output
19922026
most citedAdam: A Method for Stochastic Optimization

83.4k citations

Showing 2020 · astro-ph.HEShow all

49 papers · 2 filters

astro-ph.HE2020★ 37 cited

Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run

K. Paterson, M. J. Lundquist, J. C. Rastinejad +34

With the conclusion of the third observing run for Advanced LIGO/Virgo (O3), we present a detailed analysis of both triggered and serendipitous observations of 17 gravitational wav…

astro-ph.HE2020★ 9 cited

Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers

N. J. Klingler, A. Lien, S. R. Oates +41

On 2020 February 24, during their third observing run ("O3"), the Laser Interferometer Gravitational-wave Observatory and Virgo Collaboration (LVC) detected S200224ca: a candidate…

astro-ph.HE2020★ 24 cited

The NANOGrav 12.5-Year Data Set: Monitoring Interstellar Scattering Delays

Jacob E. Turner, Maura A. McLaughlin, James M. Cordes +33

We extract interstellar scintillation parameters for pulsars observed by the NANOGrav radio pulsar timing program. Dynamic spectra for the observing epochs of each pulsar were used…

astro-ph.HE2020★ 180 cited

LOFAR Detection of 110-188 MHz Emission and Frequency-Dependent Activity from FRB 20180916B

Z. Pleunis, D. Michilli, C. G. Bassa +32

FRB 20180916B is a well-studied repeating fast radio burst source. Its proximity (~150 Mpc), along with detailed studies of the bursts, have revealed many clues about its nature --…

astro-ph.HE2020★ 34 cited

First discovery of new pulsars and RRATs with CHIME/FRB

D. C. Good, B. C. Andersen, P. Chawla +20

We report the discovery of seven new Galactic pulsars with the Canadian Hydrogen Intensity Mapping Experiment's Fast Radio Burst backend (CHIME/FRB). These sources were first ident…

astro-ph.HE2020★ 45 cited

Dispersion measure variability for 36 millisecond pulsars at 150MHz with LOFAR

J. Y. Donner, J. P. W. Verbiest, C. Tiburzi +19

Radio pulses from pulsars are affected by plasma dispersion, which results in a frequency-dependent propagation delay. Variations in the magnitude of this effect lead to an additio…