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20112024
most citedAncient Light from Young Cosmic Cities: Physical and Observational Signatures of Galaxy Proto-Clusters

355 citations · 1.8k across the 31 of their papers we have counts for

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Showing astro-ph.GAShow all

18 papers · 1 filter

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.GA2023

Corrected SFD: A More Accurate Galactic Dust Map with Minimal Extragalactic Contamination

Yi-Kuan Chiang

The widely used Milky Way dust reddening map, the Schlegel, Finkbeiner, & Davis (1998; SFD) map, was found to contain extragalactic large-scale structure (LSS) imprints (Chiang & M…

astro-ph.GA2023★ 23 cited

Detection of thermal Sunyaev-Zel'dovich Effect in the circumgalactic medium of low-mass galaxies -- a surprising pattern in self-similarity and baryon sufficiency

Sanskriti Das, Yi-Kuan Chiang, Smita Mathur

We report on the measurement of the thermal Sunyaev-Zel'dovich (tSZ) Effect in the circumgalactic medium (CGM) of 641,923 galaxies with = at…

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…

astro-ph.GA2020★ 15 cited

Measuring the total infrared light from galaxy clusters at z=0.5-1.6: connecting stellar populations to dusty star formation

Stacey Alberts, Kyoung-Soo Lee, Alexandra Pope +13

Massive galaxy clusters undergo strong evolution from z~1.6 to z~0.5, with overdense environments at high-z characterized by abundant dust-obscured star formation and stellar mass…