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INDI is an instrument neutral distributed interface control protocol that aims to provide backend driver support and automation for a wide range of Astronomical devices (telescopes, focusers, CCDs..etc).
Project migrated to Github: https://github.com/indilib/indi
SITools2 is a new CNES generic tool performed by a joint effort between CNES and scientific laboratories. The aim of SITools is to provide a self-manageable data access layer deployed on already existing scientific laboratory databases.
Multi-SETI@home Monitor. This program was written to monitor SETI@home and BOINC activity that may be running on multiple computers over a network without having to cross mount file systems. Runs on Windows/Linux/Unix.
Convert data file from fixed width format table to CSV
Fixed width data files are probably the most annoying data to import into database.
This utility allows user to insert user-defined column separators into user-defided positions of flat file table given in fixed-width format.
I am using this utility to import astronomical catalogs provided as flat tables at CDS ftp-server into postgresql;
Build:
$ make all [cc={icc|gcc}]
Install:
$ make install [prefix=/path/to/your/bin/directory]
Example of usage:
$ gzip -dc table.dat.gz |...
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.
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.
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.
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
The purpose of this project is to build a client-server application that will send summaries from Seti@Home clients distributed all across a network to a central host, allowing that way to a monitoring program to show results and statistics for multiple c