papers
Publications (15)
astro-ph.HE2015
Swift Observations of Gamma-Ray Burst Pulse Shapes: GRB Pulse Spectral Evolution Clarified
Jon Hakkila, Amy Lien, Takanori Sakamoto +3
astro-ph.IM2009
LSST Science Book, Version 2.0
LSST Science Collaboration, Paul A. Abell, Julius Allison +245
astro-ph.CO2010
Synoptic Sky Surveys and the Diffuse Supernova Neutrino Background: Removing Astrophysical Uncertainties and Revealing Invisible Supernovae
Amy Lien, Brian D. Fields, John F. Beacom
astro-ph.HE2015
iPTF14yb: The First Discovery of a GRB Afterglow Independent of a High-Energy Trigger
S. Bradley Cenko, Alex L. Urban, Daniel A. Perley +34
astro-ph.HE2018
The 105 month Swift-BAT all-sky hard X-ray survey
Kyuseok Oh, Michael Koss, Craig B. Markwardt +10
astro-ph.CO2011
Radio Supernovae in the Great Survey Era
Amy Lien, Nachiketa Chakraborty, Brian D. Fields +1
astro-ph.HE2015
Do the Fermi Gamma-Ray Burst Monitor and Swift Burst Alert Telescope see the Same Short Gamma-Ray Bursts?
Eric Burns, Valerie Connaughton, Bin-Bin Zhang +5
astro-ph.HE2016
The Third Swift Burst Alert Telescope Gamma-Ray Burst Catalog
Amy Lien, Takanori Sakamoto, Scott D. Barthelmy +12
astro-ph.IM2019
BurstCube: Concept, Performance, and Status
Jacob R. Smith, Michael S. Briggs, Alessandro Bruno +26
astro-ph.HE2016
Probing the Cosmic Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope
Amy Lien, Takanori Sakamoto, Neil Gehrels +4
astro-ph.CO2009
Cosmic Core-Collapse Supernovae from Upcoming Sky Surveys
Amy Lien, Brian D. Fields
astro-ph.HE2019
A Search for High-Energy Counterparts to Fast Radio Bursts
Virginia Cunningham, S. Bradley Cenko, Eric Burns +8
astro-ph.HE2019
Swift spectra of AT2018cow: A White Dwarf Tidal Disruption Event?
N. Paul M. Kuin, Kinwah Wu, Samantha Oates +19
astro-ph.CO2012
The Diffuse Gamma-ray Background from Type Ia Supernovae
Amy Lien, Brian D. Fields
astro-ph.CO2013
Probing the Gamma-Ray Burst Rate with Trigger Simulations of the Swift Burst Alert Telescope
Amy Lien, Takanori Sakamoto, Neil Gehrels +4