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20232026
most citedNear-Discovery SOAR Photometry of the Third Interstellar Object: 3I/ATLAS

6 citations · 13 across the 11 of their papers we have counts for

collaborators

13 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.HE2026

The First Multi-Messenger Nova: External Shocks, TeV Photons, and Neutrinos in the Next Eruption of T CrB

E. Aydi, P. Craig, K. V. Sokolovsky +10

T Coronae Borealis is the most compelling anticipated Galactic recurrent nova and one of the best opportunities to test whether nova eruptions can become genuine multi-messenger tr…

astro-ph.SR2026

From Light to Sound: Spectroscopic Evolution & Sonification of the flaring Nova V612 Scuti

Pragati Acharya, Elias Aydi, Kirill V. Sokolovsky +17

We present photometric and spectroscopic observations of the 2017 Galactic nova V612 Sct, whose optical evolution was marked by multiple unusually large maxima. The eruption includ…

astro-ph.SR2026

TESS detection of periodic brightness variations during the rise of classical nova PGIR22akgylf

Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev +14

Classical novae are transient events powered by thermonuclear burning in a layer of hydrogen-rich material accreted by a white dwarf from its binary companion. Most classical novae…

astro-ph.HE2026

Shocks in the Symbiotic Recurrent Nova V3890 Sgr: VLBI Radio Imaging and Fermi GeV Gamma-Rays

Isabella Molina, Peter Craig, Rebecca Diesing +14

We present very long baseline interferometric (VLBI) radio imaging and Fermi/LAT GeV -ray observations of the 2019 eruption of the symbiotic recurrent nova V3890 Sgr.The VLBI im…

astro-ph.HE2025★ 1 cited

Optical Study of TRAPUM Pulsars and Modelling of the Redbacks: PSR J10364353 and PSR J18036707

A. Phosrisom, R. P. Breton, C. J. Clark +12

The Transients and Pulsars with MeerKAT (TRAPUM) project discovered eight binary millisecond pulsars in its first shallow \textit{L}-band survey of unidentified \textit{Fermi} -…

astro-ph.EP2025★ 6 cited

Near-Discovery SOAR Photometry of the Third Interstellar Object: 3I/ATLAS

Tessa T. Frincke, Atsuhiro Yaginuma, John W. Noonan +7

3I/ATLAS was discovered on UT 2025 July 1 and joins a limited but growing population of detected m scale interstellar objects. In this paper we report photometric o…

astro-ph.HE2025★ 5 cited

Multiwavelength Evidence for Two New Candidate Transitional Millisecond Pulsars in the Sub-luminous Disk State: 4FGL J0639.1--8009 and 4FGL J1824.2+1231

Rebecca Kyer, Subhroja Roy, Jay Strader +4

We report the discovery of two new Galactic accreting compact objects consistent with the respective positions of the unassociated Fermi-LAT gamma-ray sources 4FGL J0639.1--8009 an…

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

Do Neutron Star Ultra-Luminous X-Ray Sources Masquerade as Intermediate Mass Black Holes in Radio and X-Ray?

Teresa Panurach, Kristen C. Dage, Ryan Urquhart +8

Ultraluminous X-ray sources (ULXs) were once largely believed to be powered by super-Eddington accretion onto stellar-mass black holes, although in some rare cases, ULXs also serve…

astro-ph.HE2024

The Symbiotic Recurrent Nova V745 Sco at Radio Wavelengths

Isabella Molina, Laura Chomiuk, Justin D. Linford +14

V745 Sco is a Galactic symbiotic recurrent nova with nova eruptions in 1937, 1989 and 2014. We study the behavior of V745 Sco at radio wavelengths (0.6-37,GHz), covering both its 1…

astro-ph.SR2024★ 1 cited

A Survey for Radio Emission from White Dwarfs in the VLA Sky Survey

Ingrid Pelisoli, Laura Chomiuk, Jay Strader +22

Radio emission has been detected from tens of white dwarfs, in particular in accreting systems. Additionally, radio emission has been predicted as a possible outcome of a planetary…

astro-ph.SR2023

TESS photometry of the nova eruption in V606 Vul: asymmetric photosphere and multiple ejections?

Kirill V. Sokolovsky, Elias Aydi, Konstantin Malanchev +70

Lightcurves of many classical novae deviate from the canonical "fast rise - smooth decline" pattern and display complex variability behavior. We present the first TESS-space-photom…