activity
20172023
most citedThe discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck

465 citations · 985 across the 23 of their papers we have counts for

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Showing 2021Show all

5 papers · 1 filter

astro-ph.HE2021★ 10 cited

SN 2018bsz: significant dust formation in a nearby superluminous supernova

T. -W. Chen, S. J. Brennan, R. Wesson +41

We investigate the thermal emission and the extinction from dust associated with the nearby (z = 0.0267) superluminous supernova (SLSN) 2018bsz. Our dataset combines daily-cadence,…

astro-ph.GA2021★ 47 cited

An empirical representation of a physical model for the ISM [CII], CO, and [CI] emission at redshift

Shengqi Yang, Gergö Popping, Rachel S. Somerville +3

Sub-millimeter emission lines produced by the interstellar medium (ISM) are strong tracers of star formation and are some of the main targets of line intensity mapping (LIM) survey…

astro-ph.CO2021★ 16 cited

On estimating the cosmic molecular gas density from CO Line Intensity Mapping observations

Patrick C. Breysse, Shengqi Yang, Rachel S. Somerville +3

The Millimeter-wave Intensity Mapping Experiment (mmIME) recently reported a detection of excess spatial fluctuations at a wavelength of 3 mm, which can be attributed to unresolved…

astro-ph.HE2021★ 16 cited

Magnetar-Driven Shock Breakout Revisited and Implications for Double-Peaked Type I Superluminous Supernovae

Liang-Duan Liu, He Gao, Xiao-Feng Wang +1

The discovery of early bumps in some type-I superluminous supernovae (SLSNe-I) before the main peaks offers an important clue to their energy source mechanisms. In this paper, we u…

astro-ph.GA2021★ 11 cited

The prospects for observing [OIII] 52 micron emission from galaxies during the Epoch of Reionization

Shengqi Yang, Adam Lidz, Gergö Popping

The [OIII] 88 m fine structure emission line has been detected into the Epoch of Reionization (EoR) from star-forming galaxies at redshifts with ALMA. These m…