activity
20032019
most citedObservatory science with eXTP

72 citations · 178 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2019★ 4 cited

Constraining the nature of the accreting binary in CXOGBS J174623.5-310550

M. A. P. Torres, S. Repetto, T. Wevers +12

We report optical and infrared observations of the X-ray source CXOGBS J174623.5-310550. This Galactic object was identified as a potential quiescent low-mass X-ray binary accretin…

astro-ph.HE2018★ 72 cited

Observatory science with eXTP

Jean J. M. in 't Zand, Enrico Bozzo, Jinlu Qu +181

In this White Paper we present the potential of the enhanced X-ray Timing and Polarimetry (eXTP) mission for studies related to Observatory Science targets. These include flaring s…

astro-ph.HE2017★ 7 cited

Candidate Hα emission and absorption line sources in the Galactic Bulge Survey

T. Wevers, P. G. Jonker, G. Nelemans +7

We present a catalogue of candidate Hα emission and absorption line sources and blue objects in the Galactic Bulge Survey (GBS) region. We use a point source catalogue of the GBS f…

astro-ph.HE2016★ 36 cited

Disk reflection and a possible disk wind during a soft X-ray state in the neutron star low-mass X-ray binary 1RXS J180408.9-342058

N. Degenaar, D. Altamirano, M. Parker +10

1RXS J180408.9-342058 is a transient neutron star low-mass X-ray binary that exhibited a bright accretion outburst in 2015. We present Nustar, Swift, and Chandra observations obtai…

astro-ph.HE2015

A Low-Mass Main-Sequence Star and Accretion Disk in the Very Faint Transient M15 X-3

Robin Arnason, Gregory Sivakoff, Craig Heinke +2

We present near-simultaneous Chandra/HST observations of the very faint ( erg s) X-ray transient source M15 X-3, as well as unpublished archival Chandra obs…

astro-ph.SR2009★ 16 cited

No Neutron Star Companion To The Lowest Mass SDSS White Dwarf

Marcel Agueros, Craig Heinke, Fernando Camilo +6

SDSS J091709.55+463821.8 (hereafter J0917+4638) is the lowest surface gravity white dwarf (WD) currently known, with log g = 5.55 +/- 0.05 (M ~ 0.17 M_sun; Kilic et al. 2007a,b). S…