Search Results for "compiler python linux" - Page 2
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37 programs for "compiler python linux" with 2 filters applied:
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La P.A.P.A. (Python Alternative for Programming Astrophysics) want to give an alternative to the astrophysicists (and any one that use RSI-IDL) for start programming in Python using similar functions as IDL and at the same time learn the power of Python.
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KAstrometry is a Astrometry program for the KDE Desktop Environment. It aims to be a good tool to make measurements of objects in space from images taken by CCD cameras. Such measurements might be used to find orbits of astroids.
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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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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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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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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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PyXPA is a Python interface to the XPA library (http://hea-www.harvard.edu/RD/xpa/ developed by the SAO/HEAD R&D Group (http://hea-www.harvard.edu/RD/)).
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Build apps or websites quickly on a fully managed platformRun frontend and backend services, batch jobs, host LLMs, and queue processing workloads without the need to manage infrastructure.
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Python Arrays is a project to reimplement the existing Python Numeric module which adds the ability to efficiently manipulate large numeric arrays in ways similar to Matlab and IDL.
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Automated supernova finder is a software package to automatically compare FITS images to a nominated reference image with the aim of finding supernovae or other optical transient phenomena.
