A Planetary Intensity Code for Atmospheric Spectroscopy Observations
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Updated
Jun 26, 2025 - Python
A Planetary Intensity Code for Atmospheric Spectroscopy Observations
MADYS: isochronal parameter determination for young stellar and substellar objects
A Python package for calculating detection limits for exoplanet high contrast imaging (HCI) datasets.
Repository for our deep multi-frequency fusion paper in DOT imaging.
Half-Sibling Regression for High-Contrast Imaging
Direct Exoplanet Imaging with Tensor Decompositions
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
An HST pipeline for reducing wide-field imaging observations not specifically designed for High Contrast Imaging analysis. Published in Strampelli et al. 2022.
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).
Personal website to promote my research.
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