Astronomy Software

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  • 1
    novaforjava

    novaforjava

    novaforjava is a general purpose, Celestial Mechanics, Astrometry lib

    novaforjava is a general purpose, double precision, Celestial Mechanics, Astrometry and Astrodynamics library. The intended audience of libnova is java programmers, astronomers and anyone else interested in calculating positions of astronomical objects or celestial mechanics. It is a reimplementation of libnova with is the calculation engine used by the Nova project and most importantly, is free software.
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  • 2

    openSkyMatch

    Matches OpenScience Observatories images with astronomical catalogs

    openSkyMatch is a collection of Linux shell and Python scripts designed for the OpenScience Observatories program. It automates the identification and matching of detected celestial objects in locally captured FITS images with entries in large-scale sky catalogs, notably Pan-STARRS1 DR2 (II/389/ps1_dr2). The toolkit supports data preprocessing, coordinate correlation, and catalog-based validation of astronomical detections. All tools are open-source and optimized for reproducibility and transparency in citizen science astronomy.
    Downloads: 0 This Week
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  • 3
    openeqalign
    Programa para simular un ocular reticulado mediante una webcam. Permite utilizar una cámara web compatible con v4l2 para hacer alineación polar de una montura ecuatorial con el método de deriva (drift method)
    Downloads: 0 This Week
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  • 4

    pgrascom

    ASCOM driver for Firefly MV 0.3MP camera

    Downloads: 0 This Week
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  • 5
    A php port of the solunar tables calculator. Calculates Solunar Tables for any position on earth. Solunar tables are used to predict the best days and times of day to go hunting and fishing.
    Downloads: 0 This Week
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  • 6

    pwc-lxled

    PWC driver modded for Long Exposure and Led control support

    This driver is derived from the PWC driver found in the Linux kernel. It adds V4L2 controls (`V4L2_CID_FLASH_STROBE/STROBE_STOP`) to drive the led present on some cameras. It also synchronously sets the video mode when power_save is off. This driver may be used to control long exposure modded webcams (SPC900, TouCam,..) when the led is used to trigger long exposure (this avoids the use of an additional serial port).
    Downloads: 0 This Week
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  • 7

    py-astro

    An astronomical library.

    Python package for calculation right ascension, declination, and distance for solar system planets.
    Downloads: 0 This Week
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  • 8
    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.
    Downloads: 0 This Week
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  • 9
    Open source development of a tool for the astronomy community to interact with the GRB Coordinates Network (GCN) broadcast of real-time gamma-ray burst (GRB) and X-ray Flash (XRF) information. Support for satellite packets: HETE-2, Integral, Swift
    Downloads: 0 This Week
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  • 10

    pyindi-client

    Python binding to the libindi library

    This project offers a python binding to the libindi library. It uses the Simplified Wrapper and Interface Generator (SWIG). You may generate a PyIndi module which mainly defines an IndiClient class. This class could be used to build python scripts able to interact with indi servers using sendNew* methods and implementing new* methods of the BaseMediator class. PyQt applications may also be built on top of IndiClient, thus allowing rapid development of GUI Indi clients. Besides Python there are also bindings for node.js, Tcl (incomplete) and PHP (not useful). As application examples you will find a Python Websocket server with which you may build a web application interacting with Indi servers, and a simple PyQt application similar to the Kstars Indi Control Panel (was built as an exercise). Finally there is an equatorial mount 3D simulator written with Freecad and Python, planned to be connected with the PyIndi module. *** The pyindi-client binding has moved to github. ***
    Downloads: 0 This Week
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  • 11
    Implementation in Python of some of the statistical methods provided by "asurv", the survival analysis software.
    Downloads: 0 This Week
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  • 12
    This project has moved; http://astrofrog.github.com/python-montage/
    Downloads: 0 This Week
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  • 13
    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 :-)
    Downloads: 0 This Week
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  • 14
    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.
    Downloads: 0 This Week
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  • 15
    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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  • 16
    seti-stat is a simple bash script that will retrieve your SETI@home statistics using HTTP protocol, egrep and lynx browser.
    Downloads: 0 This Week
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  • 17
    rochePlot

    rochePlot

    Schematically plot the evolution of binary stars

    RochePlot is a Fortran code using PGPlot to plot a series of binaries to illustrate the key stages in the evolution of a binary star
    Downloads: 0 This Week
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  • 18

    rssfiz

    Java science library.

    Java science library. Project contains modules for physics units, particle and quantum physics, molecule, chemistry and universe definitions, also additional math classes.
    Downloads: 0 This Week
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  • 19
    ruby-sphere
    ruby-sphere is a set of libraries and user interfaces written in Ruby to calculate apparent positions of stars with a moderate accuracy. Its goal is to provide an easy way to plan astronomical observations.
    Downloads: 0 This Week
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  • 20

    ruler3PL

    Photoplate images reduction program

    Package of programs allows to make astrometric reduction of xy-coordinates tables, obtained by mesurements of any stellar frames.
    Downloads: 0 This Week
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  • 21

    rx2fits

    HF/VHF spectrosopy code for the rx888mk2 direct-sampling receiver

    rx2fits is an SDR code for the rx888mk2 direct-sampling receiver that streams spectral data with frequency up to 65 MHz to FITS files. This code is for the direct-sampling input of the receiver, which transmits real samples over USB3 at up to 130 MHz sample rate. rx2fits processes these samples to spectral intensities via a Fourier-transform poly-phase filter bank, which provides spectral resolution approaching the spectral bin width with good stop-band and adjacent-channel rejection. Sample rate, Fourier bin count, PFB frame count, integration time and receiver gain parameters can be set. Utilities for device enumeration, firmware upload, display of FITS header, file viewing, and for measuring sample rate and sample statistics are provided. The device interface is Ruslan Migirow's librx888 and dropped samples at 130 MHz are negligible. Runs on linux computers under .Net.
    Downloads: 0 This Week
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  • 22
    This program will enable you to find every solar eclipse in between about 2500 BC to 3500 AD. The central line can be displayed graphically and saved as a JPEG or PNG image file or as a PDF document.
    Downloads: 0 This Week
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  • 23

    sastrocam (simple astronomy camera)

    sastrocam (simple astronomy camera) -- simple camera control for astro

    sastrocam (simple astronomy camera) -- simple camera control for astronomical imaging in Linux. Provides a simple web interface to the camera that will function well for remote control over a low bandwidth link.
    Downloads: 0 This Week
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  • 24
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  • 25

    sidmon3

    Sudden ionospheric distubance (SID) monitor

    sidmon is a python program for receiving and recording submarine-transmitter signal intensities and directions in the VLF frequency range using a computer sound card. The intensities of these signals reflect the ability of radio waves at those wavelengths to propagate in what is essentially a waveguide formed by the earth and the ionosphere above it. Fluctuations in those signal intensities and directions often reflect daytime perturbations of the ionosphere by solar processes, such as solar flares and coronal mass ejections, making VLF receivers useful tools for probing the sun and the earth's ionosphere. For additional general information, see the web page at http://solar-center.stanford.edu/SID/.
    Downloads: 0 This Week
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