Open Source Linux Astronomy Software - Page 4
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Astronomy Software for Linux
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myFP2ESP8266 Focus Controller
This is a port of the myFP2ESP32 Wifi Focus Controller to the ESP8266
A ESP8266 WiFi focuser. DRV8825, ULN2003, L298N, L293DMINI , L9110S, Support for Webserver, ALPACA, and TCP/IP. (c) Robert Brown 2014-2025, Holger M, 2019-2021. All rights reserved. Code or portions of code may not be copied or used without appropriate credit given to author(s). -
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ESP32 Dew Controller
ESP32 4-channel dew controller.
This is an enhanced 4-Channel automated Dew Controller based on an ESP32 WiFi chip on a PCB and enclosed in a project hobby box. (c) Copyright Robert Brown 2020-2024. All Rights Reserved.Permission is granted for personal and Academic use only. Code or portions of code may not be copied or used without appropriate credit given to author. EXPANSION BOARDS - You can expand this project using the two types of project expansion boards at https://sourceforge.net/projects/myesp-boards/ -
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INDI Sharp
INDI C# Client
This project consist in a .NET/Mono assembly containing a simple INDI client and a WinForm that permits to connect to astronomical equipment INDI server, and to use drivers connected at it. -
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Moon Phase
Displays the phase of the moon in the system tray.
Displays the phase of the moon in the system tray. Additionally, a window can be displayed that shows user configurable data about the moon (rise/set times, percent illumination, etc). -
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OpenAstrology is Java based Object-orientated implementation of Astrology. OpenAstrology will provide a platfrom to plug-in in the knowledge of Astrology and the derived solution will be the best real time Astrology solution
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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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giza
A scientific plotting library for C/Fortran built on cairo
A 2D scientific plotting library built on cairo. Provides uniform output to pdf, ps, png and X-Windows. Written in C with no dependencies (other than cairo) as a direct replacement for PGPLOT. -
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lxnstack
A program to align and stack astronomical images.
Lxnstack is a program designed to align and stack astronomical images (both planetary and deep-sky). The features of latest version are: * Several stacking methods (average, median, sigma-clipping, ...) * Two automatic align method: align-points; phase correlation, * One manual align method. * sub-pixel precision (0.1 pixel for phase correlation and 0.01 pixel for manual alignment). * Automatic image derotation. * FITS file support (by installing the python2 package 'astropy') * Hot pixels suppression algorithm * CR2 files native support * Can load/save video * Grayscale RAW image support * Editing of result image's levels. * Light curve generation -
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satpos
c++ library for calculating the position of a satellite
This library is used to calculate the position of a satellite or the moon on any geographical location on the earth's surface. The Library is writte in C++ and OOP. The Actual Status of the Library can download from the svn-repository. On my website oe5tpo.com can you find infos about satpos, but this infos are all in German! -
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wxEphe
Astronomical Ephemeris
wxEphe displays Astronomical Ephemeris for The Sun, The Moon, and solar system planets, given date and observer's location. -
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FreDec
Parallelized FREquency DEComposer algorithm
This is a parallelized algorithm performing a decomposition of the time-series data into a number of sinusoidal components, disentangling them from the white Gaussian noise. The algorithm analyses all suspicious frequencies, including the ones that look like an alias at a glance, but may become preferable later. After selection of the initial frequency candidates, the algorithm passes through all their possible combinations and estimates their multi-frequency statistical significance. In the end, it prints out the set of largest frequency tuples that were still found significant. The GPU computing is implemented through CUDA and brings a significant performance increase. It is still possible to run FreDec solely on CPU, if no suitable GPU device is available in the system. See the details of the underlying theory in Baluev 2013, MNRAS, V. 436, P. 807 The description of the algorithm itself can be found in arXiv:1309.0100. Please go to the project forum to report any bugs. -
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GRad is a standalone solar radiation model, programmed in Java. It is capable of the calculation of potential (clear sky) and actual (real sky) irradiance and total irradiation for single and multiple geographical locations. Note that, while fully functional, this application is currently not developed any further.
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JavAstro
A collection of java astronomy tools
A collection of astronomy tools written in java: sky map, astronomical events, ephemerides, planet visibility, moon calendar and galilean moons. -
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Nightsky is a very basic rendering of the stars in the sky for devices that aren't powerful enough to run Stellarium
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Specview is a Java GUI_based application for 1-D spectral visualization and analysis of astronomical spectrograms generated by a variety of observatories and instruments. Note that we no longer provide file distributions of this software. You are encouraged to visit the specview web site download page: http://www.stsci.edu/institute/software_hardware/specview/download to retrieve an installer appropriate for your platform.
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Talon is a a fully automated open-source solution for automated telescope and observatory control. Talon controls all aspects of robotic astronomical observations, including telescope control, dome control, image processing, scheduled operations, and envi
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VStar
Multi-platform Variable Star Visualisation and Analysis
VStar is a multi-platform, easy-to-use variable star observation visualisation and analysis tool. Data can be read from a file or the AAVSO database, light curves and phase plots created, period analysis performed, and filters applied. Plugins can be developed, e.g. to make additional observation sources available. See also: 1. http://www.aavso.org/vstar-overview 2. http://www.aavso.org/forums/about-aavso/vstar 3. http://dbenn.wordpress.com/category/astronomy-science/vstar 4. http://www.citizensky.org/teams/vstar-software-development -
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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 * deuterium production by pp fusion * JF12 B-field * hadronic losses Full details in the Explanatory Supplement and README. Now at https://gitlab.mpcdf.mpg.de/aws/galprop Older versions, datasets etc: http://galprop.stanford.edu. See also http://www.mpe.mpg.de/~aws/propagate.html https://sourceforge.net/projects/galplot http://sourceforge.net/projects/galpropskymapco https://sourceforge.net/projects/gcrconvert https://sourceforge.net/projects/galpropsynchrotron synchrotron routines. -
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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.
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myGPS Arduino Nano DIY
Build your own GPS unit
To develop an Arduino Nano based GPS module that is low cost, portable and can be used in Astronomy. (c) Copyright Robert Brown 2014-2024. All Rights Reserved. Permission is granted for personal and Academic use only. Code or portions of code may not be copied or used without appropriate credit given to author. -
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AEPHEM is an astronomical ephemeris and reduction C library. It is compatible with JPL ephemerides. It has routines for the standard astrometric reductions, conversions between different time standards and transformations between coordinate systems.
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AOFlagger
RFI detector and quality analysis for astronomical radio observations
The AOFlagger is a tool that can find and remove radio-frequency interference (RFI) in radio astronomical observations. The code has been highly optimized for speed and accuracy. It is used by default for the LOFAR radio telescope and thus is in productional stage. The software can run in a fully automated way, but a graphical interface is provided to analyse results and tweak the strategy. The preferred input file format is the Casa Measurement Set (MS) format. I believe that the AOFlagger is the best available flagger, both in terms of accuracy and speed. It has been succesfully used on several interferometric telescopes, including LOFAR, WSRT, VLA, GMRT, ATCA and MWA, and the single-dish telescopes Parkes and Arecibo 305m. Besides the flagger, the software consists of tools to efficiently visualize data in different ways, such as plotting time-frequency diagrams and power spectra. It provides the programs rficonsole, rfigui, aoqplot, aoquality and more. -
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APLpy (the Astronomical Plotting Library in Python) is a Python module aimed at producing publication-quality plots of astronomical imaging data in FITS format. Visit http://aplpy.sourceforge.net/ for tutorials and documentation.
