activity
20002026
most citedA Huge Drop in X-ray Luminosity of the Non-Active Galaxy RXJ1242.6-1119A, and First Post-Flare Spectrum - Testing the Tidal Disruption Scenario

163 citations · 481 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026★ 2 cited

On the Deepest Search for Galactic Center Pulsars and an Examination of an Intriguing Millisecond Pulsar Candidate

Karen I. Perez, Vishal Gajjar, Slavko Bogdanov +6

We report results of one of the most sensitive pulsar surveys to date targeting the innermost region of the Galactic Center (GC) using the Robert C. Byrd Green Bank Telescope (GBT)…

astro-ph.HE2025

Noisy Timing Behavior is a Feature of Central Compact Object Pulsars

K. I. Perez, E. V. Gotthelf, J. P. Halpern

We present a timing study of the three known central compact object (CCO) pulsars, isolated cooling neutron stars in supernova remnants, using Chandra, XMM-Newton and NICER observa…

astro-ph.HE2024

The Proper Motion of the High Galactic Latitude Pulsar Calvera

Michela Rigoselli, Sandro Mereghetti, Jules P. Halpern +2

Calvera (1RXS J141256.0+792204) is a pulsar of characteristic age 285 kyr at a high Galactic latitude of b=+37°, detected only in soft thermal X-rays. We measure a new and precise…

astro-ph.HE2024

Resolving the Periods of the Asynchronous Polar 1RXS J083842.1282723

J. P. Halpern

1RXS J083842.1282723 is a nearly synchronous magnetic cataclysmic variable with a simple X-ray light curve. While its orbital period was fairly well established at $P_{\rm orb}=…

astro-ph.SR2023

A Surprising Periodicity Detected During a Super-outburst of V844 Herculis by TESS

A. Greiveldinger, P. Garnavich, C. Littlefield +6

We identify a previously undetected periodicity at a frequency of 49.080.01 d (period of 29.340.01 minutes) during a super-outburst of V844 Her observed by TESS. V…

astro-ph.HE2018★ 5 cited

The First Glitch in a Central Compact Object Pulsar: 1E 1207.4-5209

E. V. Gotthelf, J. P. Halpern

Since its discovery as a pulsar in 2000, the central compact object (CCO) 1E 1207.4-5209 in the supernova remnant PKS 1209-51/52 had been a stable 0.424 s rotator with an extremely…