activity
19932026
most citedPossible Gravitational Microlensing of a Star in the Large Magellanic Cloud

769 citations · 6.6k across the 83 of their papers we have counts for

collaborators

84 papers

astro-ph.HE2026

Early Optical Follow-up of Gamma-Ray Bursts: The Critical Role of Robotic Telescopes

Rahul Gupta, Judith Racusin, Gor Oganesyan +26

Gamma-ray bursts (GRBs) are the most luminous electromagnetic explosions in the Universe, and offer unique laboratories for studying relativistic jets, compact-object formation, pa…

astro-ph.HE2023

Cosmological Distance Measurement of 12 Nearby Supernovae IIP with ROTSE-IIIB

Govinda Dhungana, Robert Kehoe, Ryan Staten +14

We present cosmological analysis of 12 nearby () Type IIP supernovae (SNe IIP) observed with the ROTSE-IIIb telescope. To achieve precise photometry, we present a new image…

hep-ex2022★ 747 cited

First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment

J. Aalbers, D. S. Akerib, C. W. Akerlof +344

The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility in Lead, South Dak…

physics.ins-det2020★ 60 cited

The LUX-ZEPLIN (LZ) radioactivity and cleanliness control programs

D. S. Akerib, C. W. Akerlof, D. Yu. Akimov +387

LUX-ZEPLIN (LZ) is a second-generation direct dark matter experiment with spin-independent WIMP-nucleon scattering sensitivity above cm for a WIMP mass…

astro-ph.HE2020★ 19 cited

SN 2010kd: Photometric and Spectroscopic Analysis of a Slow-Decaying Superluminous Supernova

Amit Kumar, Shashi Bhushan Pandey, Reka Konyves-Toth +21

This paper presents data and analysis of SN 2010kd, a low-redshift () H-deficient superluminous supernova (SLSN), based on ultraviolet/optical photometry and optical spe…

physics.ins-det2020★ 41 cited

Simulations of Events for the LUX-ZEPLIN (LZ) Dark Matter Experiment

ZEPLIN Collaboration, D. S. Akerib, C. W. Akerlof +194

The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1--2)\,pb at a WIMP mass of 40 GeV/…