitoring, and commanding robots in remote environments. VERVE is developed by the Intelligent Robotics Group at NASA Ames Research Center and is part of the NASA Ensemble software ecosystem.
Viewpoints (vp) is a visualization tool for exploring large, multidimensional data. It enables rapid interactive analysis of data sets containing >> 106 samples, limited only by available RAM, with an arbitrary number of attributes (or dimensions) per sample.
Virtual Moon Atlas
Virtual Moon Atlas is a program that allows users to observe and study the moon and its surface. It can visualize the Moon aspect for every date and hour and pilot computerized telescopes on the Moon surface. Read more
WIP is an interactive package with a simple to use command line user interface used to produce high quality graphical output. WIP was developed as part of the Berkeley-Illinois-Maryland Association (BIMA) project.
wmJupiter shows you the actual distance of Jupiter in astronomical units (AE) and when the red spot crosses (which is a weather feature on jupiter).
wmSolar shows you the solar system viewed from top (90° heliocentric).
Xphoon sets the root window image to a picture of the moon in its current phase.