activity
20232026
most citedExploration of faint X-ray and radio sources in the massive globular cluster M14: A UV-bright counterpart to Nova Ophiuchus 1938

2 citations · 4 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.HE20261 cited

A comprehensive search for high-velocity X-ray sources: New compact object binary candidates in the Gaia era

Yue Zhao, Poshak Gandhi, Christian Knigge +6

We perform a comprehensive search for high-velocity X-ray sources with large X-ray/optical flux ratios (), identifying candidates for interacting black h…

astro-ph.HE20251 cited

Further evidence for natal kick segregation by spectral type in high-mass X-ray binaries

Pornisara Nuchvanichakul, Poshak Gandhi, Christian Knigge +4

High-mass X-ray binaries (HMXBs) are systems in which a neutron star or black hole accretes material from a massive companion. HMXBs are expected to have experienced a supernova in…

astro-ph.HE2025

Optical Counterparts to X-ray sources in LSST DP1

Yuankun, Wang, Eric C. Bellm +9

We present a crossmatch between a combined catalog of X-ray sources and the Vera C. Rubin Observatory Data Preview 1 (DP1) to identify optical counterparts. The six fields targeted…

astro-ph.HE20242 cited

Exploration of faint X-ray and radio sources in the massive globular cluster M14: A UV-bright counterpart to Nova Ophiuchus 1938

Yue Zhao, Francesca D'Antona, Antonino P. Milone +4

Using a 12 ks archival Chandra X-ray Observatory ACIS-S observation on the massive globular cluster (GC) M14, we detect a total of 7 faint X-ray sources within its half-light radiu…

astro-ph.HE2023

On the natal kick of the black hole X-ray binary H 1705--250

Cordelia Dashwood Brown, Poshak Gandhi, Yue Zhao

When a compact object is formed, an impulse (kick) will be imparted to the system by the mass lost during the core-collapse supernova (SN). A number of other mechanisms may impart…