Search Results for "http c tiny"
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Showing 27 open source projects for "http c tiny"
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HEALPix
Data Analysis, Simulations and Visualization on the Sphere
Software for pixelization, hierarchical indexation, synthesis, analysis, and visualization of data on the sphere. Please acknowledge HEALPix by quoting the web page http://healpix.sourceforge.net (or https://healpix.sourceforge.io) and publication: K.M. Gorski et al., 2005, Ap.J., 622, p.759 Full software documentation available at https://healpix.sourceforge.io/documentation.php Wiki Pages: https://sourceforge.net/p/healpix/wiki/Home Exchanging Data with HEALPix (in FITS files):... -
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p3d
General data-reduction tool for fiber-fed integral-field spectrographs
p3d is a general data-reduction tool for use with fiber-fed integral-field spectrographs (IFSs); although, the spectrum viewer works with spectrum data cubes of any origin. The tool is built about the proprietary software IDL (Harris/EXELIS; see http://www.harrisgeospatial.com), but can be used without any license. Most slowly running loops are implemented in parallelized C (OpenMP). -
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Lin-guider is an astronomical autoguiding program for Linux. It supports Philips, Logitech, uvc webcams, QHY5, QHY6, DSI2PRO, QHY5L-II-M, QHY5L-II-C, QHY5-II, ATIK, Starlight Xpress, ZWO ASI astrocams for video and FTDI chip-based, parallel port-based (LPT), GPIO-based, GPUSB devices, Nexstar-protocol based and QHY5, QHY6, QHY5L-II-M, QHY5L-II-C, QHY5-II, ATIK, Starlight Xpress, ZWO ASI astrocams for pulse guiding. Starlight Xpress ltd. is helping this project http://www.sxccd.com/
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stellarics
Inverse Compton emission from heliospheres of sun and stars
Cosmic ray electrons scatter on the photon fields around stars, including the sun, to create gamma rays by the inverse Compton effect. This program computes the spectrum and angular distribution of this emission. The software also includes general-purpose routines for inverse Compton scattering on a given electron spectrum, for example for interstellar or astrophysical source modelling. For further information see these publications: http://arxiv.org/abs/astro-ph/0607563,... -
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MieConScat is a GUI/Console program for generating MIE SCATtering data as a table of cross sections. It can generate scattering cross sections over specified angular ranges and total absorption cross sections. It was initially developed to aid work with optical particle counters (OPC) especially when CONverting data between cross section and diameter space. These methods are described in Rosenberg et al. 2012, Particle sizing calibration with refractive index correction for light scattering...
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GLORIA Project
GLObal Robotic-telescopes Intelligent Array for e-Science
GLORIA stands for "GLObal Robotic-telescopes Intelligent Array". GLORIA will be the first free and open- access network of robotic telescopes of the world. It will be a Web 2.0 environment where users can do research in astronomy by observing with robotic telescopes, and/or analyzing data that other users have acquired with GLORIA, or from other free access databases, like the European Virtual Observatory (http://www.euro-vo.org). -
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Analysis software for Nbody/SPH or SPH simulations (e.g. performed with Gadget II). See http://sourceforge.net/apps/wordpress/hyplot/about and http://sourceforge.net/apps/trac/hyplot/wiki for more information.
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galprop
Cosmic-ray propagation and emission processes
Software for cosmic-ray propagation, gamma-rays, synchrotron. Current version (r2766) includes * accurate propagation scheme * polarized synchrotron * free-free emission and absorption * new convection models * anisotropic diffusion * primary positrons * free-escape boundary conditions * new hadronic gamma-ray production models * new injection spectral breaks * upwards compatible with latest HEALPix * improved HEALPix skymap format * full reference output for a sample run *... -
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Instrumented Telescope
Software for instrumenting a Dobsonian telescope
This projects hold software required for instrumenting an alt-az telescope mount. The required hardware is documented here (http://simonbox.info/index.php/astronomy). The software enables real time conversion from (measured) alt-az to ra-dec and manages a connection to Stellarium (http://www.stellarium.org/), which allows you to view where the telescope is pointing in a virtual planetarium. -
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libsharp
Library for spherical harmonic transforms (SHT)
NOTE: as of April 24, 2015, libsharp development has moved to Github (https://github.com/dagss/libsharp). Libsharp is a collection of algorithms for efficient conversion between maps on the sphere and their spherical harmonic coefficients. It supports a wide range of pixelisations (including HEALPix, GLESP, and ECP). This library is a successor of libpsht (http://sourceforge.net/projects/libpsht). A scientific overview over the functionality is given in the paper available at... -
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Planck Level-S
Sources of the simulations package for the Planck satellite project
This project contains the sources for the simulation codes used within ESA's Planck mission (http://sci.esa.int/planck/) -
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Linux modified webcam capture software for astronomy. This project is a fork from the great Qastrocam, written by F. Sicard (http://qastrocam.sourceforge.net/). It adds some features I wrote for myself.
