activity
19992026
most citedX-ray Binary Evolution Across Cosmic Time

279 citations · 1.1k across the 43 of their papers we have counts for

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8 papers · 1 filter

astro-ph.HE2026

Ultraluminous X-ray sources in the first eROSITA survey I. Candidate catalogs

P. Weber, T. P. Roberts, S. Hämmerich +28

Ultraluminous X-ray sources (ULXs) are luminous non-nuclear X-ray point sources embedded in galaxies. Their luminosities exceeding 10^39 erg/s potentially require sub-Eddington acc…

astro-ph.HE2023★ 1 cited

The High Energy X-ray Probe: Resolved X-ray Populations in Extragalactic Environments

Bret D. Lehmer, Kristen Garofali, Breanna A. Binder +15

We construct simulated galaxy data sets based on the High Energy X-ray Probe (HEX-P) mission concept to demonstrate the significant advances in galaxy science that will be yielded…

astro-ph.HE2019★ 17 cited

Neutron Stars and Black Holes in the Small Magellanic Cloud: The SMC NuSTAR Legacy Survey

M. Lazzarini, B. F. Williams, A. E. Hornschemeier +18

We present a source catalog from the first deep hard X-ray ( keV) survey of the Small Magellanic Cloud (SMC), the NuSTAR Legacy Survey of the SMC. We observed three fields, f…

astro-ph.HE2018★ 20 cited

A long hard-X-ray look at the dual active galactic nuclei of M51 with NuSTAR

M. Brightman, M. Baloković, M. Koss +14

We present a broadband X-ray spectral analysis of the M51 system, including the dual active galactic nuclei (AGN) and several off-nuclear point sources. Using a deep observation by…

astro-ph.HE2016★ 43 cited

Long-term optical variability of high-mass X-ray binaries. II. Spectroscopy

P. Reig, A. Nersesian, A. Zezas +2

We present the results of our monitoring program to study the long-term variability of the Halpha line in high-mass X-ray binaries. We have carried out the most complete optical sp…

astro-ph.HE2013★ 15 cited

Disc-loss episode in the Be shell optical counterpart to the high-mass X-ray binary IGR J21343+4738

P. Reig, A. Zezas

The main goal of this work is to determine the properties of the optical counterpart to the INTEGRAL source IGR J21343+4738, and study its long-term optical variability. We present…