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20092026
most citedAn Ultraluminous X-ray Source Powered by An Accreting Neutron Star

767 citations · 5.3k across the 102 of their papers we have counts for

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Showing 2016Show all

9 papers · 1 filter

astro-ph.HE2016★ 18 cited

The nova-like nebular optical spectrum of V404 Cygni at the beginning of the 2015 outburst decay

F. Rahoui, J. A. Tomsick, P. Gandhi +7

We report on FORS2 optical spectroscopy of the black hole X-ray binary V404 Cygni, performed at the very beginning of its 2015 outburst decay, complemented by quasi-simultaneous $S…

astro-ph.HE2016★ 81 cited

Spectral Changes in the Hyperluminous Pulsar in NGC 5907 as a Function of Super-Orbital Phase

F. Fuerst, D. J. Walton, D. Stern +5

We present broad-band, multi-epoch X-ray spectroscopy of the pulsating ultra-luminous X-ray source (ULX) in NGC 5907. Simultaneous XMM-Newton and NuSTAR data from 2014 are best des…

astro-ph.HE2016★ 18 cited

GRS 1739-278 observed at very low luminosity with XMM-Newton and NuSTAR

F. Fuerst, J. A. Tomsick, K. Yamaoka +19

We present a detailed spectral analysis of XMM-Newton and NuSTAR observations of the accreting transient black hole GRS 1739-278 during a very faint low hard state at ~0.02% of the…

astro-ph.HE2016★ 92 cited

Living on a Flare: Relativistic Reflection in V404 Cyg Observed by NuSTAR During its Summer 2015 Outburst

D. J. Walton, K. Mooley, A. L. King +19

We present first results from a series of observations of the black hole X-ray binary V404 Cyg obtained during its summer 2015 outburst, primarily focusing on observations…

astro-ph.HE2016★ 75 cited

A 78 Day X-ray Period Detected from NGC 5907 ULX1 by Swift

D. J. Walton, F. Fuerst, M. Bachetti +12

We report the detection of a day period in the X-ray lightcurve of the extreme ultraluminous X-ray source NGC 5907 ULX1 ( erg s$^{-1…

astro-ph.HE2016★ 33 cited

A broadband X-ray spectral study of the intermediate-mass black hole candidate M82 X-1 with NuSTAR, Chandra and Swift

Murray Brightman, Fiona A. Harrison, Didier Barret +8

M82 X-1 is one of the brightest ultraluminous X-ray sources (ULXs) known, which, assuming Eddington-limited accretion and other considerations, makes it one of the best intermediat…

astro-ph.SR2016★ 21 cited

An extremely fast halo hot subdwarf star in a wide binary system

Péter Németh, Eva Ziegerer, Andreas Irrgang +4

New spectroscopic observations of the halo hyper-velocity star candidate SDSS J121150.27+143716.2 ( mag) revealed a cool companion to the hot subdwarf primary. The compone…

astro-ph.HE2016★ 131 cited

NuSTAR and Swift observations of the very high state in GX 339-4: Weighing the black hole with X-rays

M. L. Parker, J. A. Tomsick, J. A. Kennea +14

We present results from spectral fitting of the very high state of GX~339-4 with NuSTAR and Swift. We use relativistic reflection modelling to measure the spin of the black hole an…

astro-ph.HE2016★ 32 cited

A low-luminosity soft state in the short period black hole X-ray binary Swift J1753.5-0127

A. W. Shaw, P. Gandhi, D. Altamirano +6

We present results from the spectral fitting of the candidate black hole X-ray binary Swift J1753.5-0127 in an accretion state previously unseen in this source. We fit the 0.7-78 k…