Galaxy Line Emission & Absorption Modeling
Real time meteor detection by deep learning
A Python package for manipulating and correcting variable point spread functions.
pySAS is a python wrapper for the Science Analysis Software (SAS) used for analyzing XMM-Newton data. This repository is maintained by the XMM-Newton Guest Observer Facility (GOF) at Goddard Space Flight Center for testing new pySAS functionality.
Stellar aperture photometry
Bayesian model reconstruction based on astronomical spectral line observations.
SEDBYS: A python-based SED Builder for Young Stars. To cite this Original Software Publication: https://www.sciencedirect.com/science/article/pii/S2352711021000327
Machine Learning pipeline to classify astronomical sources into galaxies, quasars and stars using photometric data.
RADEX line fitter in Python
A collection of astronomical spectrum reduction and processing scripts.
Python tool to analyse infrared absorption spectra of interstellar ices
DIY dew heater bands controller
SDO Data Analysis for CLV
Multimodal Estimation Routine for the Cosmological Unravelling of Rest-frame Infrared Uniformised Spectra (MERCURIUS) uses the pymultinest package (Feroz et al. 2009; Buchner et al. 2014) to fit and plot greybody spectra given far-infrared (FIR) photometry of an object.
Toolset for planning and triggering observations with ZTF, the Zwicky Transient Facility.
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