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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.
The Automated Parameter Estimation and Model Selection Toolkit is a fast, parallelized MCMC engine written in C for Bayesian inference (parameter estimation and model selection).
ephemeritis is to be a library for ephemeris calculations. When complete, it will provide an API for calculating the positions, the rise and set times, and related information about stars, planets, the Moon, and other astronomical objects.
GCX provides a complete set of data-reduction functions for CCD photometry, accessible both from a GUI and the command line. It also controls CCD cameras and telescopes, and implements automatic observation scripting.
L.E.I.C.A. (Long Exposure Internet CAmera) is an application that takes input from your webcam, or v4l2 device, and makes a long-exposure image.
Until now there's only a python binding for this app, soon there will be a C/C++ SDL one
Oree - Optimum Real-time Estimation of Events of Interaction: real-time reconstruction of photon interaction events in Gamma Cameras. Optionally making use of a CUDA enable GPU, Oree achieves reconstruction of over 1M events/sec.
SWIM is a special non-trivial software package that monitors solar activity and the Earth's geomagnetic activity in real-time. Solar Terrestrial Dispatch has released this formerly commercial software into the public domain.
Astro Info is a multi-lingual astronomical ephemeris for the PalmOS that provides data for our solar system and other objects. If you wish to get involved, please download a copy of the source code from CVS.
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).
Sky Observer's Almanac is a tool to assist astronomers in planning an observing session. By defining targets and events that one wishes to observe, it allows the user to schedule these targets in an optimal fashion, and spend more time observing.
ACRASH is an open implementation of the CRASH Monte-Carlo continuum radiative transfer scheme presented in Ciardi et al. 2001 and Maselli et al. 2003. This code solves the radiative transfer equation for any geometry in 3D using a Monte-Carlo scheme.
Suite of hardware and software tools for Meade Autostar products, like computer interfaces, autoguide port, stepper motors, electric focuser compatible accessories.
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
Desktop gadget (Windows only). The simulation of a real horizontal sundial, dependent on a geographic position (latitude). Size can be chosen between big and small. It can use current (computer) time, or user-specified date&time.
AstroEasyCap is an optimized linux easycap DC60 driver for astronomical purpose. It comes from the great easycapdc60 driver written by rmt1947. Features : integration control using a TTL output, bypass frame processing, gray-scale optimized mode...
A system designed to drive a computer motorized telescope mount to track artificial satellites in real time. Additionally, provides video time stamping using GPS via dedicated hardware solution.
The project is a time domain correlator for the Cell Broadband Engine (Cell BE). It is the outcome of a master thesis conducted at the Swedish Institute of Space Physics (www.irfu.se). The project files can be found in the SVN repository.
ephem68k is an astronomy software the TI-92 and TI Voyage 200 CAS systems. It calculates astronomical data like julian date, local sidereal time, full/new moons, ephemerides of fixed and solar objects and more. ephem68k is based on ephem 4.29 code.
Henry is an interface for Taylor 1.4.3 package (A. Jorba & M. Zou) and was written for master thesis to compute N-body problems (in Poincare variables) and MEGNO stability factor. Work is supported by Krzysztof Gozdziewski.