K-Track is an graphical satellite prediction Program that runs under KDE. It's really accurate as it calculates using the NORAD SGP4/SDP4 Models. It Controls your Rig for doppler compensation / antenna pointing
Very simple web-interfase for astrospectrograph
Videoguide allows you to correct star position in case of bad guiding system of telescope. Here is software for videoguide, hardware part consists of PIC-ruled step motors, which tilt a glass plate, correcting by this tilt position of a star or other object. The guiding object is selected by operator in a part of video from gude's CCD-camera. Selected area can be preprocessing by wavelet-filter or median filter and/or histogram equalisation.
AEPHEM is an astronomical ephemeris and reduction C library. It is compatible with JPL ephemerides. It has routines for the standard astrometric reductions, conversions between different time standards and transformations between coordinate systems.
AGBStarViewer is a best fit and plotting SW for AGB-star spectra.
AGBStarViewer is an astronomical SW which was developed as a part of my Master Thesis at the University of Vienna. It is designed to compare star spectra and obtain best fits of many hundreds spectra. Licence: GPLv2
A framework of drivers on which generic astronomical applications can be built.
AQUYNZA is a set of C++ libraries, sample programs and doc's for the modelling, visualization and persistence of 3D environments. Its modular and highly portable. Its primary objective is helping to learn (and teach) computer graphics. (code in SPANISH)!
Drivers and applications for the range of Scientific CCD cameras produced by Apogee Instruments Inc. Both ISA and Parallel interfaces are supported. A high level library and GUI are provided for Astronomical applications.
Astronomy program using Eclipse RCP.
Control Applications for Astronomical CCD Cameras
Application for logging, planning, and searching astronomy observations. Written in Python/Tkinter with support for xmlrpc/SOAP as a secondary goal.
Astronomy computing for educational purpose
For nearly a decade Skype and Telescope Magazine provided small BASIC programs demonstrating astronomy computing for educational and inspirational purpose. This project is an inspiration of those programs, using not only BASIC, but any programming language in which it may be fun using.
The 'BandSystem' spectral analysis system is a rule-based system for the classification of mineral spectra. It consists of a preprocessor, a feature extractor, and a rule-based system to identify minerals from infra-red reflectance spectra.
A bash script that allows Seti @ Home users to queue up and process multiple work units. This means you don't have to connect to the seti servers after every work unit, and only when you want to.
CELUI Is a general purpose C++ OpenGL cross-platform GUI framework that allows to create animated and rich user interfaces for simulations and games.
Code to produce models of white dwarf stars
ChandraWD solves the hydrostatic equilibrium equation using degenerate gas equations of state. It produces models of the internal structure of white dwarf stars.
DIANE -- Distributed Analysis Environment for Parallel Scientific Applications. Keywords: middleware, Master Worker Workflow Manager, GRID.
The aim of this project is to produce high-res/quality printable star maps according to your latitude. This projected was founded at the Deutsche SchülerAkademie Steinmühle 2004. It's a cooperation of the astronomy and cg courses.
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.
Program to calculate Easter date for any year. It can also display palm Sunday, Ash Wedenesday, Lent and other dates. In the future, it will be a complete holiday calendar.
Gigapixel GPU accelerated radio interferometric imager
ExCon can create images with a very wide field of view (more than billion pixels). It implements novel gridding and image weighting algorithms. It is well suited to make ultra deep radio interferometric images, minimizing aliasing artefacts and PSF variation. NVIDIA GPU acceleration is available. JAVA/SCALA support available.
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.
Gnorbits is an open source 3-D orbit program. It supports multiple bodies of varying masses and initial velocities, using a GTK interface.
Image stacking software for Unix/Linux, primarily for Astrophotography
Simple image stacking software for Unix/Linux, primarily for Astrophotography. Written in GTKMM (C++). Note: Currently being planned/implemented; not final working software yet.
Finds the cosmological power spectrum from a N-body simulation using the MPI FFTW library. May be run as a parallel computation for increased resolution. Reads in binary Gadget2 files.
Toolbox for high-level analysis of astronomical gamma-ray data
GammaLib is a versatile toolbox for the high-level analysis of astronomical gamma-ray data. It consists of a C++ library and a Python module that exposes the full functionality of the library to Python. The library provides an abstract data analysis framework that is independent of any specific gamma-ray telescope. Instrument specific aspects, such as handling of data formats and response functions, are implemented as isolated and well defined modules sharing an identical abstract interface. This enables a joint multi-instrument analysis of data, allowing for consistent broad-band spectral fitting or imaging. So far, GammaLib supports analysis of data obtained with COMPTEL, Fermi/LAT, and Cherenkov telescopes (CTA, H.E.S.S., MAGIC, VERITAS). Except for HEASARC's cfitsio library that is used to implement the FITS interface, GammaLib does not rely on any third-party software. All functionalities are implemented natively.