A Planetary Intensity Code for Atmospheric Spectroscopy Observations
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Updated
Dec 9, 2024 - Python
A Planetary Intensity Code for Atmospheric Spectroscopy Observations
A Python package for calculating detection limits for exoplanet high contrast imaging (HCI) datasets.
MADYS: isochronal parameter determination for young stellar and substellar objects
Repository for our deep multi-frequency fusion paper in DOT imaging.
Direct Exoplanet Imaging with Tensor Decompositions
Half-Sibling Regression for High-Contrast Imaging
Color Classification of Extrasolar Giant Planets
Generator of synthetic reflection spectra of Earth-like exoplanets observed by the Habitable Worlds Observatory using the Planetary Spectrum Generator
Various IDL procedures as part of a direct imaging data reduction and analysis pipeline for LBT data.
Miscellaneous IDL procedures that may be useful for astronomical research (incl. direct imaging) but are not included in the IDL Astronomy User's Library (ASTROLIB).
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