activity
20022026
most citedLSST Science Book, Version 2.0

924 citations · 17.8k across the 309 of their papers we have counts for

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Showing 2019 · astro-ph.HEShow all

14 papers · 2 filters

astro-ph.HE2019★ 13 cited

GS 2000+25: The Least Luminous Black Hole X-ray Binary

J. Rodriguez, R. Urquhart, R. M. Plotkin +6

Little is known about the properties of the accretion flows and jets of the lowest-luminosity quiescent black holes. We report new, strictly simultaneous radio and X-ray observatio…

astro-ph.HE2019★ 21 cited

A New Likely Redback Millisecond Pulsar Binary with a Massive Neutron Star: 4FGL J2333.1--5527

Samuel J. Swihart, Jay Strader, Ryan Urquhart +7

We present the discovery of a likely new redback millisecond pulsar binary associated with the \emph{Fermi} -ray source 4FGL J2333.1--5527. Using optical photometric and spectro…

astro-ph.HE2019★ 10 cited

Slow Decline and Rise of the Broad [OIII] Emission Line in Globular Cluster Black Hole Candidate RZ2109

Kristen C. Dage, Stephen E. Zepf, Arash Bahramian +6

RZ2109 is the first of several extragalactic globular clusters shown to host an ultraluminous X-ray source. RZ2109 is particularly notable because optical spectroscopy shows it has…

astro-ph.HE2019★ 102 cited

The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin

Wen-fai Fong, P. K. Blanchard, K. D. Alexander +25

We present a revised and complete optical afterglow light curve of the binary neutron star merger GW170817, enabled by deep Hubble Space Telescope (HST) F606W observations at $\app…

astro-ph.HE2019★ 63 cited

Searches After Gravitational-waves Using ARizona Observatories (SAGUARO): System Overview and First Results from Advanced LIGO/Virgo's Third Observing Run

M. J. Lundquist, K. Paterson, W. Fong +53

We present Searches After Gravitational-waves Using ARizona Observatories (SAGUARO), a comprehensive effort dedicated to the discovery and characterization of optical counterparts…

astro-ph.HE2019★ 1 cited

Supersoft X-ray emission from a white dwarf binary not powered by nuclear fusion

Thomas J. Maccarone, Thomas J. Nelson, Peter J. Brown +17

Supersoft X-ray sources are stellar objects which emit X-rays with temperatures of about 1 million Kelvin and luminosities well in excess of what can be produced by stellar coronae…

astro-ph.HE2019★ 53 cited

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…

astro-ph.HE2019★ 27 cited

The Most Rapidly Declining Type I Supernova 2019bkc/ATLAS19dqr

Ping Chen, Subo Dong, M. D. Stritzinger +21

We report observations of the hydrogen-deficient supernova (SN) 2019bkc/ATLAS19dqr. With B- and r-band decline between peak and 10 days post peak of Delta m_10(B)=5.24+/-0.07 mag a…

astro-ph.HE2019★ 1 cited

Astro2020 Science White Paper: Populations of Black Holes in Binaries

Thomas J. Maccarone, Laura Chomiuk, James Miller-Jones +9

Black holes in binary star systems are vital for understanding the process of pr oducing gravitational wave sources, understanding how supernovae work, and for p roviding fossil ev…

astro-ph.HE2019★ 107 cited

Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS

Thomas W. -S. Holoien, Patrick J. Vallely, Katie Auchettl +22

We present the discovery and early evolution of ASASSN-19bt, a tidal disruption event (TDE) discovered by the All-Sky Automated Survey for Supernovae (ASAS-SN) at a distance of $d\…

astro-ph.HE2019

Flaring, Dust Formation, And Shocks In The Very Slow Nova ASASSN-17pf (LMCN 2017-11a)

E. Aydi, L. Chomiuk, J. Strader +25

We present a detailed study of the 2017 eruption of the classical nova ASASSN-17pf (LMCN 2017-11a), which is located in the Large Magellanic Cloud, including data from AAVSO, ASAS-…

astro-ph.HE2019★ 19 cited

PSR J1306--40: An X-ray Luminous Redback with an Evolved Companion

Samuel J. Swihart, Jay Strader, Laura Chomiuk +1

PSR J1306--40 is a millisecond pulsar binary with a non-degenerate companion in an unusually long 1.097 day orbit. We present new optical photometry and spectroscopy of this…

astro-ph.HE2019★ 4 cited

Radio Pulsar Populations

D. R. Lorimer, N. Pol, K. Rajwade +9

Our understanding of the neutron star population is informed to a great degree by large-scale surveys that have been carried out by radio facilities during the past fifty years. We…

astro-ph.HE2019★ 117 cited

Optical spectroscopy and demographics of redback millisecond pulsar binaries

Jay Strader, Samuel J. Swihart, Laura Chomiuk +12

We present the first optical spectroscopy of five confirmed (or strong candidate) redback millisecond pulsar binaries, obtaining complete radial velocity curves for each companion…