activity
20162026
most citedOptical spectroscopy and demographics of redback millisecond pulsar binaries

117 citations · 770 across the 30 of their papers we have counts for

collaborators

33 papers

astro-ph.HE2026

Three New Likely Spider Millisecond Pulsar Binaries and Optical Kinematic Tracers of Intrabinary Shocks

Jay Strader, Rebecca Kyer, Laura Chomiuk +9

We report the discovery of three candidate spider millisecond pulsars via multi-wavelength follow-up of unassociated Fermi Large Area Telescope gamma-ray sources. All have optical…

astro-ph.HE2025

Radio Observations of a Candidate Redback Millisecond Pulsar: 1FGL J0523.5-2529

O. A. Johnson, E. F. Keane, D. J. McKenna +4

Redback pulsars are a subclass of millisecond pulsar system with a low-mass non-degenerate companion star being ablated by the pulsar. They are of interest due to the insights they…

astro-ph.HE2025

PSR J1947-1120: A New Huntsman Millisecond Pulsar Binary

Jay Strader, Paul S. Ray, Ryan Urquhart +11

We present the discovery of PSR J1947-1120, a new huntsman millisecond pulsar with a red giant companion star in a 10.3 d orbit. This pulsar was found via optical, X-ray, and radio…

astro-ph.HE2024

Mass estimates from optical modelling of the new TRAPUM redback PSR J1910-5320

O. G. Dodge, R. P. Breton, C. J. Clark +17

Spider pulsars continue to provide promising candidates for neutron star mass measurements. Here we present the discovery of PSR~J19105320, a new millisecond pulsar discovered i…

astro-ph.HE2022★ 17 cited

Multi-Wavelength Observations Of A New Redback Millisecond Pulsar 4FGL J1910.7-5320

Ka-Yui Au, Jay Strader, Samuel J. Swihart +9

We present the study of multi-wavelength observations of an unidentified Fermi Large Area Telescope (LAT) source, 4FGL J1910.7-5320, a new candidate redback millisecond pulsar bina…

astro-ph.HE2022★ 38 cited

A New Flaring Black Widow Candidate and Demographics of Black Widow Millisecond Pulsars in the Galactic Field

Samuel J. Swihart, Jay Strader, Laura Chomiuk +4

We present the discovery of a new optical/X-ray source likely associated with the Fermi -ray source 4FGL J1408.6-2917. Its high-amplitude periodic optical variability, large spe…

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.SR2022★ 8 cited

1RXH J082623.6-505741: a new long-period cataclysmic variable with an evolved donor and a low mass transfer rate

Kirill V. Sokolovsky, Jay Strader, Samuel J. Swihart +13

We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a K-t…

astro-ph.SR2022★ 1 cited

UGPS J194310+183851: an Unusual Optical and X-ray Faint Cataclysmic Variable?

C. Morris, T. J. Maccarone, P. W. Lucas +7

The growing number of multi-epoch optical and infrared sky surveys are uncovering unprecedented numbers of new variable stars, of an increasing number of types. The short interval…

astro-ph.HE2022★ 50 cited

A Gamma-ray Pulsar Timing Array Constrains the Nanohertz Gravitational Wave Background

M. Ajello, W. B. Atwood, L. Baldini +129

After large galaxies merge, their central supermassive black holes are expected to form binary systems whose orbital motion generates a gravitational wave background (GWB) at nanoh…

astro-ph.HE2022★ 17 cited

Gamma-ray Eclipses and Orbital Modulation Transitions in the Candidate Redback 4FGL J1702.7-5655

R. H. D. Corbet, L. Chomiuk, J. B. Coley +8

Observations with the Fermi Large Area Telescope (LAT) of the gamma-ray source 4FGL J1702.7-5655, previously classified as a candidate millisecond pulsar, show highly-significant m…

astro-ph.HE2022★ 18 cited

Discovery, Timing, and Multiwavelength Observations of the Black Widow Millisecond Pulsar PSR J1555-2908

Paul S. Ray, Lars Nieder, Colin J. Clark +21

We report the discovery of PSR J1555-2908, a 1.79 ms radio and gamma-ray pulsar in a 5.6 hr binary system with a minimum companion mass of 0.052 . This fast and energetic…

astro-ph.HE2022★ 11 cited

4FGL J1120.0-2204: A Unique Gamma-ray Bright Neutron Star Binary with an Extremely Low Mass Proto-White Dwarf

Samuel J. Swihart, Jay Strader, Elias Aydi +5

We have discovered a new X-ray emitting compact binary that is the likely counterpart to the unassociated Fermi-LAT GeV -ray source 4FGL J1120.0-2204, the second brightest Fermi…

astro-ph.HE2021★ 14 cited

Multiwavelength evidence for a new flare-mode transitional millisecond pulsar

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

We report the discovery of a new low-mass X-ray binary near the center of the unassociated Fermi GeV gamma-ray source 4FGL J0540.0-7552. The source shows the persistent presence of…

astro-ph.SR2021★ 24 cited

The Loudest Stellar Heartbeat: Characterizing the most extreme amplitude heartbeat star system

T. Jayasinghe, C. S. Kochanek, J. Strader +16

We characterize the extreme heartbeat star system MACHO 80.7443.1718 in the LMC using TESS photometry and spectroscopic observations from the Magellan Inamori Kyocera Echelle (MIKE…

astro-ph.HE2021★ 23 cited

Discovery of a New Redback Millisecond Pulsar Candidate: 4FGL J0940.3-7610

Samuel J. Swihart, Jay Strader, Elias Aydi +3

We have discovered a new candidate redback millisecond pulsar binary near the center of the error ellipse of the bright unassociated Fermi-LAT -ray source 4FGL J0940.3-7610. The…

astro-ph.IM2020★ 8 cited

Identifying Candidate Optical Variables Using Gaia Data Release 2

Shion Andrew, Samuel J. Swihart, Jay Strader

Gaia is undertaking a deep synoptic survey of the Galaxy, but photometry from individual epochs has, as of yet, only been released for a minimal number of sources. We show that it…

astro-ph.HE2020★ 74 cited

Early spectral evolution of classical novae: consistent evidence for multiple distinct outflows

E. Aydi, L. Chomiuk, L. Izzo +18

The physical mechanism driving mass ejection during a nova eruption is still poorly understood. Possibilities include ejection in a single ballistic event, a common envelope intera…

astro-ph.HE2020★ 25 cited

A New Candidate Transitional Millisecond Pulsar in the Sub-luminous Disk State: 4FGL J0407.7--5702

Jessie M. Miller, Samuel J. Swihart, Jay Strader +7

We report the discovery of a variable optical and X-ray source within the error ellipse of the previously unassociated Fermi Large Area Telescope -ray source 4FGL J0407.7--5702.…

astro-ph.HE2020★ 19 cited

The MAVERIC Survey: New compact binaries revealed by deep radio continuum observations of the Galactic globular cluster Terzan 5

Ryan Urquhart, Arash Bahramian, Jay Strader +12

Owing to its massive, dense core, Terzan 5 has the richest population of millisecond pulsars known among Galactic globular clusters. Here we report new deep GHz radio contin…

astro-ph.HE2020★ 19 cited

The Swift Bulge Survey: optical and near-IR follow-up featuring a likely symbiotic X-ray binary & a focused wind CV

A. W. Shaw, C. O. Heinke, T. J. Maccarone +13

The nature of very faint X-ray transients (VFXTs) - transient X-ray sources that peak at luminosities - is poorly understood. The faint and of…

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★ 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

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-…