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
A set of tools for use by MAST community contributors preparing High Level Science Products (HLSP) or MAST Community Contributed Missions (MCCM) data collections. Currently, "Filename Check" is available, and "Metadata Check" will be coming soon.
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
Repository of pAstroCORE software.
Multi-spectral faint emission detection and color extraction tool.
Machine Learning pipeline to classify astronomical sources into galaxies, quasars and stars using photometric data.
Reduced data and scripts to reproduce the figures in the study of globular clusters using genetically modified galaxy merger histories
Fast neural posterior estimation for gravitational wave events using normalizing flows efficiently infers high-dimensional GW parameters from waveform data.
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.
DIY dew heater bands controller
Python tool to analyse infrared absorption spectra of interstellar ices
RADEX line fitter in Python
Toolset for planning and triggering observations with ZTF, the Zwicky Transient Facility.
A collection of astronomical spectrum reduction and processing scripts.
The HST/WFC3 IR Point Spread Function: A 13-Year Empirical Characterization for Precision Astronomy in the JWST Era
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