activity
20152023
most citedMultiwavelength Study of Quiescent States of Mrk 421 with Unprecedented Hard X-Ray Coverage Provided by NuSTAR in 2013

143 citations · 1k across the 26 of their papers we have counts for

collaborators

26 papers

astro-ph.GA2023★ 4 cited

Tracing the Total Stellar Mass and Star Formation of High-Redshift Protoclusters

Roxana Popescu, Alexandra Pope, Kyoung-Soo Lee +6

As the progenitors of present-day galaxy clusters, protoclusters are excellent laboratories to study galaxy evolution. Since existing observations of protoclusters are limited to t…

astro-ph.HE2023★ 16 cited

Scary Barbie: An Extremely Energetic, Long-Duration Tidal Disruption Event Candidate Without a Detected Host Galaxy at z = 0.995

Bhagya M. Subrayan, Dan Milisavljevic, Ryan Chornock +19

We report multi-wavelength observations and characterization of the ultraluminous transient AT 2021lwx (ZTF20abrbeie; aka ``Barbie'') identified in the alert stream of the Zwicky T…

astro-ph.GA2023★ 29 cited

ODIN: Where Do Lyman-alpha Blobs Live? Contextualizing Blob Environments within the Large-Scale Structure

Vandana Ramakrishnan, Byeongha Moon, Sang Hyeok Im +16

While many Lyman-alpha Blobs (LABs) are found in and around several well-known protoclusters at high redshift, how they trace the underlying large-scale structure is still poorly u…

astro-ph.HE2023★ 42 cited

The optical light curve of GRB 221009A: the afterglow and the emerging supernova

M. D. Fulton, S. J. Smartt, L. Rhodes +46

We present extensive optical photometry of the afterglow of GRB~221009A. Our data cover \,days from the time of \textit{Swift} and \textit{Fermi} GRB detections. Photom…

astro-ph.GA2022★ 28 cited

Evaluating Lya Emission as a Tracer of the Largest Cosmic Structure at z~2.47

Yun Huang, Kyoung-Soo Lee, Olga Cucciati +13

The discovery and spectroscopic confirmation of Hyperion, a proto-supercluster at z~2.47, provides an unprecedented opportunity to study distant galaxies in the context of their la…

astro-ph.GA2022★ 7 cited

Measuring the Total Ultraviolet Light from Galaxy Clusters at z=0.5-1.6: The Balance of Obscured and Unobscured Star-Formation

Jed McKinney, Vandana Ramakrishnan, Kyoung-Soo Lee +4

Combined observations from UV to IR wavelengths are necessary to fully account for the star-formation in galaxy clusters. Low mass (log M/Msun<10) galaxies are typically not indivi…