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20002026
most citedThe Evolution of Normal Galaxy X-ray Emission Through Cosmic History: Constraints from the 6 Ms Chandra Deep Field-South

230 citations · 2k across the 69 of their papers we have counts for

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Showing 2019Show all

6 papers · 1 filter

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.HE2019★ 4 cited

Broad Band X-ray Constraints on the Accreting Black Hole in Quasar 4C 74.26

P. Tzanavaris, T. Yaqoob, S. LaMassa +2

X-ray data for quasar 4C 74.26 have previously been modeled with a broad Fe K emission line and reflection continuum originating in the inner part of the accretion disk around t…

astro-ph.GA2019★ 125 cited

X-ray Binary Luminosity Function Scaling Relations for Local Galaxies Based on Subgalactic Modeling

Bret D. Lehmer, Rafael T. Eufrasio, Panayiotis Tzanavaris +7

We present new Chandra constraints on the X-ray luminosity functions (XLFs) of X-ray binary (XRB) populations, and their scaling relations, for a sample of 38 nearby galaxies (D =…

astro-ph.HE2019

Astro 2020 Science White Paper: Time Domain Studies of Neutron Star and Black Hole Populations: X-ray Identification of Compact Object Types

N. Vulic, A. E. Hornschemeier, V. Antoniou +16

What are the most important conditions and processes governing the growth of stellar-origin compact objects? The identification of compact object type as either black hole (BH) or…

astro-ph.GA2019

Astro2020: Hot Drivers of Stellar Feedback from 10 to 10,000 pc

Edmund Hodges-Kluck, Laura A. Lopez, Mihoko Yukita +5

Stellar feedback -- stars regulating further star formation through the injection of energy and momentum into the interstellar medium -- operates through a complex set of processes…

astro-ph.HE2019★ 46 cited

A ~60-day super-orbital period originating from the ultraluminous X-ray pulsar in M82

Murray Brightman, Fiona A. Harrison, Matteo Bachetti +6

Ultraluminous X-ray (ULX) pulsars are a new class of object powered by apparent super-critical accretion onto magnetized neutron stars. Three sources in this class identified so fa…