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20142022
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations · 1.9k across the 22 of their papers we have counts for

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astro-ph.HE2022★ 14 cited

Multiple Flares in the Changing-Look AGN NGC 5273

J. M. M. Neustadt, J. T. Hinkle, C. S. Kochanek +15

NGC 5273 is a known optical and X-ray variable AGN. We analyze new and archival IR, optical, UV, and X-ray data in order to characterize its long-term variability from 2000 to 2022…

astro-ph.HE2022★ 36 cited

A JWST Near- and Mid-Infrared Nebular Spectrum of the Type Ia Supernova 2021aefx

Lindsey A. Kwok, Saurabh W. Jha, Tea Temim +55

We present JWST near- and mid-infrared spectroscopic observations of the nearby normal Type Ia supernova SN 2021aefx in the nebular phase at days past maximum light. Our Nea…

astro-ph.HE2022★ 29 cited

Optical/-ray blazar flare correlations: understanding the high-energy emission process using ASAS-SN and Fermi light curves

T. de Jaeger, B. J. Shappee, C. S. Kochanek +7

Using blazar light curves from the optical All-Sky Automated Survey for Supernovae (ASAS-SN) and the -ray \textit{Fermi}-LAT telescope, we performed the most extensive statistic…

astro-ph.HE2022★ 18 cited

The ASAS-SN Bright Supernova Catalog -- V. 2018-2020

K. D. Neumann, T. W. -S. Holoien, C. S. Kochanek +55

We catalog the 443 bright supernovae discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) in along with the 519 supernovae recovered by ASAS-SN and 516 a…

astro-ph.HE2016★ 58 cited

The ASAS-SN Bright Supernova Catalog II. 2015

T. W. -S. Holoien, J. S. Brown, K. Z. Stanek +41

This manuscript presents information for all supernovae discovered by the All-Sky Automated Survey for SuperNovae (ASAS-SN) during 2015, its second full year of operations. The sam…

astro-ph.HE2016★ 68 cited

The Long Term Evolution of ASASSN-14li

J. S. Brown, T. W. -S Holoien, K. Auchettl +5

We present late-time optical spectroscopy taken with the Large Binocular Telescope's Multi-Object Double Spectrograph, late-time SWIFT UVOT and XRT observations, as well as improve…