activity
20062024
most citedA fast radio burst associated with a Galactic magnetar

767 citations · 6.7k across the 123 of their papers we have counts for

collaborators
Showing 2020Show all

10 papers · 1 filter

astro-ph.GA2020★ 95 cited

Quasars That Have Transitioned from Radio-quiet to Radio-loud on Decadal Timescales Revealed by VLASS and FIRST

Kristina Nyland, Dillon Z. Dong, Pallavi Patil +21

We have performed a search over 3440 deg of Epoch 1 (2017-2019) of the Very Large Array Sky Survey to identify unobscured quasars in the optical () and obscured…

astro-ph.SR2020★ 15 cited

Imaging Spectroscopy of CME-Associated Solar Radio Bursts

Sherry Chhabra, Dale E. Gary, Gregg Hallinan +4

We present first results of a solar radio event observed with the Owens Valley Radio Observatory Long Wavelength Array (OVRO-LWA) at metric wavelengths. We examine a complex event…

astro-ph.SR2020★ 13 cited

Detection of 24 GHz Continuum Emission from Eridani

Akshay Suresh, Shami Chatterjee, James M. Cordes +2

The nearby star has been a frequent target of radio surveys for stellar emission and extraterrestial intelligence. Using deep observations with the…

astro-ph.HE2020★ 13 cited

The JAGWAR Prowls LIGO/Virgo O3 Paper I: Radio Search of a Possible Multi-Messenger Counterpart of the Binary Black Hole Merger Candidate S191216ap

D. Bhakta, K. P. Mooley, A. Corsi +7

We present a sensitive search with the Karl G. Jansky Very Large Array (VLA) for the radio counterpart of the gravitational wave candidate S191216ap, classified as a binary black h…

astro-ph.SR2020★ 16 cited

On the Correlation between L Dwarf Optical and Infrared Variability and Radio Aurorae

Tyler Richey-Yowell, Melodie M. Kao, J. Sebastian Pineda +2

Photometric variability attributed to cloud phenomena is common in L/T transition brown dwarfs. Recent studies show that such variability may also trace aurorae, suggesting that lo…

astro-ph.GA2020★ 21 cited

Caltech-NRAO Stripe 82 Survey (CNSS). IV. The Birth of Radio-loud Quasar 013815+00

Magdalena Kunert-Bajraszewska, Aleksandra Wolowska, Kunal Mooley +2

It is believed that the gas accretion onto the supermassive black holes (SMBHs) is the main process of powering its luminous emission, which occurs in optical, UV and X-ray regimes…