activity
20122026
most citedX-ray Properties of NGC 253's Starburst-Driven Outflow

33 citations · 279 across the 23 of their papers we have counts for

collaborators

21 papers

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.HE2024

A NuSTAR Census of the X-ray Binary Population of the M31 Disk

Hannah Moon, Daniel R. Wik, V. Antoniou +11

Using hard (E>10 keV) X-ray observations with NuSTAR, we are able to differentiate between accretion states, and thus compact object types, of neutron stars and black holes in X-ra…

astro-ph.GA2024★ 14 cited

The first all-sky survey of star-forming galaxies with eROSITA: Scaling relations and a population of X-ray luminous starbursts

E. Kyritsis, A. Zezas, F. Haberl +11

We present a study of X-ray normal galaxies using data from the first all-sky scan of the eROSITA X-ray survey. eRASS1 provides the first unbiased X-ray census of normal galaxies a…

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.GA2023

Modeling the High-Energy Ionizing Output from Simple Stellar and X-ray Binary Populations

Kristen Garofali, Antara R. Basu-Zych, Benjamin D. Johnson +9

We present a methodology for modeling the joint ionizing impact due to a "simple X-ray population" (SXP) and its corresponding simple stellar population (SSP), where "simple" refer…

astro-ph.HE2023★ 11 cited

Multiwavelength Characterization of the High Mass X-ray Binary Population of M33

Margaret Lazzarini, Kyros Hinton, Cheyanne Shariat +12

We present multi-wavelength characterization of 65 high mass X-ray binary (HMXB) candidates in M33. We use the Chandra ACIS survey of M33 (ChASeM33) catalog to select hard X-ray po…

astro-ph.HE2022★ 33 cited

X-ray Properties of NGC 253's Starburst-Driven Outflow

Sebastian Lopez, Laura A. Lopez, Dustin D. Nguyen +5

We analyze image and spectral data from 365~ks of observations from the {\it Chandra} X-ray Observatory of the nearby, edge-on starburst galaxy NGC 253 to constrain proper…

astro-ph.GA2021★ 20 cited

The eROSITA Final Equatorial-Depth Survey (eFEDS): Presenting The Demographics of X-ray Emission From Normal Galaxies

N. Vulic, A. E. Hornschemeier, F. Haberl +17

The Final Equatorial Depth Survey (eFEDS), completed during the calibration and performance verification phase of the instrument on $\it{Spectrum\, Ro…

astro-ph.HE2020★ 16 cited

Multiwavelength Characterization of the High Mass X-ray Binary Population of M31

Margaret Lazzarini, Benjamin F. Williams, Meredith Durbin +7

We present our analysis of high quality high mass X-ray binary (HMXB) candidates in M31 selected from point-source optical-counterpart candidates from the Chandra-PHAT survey catal…

astro-ph.HE2020★ 13 cited

On the X-ray Spectral Energy Distributions of Star-Forming Galaxies: the 0.3-30 keV Spectrum of the Low-Metallicity Starburst Galaxy VV 114

Kristen Garofali, Bret D. Lehmer, Antara Basu-Zych +6

Binary population synthesis combined with cosmological models suggest that X-ray emission from star-forming galaxies, consisting primarily of emission from X-ray binaries (XRBs) an…

astro-ph.GA2020★ 13 cited

The Next Generation X-ray Galaxy Survey with eROSITA

Antara R. Basu-Zych, Ann E. Hornschemeier, Frank Haberl +6

eROSITA, launched on 13 July 2019, will be completing the first all-sky survey in the soft and medium X-ray band in nearly three decades. This 4-year survey, finishing in late 2023…

astro-ph.GA2020★ 13 cited

Identifying New X-ray Binary Candidates in M31 using Random Forest Classification

R. M. Arnason, P. Barmby, N. Vulic

Identifying X-ray binary (XRB) candidates in nearby galaxies requires distinguishing them from possible contaminants including foreground stars and background active galactic nucle…

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

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.HE2018★ 11 cited

On the Nature of the X-ray Emission from the Ultraluminous X-ray Source, M33 X-8: New Constraints from NuSTAR and XMM-Newton

Lacey A. West, Bret D. Lehmer, Daniel Wik +12

We present nearly simultaneous NuSTAR and XMM-Newton observations of the nearby (832 kpc) ultraluminous X-ray source (ULX) M33 X-8. M33 X-8 has a 0.3-10 keV luminosity of LX ~ 1.4…

astro-ph.GA2018★ 19 cited

Comparing Chandra and Hubble in the Northern Disk of M31

Benjamin F. Williams, Margaret Lazzarini, Paul Plucinsky +9

The X-ray source populations within galaxies are typically difficult to identify and classify from X-ray data alone. We are able to break through this barrier by combining deep new…

astro-ph.GA2018★ 19 cited

Black Holes and Neutron Stars in Nearby Galaxies: Insights from NuSTAR

Neven Vulic, Ann E. Hornschemeier, Daniel R. Wik +8

Nearby galaxy surveys have long classified X-ray binaries (XRBs) by the mass category of their donor stars (high-mass and low-mass). The NuSTAR observatory, which provides imaging…

astro-ph.GA2017★ 6 cited

Milky Way Globular Cluster Metallicity and Low-Mass X-ray Binaries: The Red Giant Influence

Neven Vulic, Pauline Barmby, Sarah C. Gallagher

Galactic and extragalactic studies have shown that metal-rich globular clusters (GCs) are approximately three times more likely to host bright low-mass X-ray binaries (LMXBs) than…

astro-ph.GA2016★ 17 cited

X-Rays Beware: The Deepest Chandra Catalogue of Point Sources in M31

N. Vulic, S. C. Gallagher, P. Barmby

This study represents the most sensitive Chandra X-ray point source catalogue of M31. Using 133 publicly available Chandra ACIS-I/S observations totalling ~1 Ms, we detected 795 X-…

astro-ph.GA2014★ 6 cited

Faint X-ray Binaries and Their Optical Counterparts in M31

N. Vulic, S. C. Gallagher, P. Barmby

X-ray binaries (XRBs) are probes of both star formation and stellar mass, but more importantly remain one of the only direct tracers of the compact object population. To investigat…

astro-ph.CO2012★ 7 cited

Stacking Star Clusters in M51: Searching for Faint X-Ray Binaries

N. Vulic, P. Barmby, S. C. Gallagher

The population of low-luminosity (< 10^35 erg/s) X-Ray Binaries (XRBs) has been investigated in our Galaxy and M31 but not further. To address this problem, we have used data from…