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20012019
most citedA gravitational-wave standard siren measurement of the Hubble constant

1.2k citations · 1.7k across the 9 of their papers we have counts for

collaborators

9 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.CO2017★ 1.2k cited

A gravitational-wave standard siren measurement of the Hubble constant

B. P. Abbott, R. Abbott, T. D. Abbott +1308

The detection of GW170817 in both gravitational waves and electromagnetic waves heralds the age of gravitational-wave multi-messenger astronomy. On 17 August 2017 the Advanced LIGO…

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-ph2007★ 20 cited

Investigating the nature of absorption lines in the Chandra X-ray spectra of the neutron star binary 4U 1820-30

E. M. Cackett, J. M. Miller, J. Raymond +5

We use four Chandra gratings spectra of the neutron star low-mass X-ray binary 4U 1820-30 to better understand the nature of certain X-ray absorption lines in X-ray binaries, inclu…

astro-ph2006★ 24 cited

A detection of the donor star of Aquila X-1 during its 2004 outburst?

R. Cornelisse, J. Casares, D. Steeghs +4

Phase-resolved high resolution optical spectroscopy has revealed narrow N III and He II emission lines from the soft X-ray transient Aquila X-1 during its 2004 outburst that move a…

astro-ph2005★ 11 cited

Optical identification of IGR J19140+0951

J. J. M. in 't Zand, P. G. Jonker, G. Nelemans +2

IGR J19140+0951 was discovered by INTEGRAL in 2003 in the 4-100 keV band. Observations with INTEGRAL and RXTE provide a tentative identification as a high-mass X-ray binary (HMXB)…