Search Results for "open source software framework"
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Showing 21 open source projects for "open source software framework"
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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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U-Net Fusion RFI
U-Net for RFI Detection based on @jakeret's implementation
See original code here: https://github.com/jakeret/tf_unet Currently this project is based on Tensorflow 1.13 code base and there are no plans to transfer to TF version 2. The primary improvements to this code base include a training and evaluation framework, along with a fusion based approach to detection, combining a number of models (currently hard coded to two trained models) along with Sum Threshold as an additional "expert." Additional work is being done to add custom layers to... -
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Pikon-Stelarium interface
Pikon-Stelarium interface to use with azimuthal mount
This is a full project to make an software-drived azimuthal mount for the Pikon telescope, it can be use for others telescope. This project include : . Some other parts to print to adapt to the Pikon . Python code for raspberry Needed parts for "as it" use : . 1 Raspberry (model A suit well) . 3 motors steppers . 3 steppers drivers . 1 BNO055 (the one from adafruit was used) . 1 Pikon driver . 1 GPS module Sofware requirement : . raspbian . python 3 . some python libraries -
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CMD Plot Tool
Calculates and plots Colour Magnitude Diagrams from Astronomical data
CMD Plot Tool calculates and plots Colour Magnitude Diagrams (CMDs) from astronomical photometric data, e.g. of a star cluster observed in two filter bandpasses. It can handle multiple file formats (plain text, DAOPHOT .mag files, ACS Survey of Galactic Globular Clusters .zpt files) to generate professional and customised plots, without the usual steep learning curve. Development using Python, OOP and a formal software development lifecycle model (Agile) allowed for the creation of an... -
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Now maintained at github.com/spacepy/spacepy Space Science library for Python - contains superposed epoch classes, drift shell tracing, access to magnetic field models, streamline tracing, bootstrap confidence limits, time and coordinate conversions, etc.
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RTS2 - Remote Telescope System
Open source observatory control software
RTS2 is project to create an open source environment for control of a fully autonomous observatory. It is running about dozen fully autonomous observatories. Its modular design allow easily addition of new devices (to already huge supported HW list). -
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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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FABS
Fluorescence and absorption spectroscopy made easy
FABS is a program designed to run a fluorescence/absorption spectrometer on Windows. The program analyzes spectra and provides graphs and data files. Users may choose to input video files from cell phones or other cameras, still images, or even live streams of video from webcams. FABS can perform any necessary calibration and image preprocessing. Experienced users have a number of more advanced options such as background subtraction, adjustments for nonlinearities in detector response,... -
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MYRaf Project
An Easy GUI for IRAF Photometry
The MYRaf is a practicable astronomical image reduction and photometry software and interface for IRAF. For this purpose, MYRaf uses iraf, PyRAF and alipy via great programming language Python and Qt framework. Also MYRaf is a absolutely free software and distributed with GPLv3 license. You can use it without restrictive licenses, make copies for your friends, school or business. -
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Implementation in Python of some of the statistical methods provided by "asurv", the survival analysis software.
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py-astro
An astronomical library.
Python package for calculation right ascension, declination, and distance for solar system planets. -
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QDeblend3D is a dedicated software tool for the deblending of QSO and host galaxy emission in 3D datacubes obtained with optical IFU spectrographs. The GUI allows to control the process and to visualize the results with an integrated cube viewer.
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pyastrolib is a python library providing professional astronomers a robust set of tools for astronomical data analysis. This project will provide all the functionality as NASA's IDL Astronomy User's Library in addition to other planned features.
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Tokenizer and translator for the IDL language, principally used with the IDL environment from ITTVis and GDL.
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klathon is an environment in which you can switch between the two languages: Python and CLASS (CLASS is a famous software for astronomy). You can program in one language and switch to the other halfway, thus heavily enhance CLASS's controlling ability.
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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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Python & NOVAS. Use Python to calculate the position of Sun, Moon, Planets and Stars with unprecedented precision. PyNOVAS can be used by (Amateur) Astronomers, Sailors and other people interested in Celestial Navigation, Astronomy and Astrometry.
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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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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.
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