A Planetary Intensity Code for Atmospheric Spectroscopy Observations
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Updated
Aug 28, 2026 - 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
Synthetic spectra generation and CNN-based retrieval of Earth-like exoplanets for the Habitable Worlds Observatory, based on the HabEx and LUVOIR mission concepts.
Interactive offline all-sky atlas of published images of circumstellar disks, directly imaged companions, and coronagraphic quasar hosts — 740+ systems, 3100+ image records, every image cited to its paper
Color Classification of Extrasolar Giant Planets
An HST pipeline for reducing wide-field imaging observations not specifically designed for High Contrast Imaging analysis. Published in Strampelli et al. 2022.
Personal website to promote my research.
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).
Various IDL procedures as part of a direct imaging data reduction and analysis pipeline for LBT data.
A working reference on direct-imaging exoplanet detection: the contrast and angular-resolution physics, worked numerical examples including HR 8799 b, real detection statistics, and an interactive calculator built on the actual equations.
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