Showing 8 open source projects for "python package"

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  • 1
    ChiantiPy is a Python package for the CHIANTI atomic database for astrophysical spectroscopy. It provides access to the database and the ability to calculate various physical quantities for the interpretation of astrophysical spectra.
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  • 2
    lxnstack

    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...
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  • 3

    Galactus

    A neutral hydrogen galaxy modeling and fitting tool

    Galactus is a new astronomical modeling package. The aim is to model and fit datacubes from radio synthesis telescopes. Galactus is the only HI tool which can predict the HI (self-)absorption.
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  • 4
    Python Planetary Physics Package
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  • 5
    Henry is an interface for Taylor 1.4.3 package (A. Jorba & M. Zou) and was written for master thesis to compute N-body problems (in Poincare variables) and MEGNO stability factor. Work is supported by Krzysztof Gozdziewski.
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  • 6
    Sparrow is a package for single-dish astronomical data-reduction developed by the National Radio Astronomy Observatory.
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  • 7

    OCFit

    Python package for fitting of O-C diagrams.

    Python package OCFit includes 4 classes for analysis and fitting of O-C diagrams of Eclipsing binaries In a case of using this package for scientific purposes, please, cite our paper Gajdoš & Parimucha (2018) where you can also find more detail description about fitting functions and used models. For install it, download/clone this repository or download suitable binary file from releases.
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  • 8
    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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