Showing 9 open source projects for "program files"

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  • 1

    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...
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  • 2
    U-Net Fusion RFI

    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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  • 3
    PARot polar aligner

    PARot polar aligner

    Software for polar alignment of equatorial mounts

    PARot is a program for ultra fast and precise polar alignment of equatorial mounts. You can easily achieve alignment accuracy better than 1 arcmin in 5 minutes of time. You take one image of the celestial pole, rotate the mount around the RA axis and take another image. The program compares the images and shows you the necessary adjustment. The adjustment process is controlled by the live-liew created by your camera. Requirements: * A computer with Windows OS (tested with WinXP x64, Win7...
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  • 4
    lxnstack

    lxnstack

    A program to align and stack astronomical images.

    .... * 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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  • 5
    FABS

    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.
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  • 6
    Slnečné škvrny

    Slnečné škvrny

    Program na spracovanie pozorovaní slnečných škvŕn

    ...Pozorovania sú následne štatisticky spracované do tabuliek a grafov popisujúcich aktivitu Slnka. Program taktiež umožňuje výpočet fyzikálnych súradníc Slnka, Carringtonovej otočky a juliánskeho dátumu. Program je určený pre astronómov – amatérov aj profesionálnych astronómov. Program rieši komplexne problém pozorovania slnečných škvŕn. Taktiež realizuje kontrolu vstupných dát od užívateľa. Pre správne fungovanie programu je potrebné dať užívateľovi právo zapisovať do priečinku "C:\Program Files\Slnecne skvrny".
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  • 7

    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.
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  • 8

    galprop_skymap_convert

    Convert galprop skymaps to standard healpix

    A routine for converting GALPROP-generated HealPix skymaps to a compatible format which can be plotted by Aladin (v7), available from CDS at http://aladin.u-strasbg.fr. This allows free rotation of the sphere, avoiding the distortions of Aitoff and other projections often used. It is a very practical way to view and prepare skymap plots of GALPROP output. GALPROP outputs a spectrum per HealPix pixel, while Aladin requires each energy to be stored as a column. A conversion is required to...
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  • 9

    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.
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