papers

Publications (47)

astro-ph.HE2025

Optimizing Kilonova Searches: A Case Study of the Type IIb SN 2025ulz in the Localization Volume of the Low-Significance Gravitational Wave Event S250818k

Noah Franz, Bhagya Subrayan, Charles D. Kilpatrick +54

Kilonovae, the ultraviolet/optical/infrared counterparts to binary neutron star mergers, are an exceptionally rare class of transients. Optical follow-up campaigns are plagued by c…

astro-ph.HE2019

GRB 180620A: Evidence for late-time energy injection

Rosa L. Becerra, Fabio De Colle, Alan M. Watson +11

The early optical emission of gamma-ray bursts gives an opportunity to understand the central engine and first stages of these events. About 30\% of GRBs present flares whose origi…

astro-ph.CO2011

Constraints on the Progenitor System of the Type Ia Supernova SN 2011fe/PTF11kly

Weidong Li, Joshua S. Bloom, Philipp Podsiadlowski +25

Type Ia supernovae (SNe) serve as a fundamental pillar of modern cosmology, owing to their large luminosity and a well-defined relationship between light-curve shape and peak brigh…

astro-ph.IM2011

Active Learning to Overcome Sample Selection Bias: Application to Photometric Variable Star Classification

Joseph W. Richards, Dan L. Starr, Henrik Brink +6

Despite the great promise of machine-learning algorithms to classify and predict astrophysical parameters for the vast numbers of astrophysical sources and transients observed in l…

astro-ph2008

Generalized Tests for Selection Effects in GRB High-Energy Correlations

Nathaniel R. Butler, Daniel Kocevski, Joshua S. Bloom

Several correlations among parameters derived from modelling the high-energy properties of GRBs have been reported. We show that well-known examples of these have common features i…

astro-ph2007

X-ray Hardness Variations as an Internal/External Shock Diagnostic

Nathaniel R. Butler, Daniel Kocevski

The early, highly time-variable X-ray emission immediately following GRBs exhibits strong spectral variations that are unlike the temporally smoother emission which dominates after…