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1100 days in the life of the supernova 2018ibb
Free accessThe best pair-instability supernova candidate, to date⋆EDP Sciences | 2024| -
A reduction procedure and pipeline for the detection of trans-Neptunian objects using occultations
Free accessArXiv | 2023| -
A bias-corrected luminosity function for red supergiant supernova progenitor stars
Free accessArXiv | 2023| -
A search for Kuiper Belt occultations using the Weizmann Fast Astronomical Survey Telescope
Free accessArXiv | 2023| -
The Early Ultraviolet Light-Curves of Type II Supernovae and the Radii of Their Progenitor Stars
Free accessArXiv | 2023| -
1100 days in the life of the supernova 2018ibb -- The best pair-instability supernova candidate, to date
Free accessArXiv | 2023| -
Strong NIR emission following the long duration GRB 211211A: Dust heating as an alternative to a kilonova
Free accessArXiv | 2022| -
Measuring time delays: II. Using observations of the unresolved flux and astrometry
Free accessArXiv | 2021| -
Measuring time delays: I. Using a flux time series that is a linear combination of time-shifted light curves
Free accessArXiv | 2021| -
The Weizmann Fast Astronomical Survey Telescope (W-FAST): System Overview
Free accessArXiv | 2021| -
Second Timescale Photometry of the Very Fast Nova V1674 Her with Palomar Gattini-IR
Free accessArXiv | 2021|
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