Red Hat Ansible Automation Platform on Microsoft Azure
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This is a specialised utility that works with the astronomical digital video (ADV) standard (http://tech.groups.yahoo.com/group/adv-standard/) and converts individual video frames to FITS files.
ADV files can be recorded by devices such as the
Astronomical Digital Video System (ADVS) - http://www.astrodigitalvideo.com.au/
Astrosoft is a free indian astrology software program for astrologers and astrological students. Its a Java Swing based GUI Application.
It provides Birth chart of individual with details of Lagna, Rasi, Nakshata, Thithi, Paksha and many more features.
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.
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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.
JOrrery simulates the motion of planets moving under gravity.
It comes with a number of initial "scenarios" you can run, such as "The solar system", "Earth & Moon" etc. You can also add more planets during a simulation.
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.
Ksetiwatch monitors multiple SETI@home clients running on your computer or in your local network, and logs/manages completed work units. It is developed for the K Desktop Environment.
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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
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