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Open PECTool
Open PECTool - manipulate peroidic error data for Celestron mounts.
This is clone of the Celestron PECTool used to upload, download and manipulate PEC data. It is intended to work with Celestron Nexstar mounts like NexStar GPS, NexStar GPS-SA, NexStar iSeries, NexStar SE Series, NexStar GT, Advanced-VX, Advanced-GT and CGE mounts. Communication to the hand control is 9600 bits/sec, no parity and one stop bit via the RS-232 port on the base of the hand control. To build it libnexstar version 0.11 or newer is needed, which can be found here:... -
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galplot
Plot GALPROP output
Plot package for GALPROP https://sourceforge.net/projects/galprop Plots models and data for cosmic-ray spectra, secondary/primary ratios, gamma rays, synchrotron. Includes gamma-ray source population synthesis and corresponding plots. For gamma rays, convolves models with the Fermi-LAT response. This release is to assess interest. It requires many input data files (not included) which will be made available as required. With the data provided cosmic-ray spectra and ratios and source... -
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gcr_convert
converts cosmic-ray files from GALPROP for viewing / plotting.
The GALPROP program (http://galprop.stanford.edu) computes cosmic-ray propagation in the Galaxy, in 2D or 3D. The ouput cosmic-ray distribution is in the form of FITS files which however are not convenient for viewing or plotting with the standard ftools program fv, since the files have 4 or 5 dimensional arrays (due to the momentum and species axes) while fv handles only 3 dimensional arrays. This program converts to fv-compatible FITS files, either from 2D to (R,z) or from 3D to (x,z) at... -
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Gerbil
Hyperspectral Image Visualization and Analysis Framework
The Gerbil project moved to http://www.gerbilvis.org Please visit us there for up-to-date information and current software releases! -
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galprop_propel
GALPROP update for accurate propagation calculation
The GALPROP program (http://galprop.stanford.edu) computes cosmic-ray propagation numerically. To obtain manifestly accurate solutions an explicit method is now available to replace the Crank-Nicolson operator-splitting method. This can be implemented in the public version of GALPROP with the update provided here. Instructions: replace the four files propel.cc, propel_diagnostics, Galdef.cc and Galdef.h and rebuild the executable. Add solution_method and solution_convergence to the galdef... -
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ADV2FITS
Converts ADV video frames into FITS files
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/ -
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bremsstrahlung
Non-thermal bremsstrahlung c++ routine
A C++ version of the public GALPROP (http://galprop.stanford.edu) routine to compute non-thermal bremsstrahlung, with added features to compute the gamma-ray emissivity either differential or in user-defined bands. -
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hadronic gamma rays
gamma rays from hadronic processes in astrophysics
...Astroparticle Physics, 27, 429 (2007). These require significant effort in practice to compute emissivities for given input spectra. To supplement these matrices I provide here a C++ class which reads the matrices, interpolates on user-defined particle and gamma-ray energy grids, and computes the gamma-ray emissivity either differential or in user-defined bands. A sample user program is provided which can be edited to provide the required functionality. See also http://sourceforge.net/projects/galprop, which includes more models. -
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Libpsht is a collection of algorithms for efficient conversion between maps on the sphere and their spherical harmonic coefficients. It supports a wide range of pixelisations (including HEALPix, GLESP, and ECP). Development for this libary has stopped; its successor is libsharp (http://sourceforge.net/projects/libsharp).
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qapod - Fetch each day a new picture from web, store them and put them onto your background, now mainly apod (astronomic picture of the day, http://antwrp.gsfc.nasa.gov/apod/astropix.html). It can also greet YOU with a nice picture every morning :-)
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SimuSpace
Simuspace is an realistic environnement simulator
The first goal of this project is to create a realistic environnment simulator including most of the last scientist discovery. The domain are astrophysics, geophysics, electromagnetics, ... The second goal of this project is the creation of an interface to use this environnment. In particular the fact that it is possible to connect/command/control some automatic tools (robot, sensor, ... ) note : les images utilisés proviennent de http://www.photo-libre.fr -
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a program to retrieve magnetic power spectra from Faraday rotation maps using a method described in http://arxiv.org/abs/0912.3930
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This program should compute ZHR from data contained in IMO VMDB (http://www.imo.net/data/visual), or other sources with same structure. ZHR should be calculated on arbitrary interval. It should produce analytical and graphical output.
