Wo ist Io ist eine Android Astronomie Anwendung, die Daten über Himmelskörper im Sonnensystem berechnet. Es bietet Auf- und Untergangs Visualisierungen und -Zeiten für alle Planeten und eine Spiral-Graph Ansicht der Jupitermonde für nächsten Tagen
Analyse output from MCMC codes like SPINspiral and lalinference_mcmc
analyseMCMC post-processes, analyses and plots output from the LIGO/Virgo gravitational-wave inspiral parameter-estimation codes SPINspiral and lalinference_mcmc.
Very simple utilite to manage Apogee cameras
Very simple utilite to manage Apogee cameras
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.
The CASPER library is used to program FPGA systems for high speed digital signal processing for astronomical research. This version uses Xilinx XSG/ISE/EDK 8.2.
Plot GALPROP output
Plot package for GALPROP https://sourceforge.net/projects/galprop Plots models and data for cosmic-ray spectra, secondary/primary ratios, gamma rays, synchrotron. Includes gamma-ray source population synthesis and corresponding plots. For gamma rays, convolves models with the Fermi-LAT response. This release is to assess interest. It requires many input data files (not included) which will be made available as required. With the data provided cosmic-ray spectra and ratios and source population synthesis will work. Uses CERN root package. See README for details. Plots produced with GALPLOT can be seen in http://arxiv.org/abs/1101.1381 http://adsabs.harvard.edu/abs/2011A%26A...534A..54S http://adsabs.harvard.edu/abs/2011ApJ...739...29B and http://arxiv.org/abs/1309.2947, published version: http://mnras.oxfordjournals.org/content/early/2013/10/03/mnras.stt1718.abstract . Uses the cosmic-ray database https://sourceforge.net/projects/cosmicraydataba
Technological demo of OpenGL ES 2 Android NDK
Technological demo of OpenGL ES 2 for Android platform. It reads public NORAD satellite database and shows the satellite positions and altitude related to Earth in the form of beams (the height of the beam represents the relative altitude). NOTE: The project has been moved to GitHub: https://github.com/nuald/glSatellite-Demo The old one stays here just for the historical reasons. The 3D features present: - OpenGL ES 2; - rotating, multi-touch zooming and moving the globe; - stars on a fixed background; - each satellite is represented by a beam with a unique color; - identifying the corresponding satellite if a beam has been tapped (based on color picking method). Additionally to 3D features presented the application is: - using NDK with C++11 features compiled by LLVM clang; - mixing Java views with OpenGL views (Java is used for settings activity, information and ads panels); - using Android custom message queue to send asynchronous messages from Java to JNI
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.
Graphing System with a C language interface. Astrology program as sample, many others. Uses Qt to do the actual graphics.
*WARNING* gtburst moved to github (https://github.com/giacomov/gtburst). ########################################## gtBurst is a tool to download data, analyze and simulate Gamma-ray Bursts and Solar Flares as observed by the NASA Fermi satellite.
gamma rays from hadronic processes in astrophysics
Cosmic-ray hadronic interaction matrices for gamma-ray and other secondaries for an interstellar medium target are available as described in Huang et al. Astroparticle Physics, 27, 429 (2007). These require significant effort in practice to compute emissivities for given input spectra. To supplement these matrices I provide here a C++ class which reads the matrices, interpolates on user-defined particle and gamma-ray energy grids, and computes the gamma-ray emissivity either differential or in user-defined bands. A sample user program is provided which can be edited to provide the required functionality. See also http://sourceforge.net/projects/galprop, which includes more models.
jFITS is a Java Swing based application and applet for quickly viewing and performing simple operations on astronomical FITS formatted CCD imaging data.
klathon is an environment in which you can switch between the two languages: Python and CLASS (CLASS is a famous software for astronomy). You can program in one language and switch to the other halfway, thus heavily enhance CLASS's controlling ability.
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
Library for spherical harmonic transforms (SHT)
NOTE: as of April 24, 2015, libsharp development has moved to Github (https://github.com/dagss/libsharp). Libsharp is a collection of algorithms for efficient conversion between maps on the sphere and their spherical harmonic coefficients. It supports a wide range of pixelisations (including HEALPix, GLESP, and ECP). This library is a successor of libpsht (http://sourceforge.net/projects/libpsht). A scientific overview over the functionality is given in the paper available at http://arxiv.org/abs/1303.4945.
Simple frame grabber application (similar to xawtv) that can capture directly into a series of FITS files, suitable for further processing with IRIS.
Modify a manual filterwheel and add stepper motor and Arduino
A project by Clive Stachon and Robert Brown in modifying a manual 5 slot filter wheel to automatic using an Arduino Nano and stepper motor. Windows application, ASCOM driver and Arduino firmware provided. This project is still in development mode. CODE IS SUBJECT TO RAPID CHANGE. DO NOT START THIS TILL HARDWARE AND SOFTWARE ARE COMPLETED. DO NOT PURCHASE ANYTHING TILL THE PROTOTYPE IS FINISHED - IT WILL BE POSTED HERE WITH FULL DETAILS AND IMAGES AND INSTRUCTIONS.
Project moved to Google Code since SourceForce is a broken, buggy, non-responsive service. I had to re-log in over 100 times just to change this description. Please visit the project at http://code.google.com/p/starflighttlc/ for the latest version of th
This Python project creates several interfaces to HiRISE image data: * a wrapper around the ISIS framework for processing HiRISE raw images. Using Python's multiprocessing library, the time from raw data to mosaic has decreased significantly on multi-co
qapod - Fetch each day a new picture from web, store them and put them onto your background, now mainly apod (astronomic picture of the day, http://antwrp.gsfc.nasa.gov/apod/astropix.html). It can also greet YOU with a nice picture every morning :-)
retep is a collection of Java API's covering PDF, XML, J2EE , Swing and now NetBeans modules for displaying astronomical maps, controlling modern "Go-To" telescopes - all in java., and accessing online databases.
seti-stat is a simple bash script that will retrieve your SETI@home statistics using HTTP protocol, egrep and lynx browser.
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
ruby-sphere is a set of libraries and user interfaces written in Ruby to calculate apparent positions of stars with a moderate accuracy. Its goal is to provide an easy way to plan astronomical observations.
sastrocam (simple astronomy camera) -- simple camera control for astro
sastrocam (simple astronomy camera) -- simple camera control for astronomical imaging in Linux. Provides a simple web interface to the camera that will function well for remote control over a low bandwidth link.