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GUI to configurate and start XPlanet easily. Adds a downloader to XPlanet to load clouds, images and marker files from the internet. Generates cmd (windows) and configuration files for XPlanet and the downloader. Hides in the System Tray.
Virtual telescope written in Java for mobile phones. Uses CLDC1.1 and MIDP2.0. Tested on mobile phone with 2MB RAM and 60MB storage. The largest catalog uses TYCHO2(2.5M stars) and NGC+ IC(13k DSO) .Sky plotted in dark red. Has desktop version also.
pyastrolib is a python library providing professional astronomers a robust set of tools for astronomical data analysis. This project will provide all the functionality as NASA's IDL Astronomy User's Library in addition to other planned features.
JSatTrak is a Satellite tracking program written in Java. It allows you to predict the position of any satellite in real time or in the past or future. It uses advanced SGP4/SDP4 algorithms developed by NASA/NORAD to propagate the satellite orbits.
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SPIDR (Space Physics Interactive Data Resource) is a distributed database and application server network, built to select, visualize and model historical space weather data. SPIDR is a web-application and a grid of data mining web-services.
PulsarHunter is a java based package for pulsar searching. It operates on a number of standard data formats. This package also includes the JReaper graphical candidate selection tool.
displays the current phase of the Moon as an applet for the gnome panel. Clicking on the applet displays sundry data pertaining to the moon including various clock functions. The user can select between a real image as well as a cartoon image of the
PaperScope is a graphical tool for exploring the data holdings of the Astrophysics Data System (http://adsabs.harvard.edu/). It enables the user to explore the relationships between Astrophysics papers and locate papers of research interest.
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.
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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.
Jaude is "Java pour les Astronomes Utilisateurs de Detecteurs Electroniques". Jaude is Eclipse RCP and plugin based. So it will provide an Eclipse interface for JSky library (http://archive.eso.org/JSky/).
A high performance visualization tool for stars and particles able to run on Beowulfs. Rendering step is implemented separately and optimized for SSE, compatible with OpenGL. Navigation mechanism with quaternions. Ten color maps, sobel contour detect
GLNebula is a program designed for the real-time visualization of planetary nebulae models produced by photoionization codes. It uses camera-oriented quads and point sprites to achieve real-time speeds, also provides free camera movements.
jFITS is a Java Swing based application and applet for quickly viewing and performing simple operations on astronomical FITS formatted CCD imaging data.
GIRAFFE Base Line Data Reduction Software is a set of python scripts and modules
and a C library to reduce FITS images produced by the Very Large Telescope (VLT)
FLAMES instrument.
Application for astronomical photos processing. Intended mainly for amateur astrophotography, for catching "beauty of the universe" rather than some serious scientific data. Includes automatic image registration.
Uranograph is a set of classes and methods written in Java for generating printable and viewable star charts based on different data sources. Currently the Lambert azimuthal equal-area projection is implemented. Output in SVG and PDF (with iText library)
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.
KSetiSpy is a KDE program for monitoring the SETI@home client and displaying information about the data it analyzes.
It offers the same user interface as SETI Spy, a popular Windows utility.
Feature extraction toolkit based on a wavelet multiscale
vision model. Includes 1D signal processing sample application for line
identification and classification of astronomical spectra.