Search Results for "gnu/linux" - Page 18
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Showing 490 open source projects for "gnu/linux"
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NTuple is a Python module used by high-energy physicists and astrophysicists to easily and efficiently access ntuple data stored in large ROOT data stores. Specifically, NTuple provides a friendly Pythonic interface to TNtuples and TTrees stored in TFiles
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XAudine : Linux control command software,GUI and device drivers for operating Audine astronomy CCD camera.
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A web atlas using the planetary body renderer, Xplanet. Explore the solar system. Overlay clouds, cities, weather forecasts, and more. Navigate by point and click. Search global databases.
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The Universe Simulator project's goal is to provide a set of libraries for simulating all known and understood physical phenomena.
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Accrete is a physical simulation of solar system planet formation. This simulation works by modelling a dust cloud around a Sun-like star, injecting a series of masses which collect dust, and form planets by accretion.
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A library allowing in-memory use of FITS data. Provides a simple interface to many CFITSIO routines. This reads and writes FITS images, tables, and headers; and provides convenient structures for passing data to other software, eg. SExtractor library.
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Script for control of seti program, support multiseti, smp, dial connect, process idle, proxy, work offline, nice, stats. etc...
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Application for logging, planning, and searching astronomy observations. Written in Python/Tkinter with support for xmlrpc/SOAP as a secondary goal.
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This project will be dedicated to developing a standard XML Schema and related technologies for the purpose of platform independent exchange of astronomical observations.
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KTelescope is a robust Server/Client control library for Meade's LX200 based telescopes. The library is divided into two components: A Low level modulo that allows access to the LX200 command set, and a Client/Server skeleton for remote control.
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This package is a collection of libraries, data processing filters, and UI applications to aid in the analysis and visualization of scientific data stored in the Radar Data Format.
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SImg is astronomical image processing software for Linux. Some of the features are deconvolution (various algorithms), removing interferences, automatic shifting of images, computation of PSF and and a visualization tool.
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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.
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The Open Source Space Flight Dynamics (OSSFD) project is intended to provide the community with an open source solution to space flight dynamics.
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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.
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The Online Astronomy Project will create a complete, web-enabled, robotic astronomy system that is hardware independent (ASCOM standard abstraction layer) and capable of servicing multiple telescopes and types of observation programs at once.
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Monitor for SETI@Home clients written in Java. Monitors statistics for a user, as well as work units.
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TNF2 is based loosely on the original game TNF (The New Frontiers) http://www.geocities.com/TimesSquare/Castle/2979/ written and designed by Jerry Revell Jerry@starchase.demon.co.uk. Simply put the game is about space colonization. Each player runs a
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It is a cross-platform astronomical software, with plug-ins support. A object-oriented library for astronomy and a graphic interface. C++, graphical tools-kit is wxWindows.
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OpenWD is a scientific project to develop state-of-the-art models of white dwarf stars, to draw upon the collective expertise of astronomers around the world, and to facilitate comparisons between evolutionary and pulsational studies of white dwarf stars
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Project Galileo at Sourceforge.net aims to provide developers a unique opportunity to develop open source software for an on-line telescope for schools across the UK. See http://www.projectgalileo.org.uk for more details.
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Calculates the shape of a telescope mirror from a sequence of Foucault test images. Java-based GUI simplifies entering and organizing measurement data. Logging and comparison functions enable quantification of the effects of various figuring strokes.
