Search Results for "programming c++ library" - Page 3
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Showing 72 open source projects for "programming c++ library"
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Finds the cosmological power spectrum from a N-body simulation using the MPI FFTW library. May be run as a parallel computation for increased resolution. Reads in binary Gadget2 files.
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Astrog is a library for performing astronomical calculations, accelerated by using a graphics processing unit (GPU).
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GIRAFFE Data Reduction
GIRAFFE Data Reduction Software
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. -
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libscmodcam provides an easy way for Linux applications to capture long-exposure frames from a Philips USB webcam (if it is supported by the PWC kernel driver). Currently only the SC1 modification and the C++ language are supported.
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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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AQUYNZA is a set of C++ libraries, sample programs and doc's for the modelling, visualization and persistence of 3D environments. Its modular and highly portable. Its primary objective is helping to learn (and teach) computer graphics. (code in SPANISH)!
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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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MightySETIInfo. Yet another SETI@Home email sig/HTML summary. Written in C++. Uses the Fox GUI library, and ftp4w32. Only tested with Win32 but should be easy to port to *nix. Works with SetiHide. Output files are customizable with HTML-like templates.
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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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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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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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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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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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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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spice-dlm provides a seamless mechanism for IDL users to access the SPICE library from JPL/NAIF, providing ephemeris information for solar system objects and spacecraft.
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JFitsio is a Java library wrapping the CFITSIO library using the Java Native Interfaces (JNI) to provide acess to FITS files.
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cplmm is a library of C++ wrappers for the ESO (European Southern Observatory) Common Pipeline Library (CPL).
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QuantimSim is a physics simulation engine. Some aspects of astrophysics, electromagnetism, relativity, thermodynamics, statistical mechanics and quantum mechanics will be included in the simulation library.
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This project is an initial reference implementation of the VSI-E protocol. The implementation has been done using the C/C++ language and is in the form of a re-useable library developed on the Linux platform.
