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1
High resolution stationary digital breast tomosynthesis using distributed carbon nanotube x-ray source array
High resolution stationary digital breast tomosynthesis using distributed carbon nanotube x-ray source array
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High resolution stationary digital breast tomosynthesis using distributed carbon nanotube x-ray source array

Medical physics (Lancaster), 2012-04, Vol.39 (4), p.2090-2099 [Peer Reviewed Journal]

American Association of Physicists in Medicine ;2012 American Association of Physicists in Medicine ;Copyright © 2012 American Association of Physicists in Medicine 2012 American Association of Physicists in Medicine ;ISSN: 0094-2405 ;EISSN: 2473-4209 ;DOI: 10.1118/1.3694667 ;PMID: 22482630 ;CODEN: MPHYA6

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2
Hard X-Ray Excess from the Magnificent Seven Neutron Stars
Hard X-Ray Excess from the Magnificent Seven Neutron Stars
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Hard X-Ray Excess from the Magnificent Seven Neutron Stars

The Astrophysical journal, 2020-11, Vol.904 (1), p.42 [Peer Reviewed Journal]

2020. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Nov 01, 2020 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abb4ea

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3
The Long Stare at Hercules X-1. I. Emission Lines from the Outer Disk, the Magnetosphere Boundary, and the Accretion Curtain
The Long Stare at Hercules X-1. I. Emission Lines from the Outer Disk, the Magnetosphere Boundary, and the Accretion Curtain
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The Long Stare at Hercules X-1. I. Emission Lines from the Outer Disk, the Magnetosphere Boundary, and the Accretion Curtain

The Astrophysical journal, 2022-09, Vol.936 (2), p.185 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac897e

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4
Monitoring the X-Ray Variability of Bright X-Ray Sources in M33
Monitoring the X-Ray Variability of Bright X-Ray Sources in M33
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Monitoring the X-Ray Variability of Bright X-Ray Sources in M33

The Astrophysical journal, 2024-02, Vol.961 (2), p.168 [Peer Reviewed Journal]

2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ad151a

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5
Elevated Hot Gas and High-mass X-Ray Binary Emission in Low-metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe
Elevated Hot Gas and High-mass X-Ray Binary Emission in Low-metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe
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Elevated Hot Gas and High-mass X-Ray Binary Emission in Low-metallicity Galaxies: Implications for Nebular Ionization and Intergalactic Medium Heating in the Early Universe

The Astrophysical journal, 2022-05, Vol.930 (2), p.135 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac63a7

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6
The Redshift Evolution of Ultraluminous X-Ray Sources out to z ∼ 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background
The Redshift Evolution of Ultraluminous X-Ray Sources out to z ∼ 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background
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The Redshift Evolution of Ultraluminous X-Ray Sources out to z ∼ 0.5: Comparison with X-Ray Binary Populations and Contribution to the Cosmic X-Ray Background

The Astrophysical journal, 2022-06, Vol.932 (1), p.27 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac6bed

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7
Young Black Hole and Neutron Star Systems in the Nearby Star-forming Galaxy M33: The NuSTAR View
Young Black Hole and Neutron Star Systems in the Nearby Star-forming Galaxy M33: The NuSTAR View
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Young Black Hole and Neutron Star Systems in the Nearby Star-forming Galaxy M33: The NuSTAR View

The Astrophysical journal, 2022-05, Vol.930 (1), p.64 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac6351

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8
Observations of 4U 1626–67 with the Imaging X-Ray Polarimetry Explorer
Observations of 4U 1626–67 with the Imaging X-Ray Polarimetry Explorer
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Observations of 4U 1626–67 with the Imaging X-Ray Polarimetry Explorer

The Astrophysical journal, 2022-11, Vol.940 (1), p.70 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac98c2

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9
Pulsator-like Spectra from Ultraluminous X-Ray Sources and the Search for More Ultraluminous Pulsars
Pulsator-like Spectra from Ultraluminous X-Ray Sources and the Search for More Ultraluminous Pulsars
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Pulsator-like Spectra from Ultraluminous X-Ray Sources and the Search for More Ultraluminous Pulsars

The Astrophysical journal, 2017-02, Vol.836 (1), p.113 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Feb 10, 2017 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/836/1/113

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10
Origin and Composition of the Galactic Diffuse X-Ray Emission Spectra by Unresolved X-Ray Sources
Origin and Composition of the Galactic Diffuse X-Ray Emission Spectra by Unresolved X-Ray Sources
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Origin and Composition of the Galactic Diffuse X-Ray Emission Spectra by Unresolved X-Ray Sources

The Astrophysical journal, 2024-02, Vol.961 (2), p.205 [Peer Reviewed Journal]

2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ad0dff

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11
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification
Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification
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Population of X-Ray Sources in the Intermediate-age Cluster NGC 3532: a Test Bed for Machine-learning Classification

The Astrophysical journal, 2023-05, Vol.948 (1), p.59 [Peer Reviewed Journal]

2023. The Author(s). Published by the American Astronomical Society. ;2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/acb3a6

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12
The eROSITA X-ray telescope on SRG
The eROSITA X-ray telescope on SRG
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The eROSITA X-ray telescope on SRG

Astronomy and astrophysics (Berlin), 2021-03, Vol.647 (A1) [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/202039313

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13
X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei
X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei
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X-Ray Coronal Properties of Swift/BAT-selected Seyfert 1 Active Galactic Nuclei

The Astrophysical journal, 2022-03, Vol.927 (1), p.42 [Peer Reviewed Journal]

2022. The Author(s). Published by the American Astronomical Society. ;2022. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac45f6

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14
Constraining the White-dwarf Mass and Magnetic Field Strength of a New Intermediate Polar through X-Ray Observations
Constraining the White-dwarf Mass and Magnetic Field Strength of a New Intermediate Polar through X-Ray Observations
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Constraining the White-dwarf Mass and Magnetic Field Strength of a New Intermediate Polar through X-Ray Observations

The Astrophysical journal, 2023-09, Vol.954 (2), p.138 [Peer Reviewed Journal]

2023. The Author(s). Published by the American Astronomical Society. ;2023. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ace90c

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15
Optical Analysis and Modeling of HD96670, a New Black Hole X-Ray Binary Candidate
Optical Analysis and Modeling of HD96670, a New Black Hole X-Ray Binary Candidate
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Optical Analysis and Modeling of HD96670, a New Black Hole X-Ray Binary Candidate

The Astrophysical journal, 2021-05, Vol.913 (1), p.48 [Peer Reviewed Journal]

2021. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing May 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abf24c

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16
Central X-Ray Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole
Central X-Ray Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole
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Central X-Ray Point Sources Found to Be Abundant in Low-mass, Late-type Galaxies Predicted to Contain an Intermediate-mass Black Hole

The Astrophysical journal, 2021-12, Vol.923 (2), p.246 [Peer Reviewed Journal]

2021. The Author(s). Published by the American Astronomical Society. ;Copyright IOP Publishing Dec 01, 2021 ;Attribution ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac34f4

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17
Monitoring supergiant fast X-ray transients with Swift: results from the first year
Monitoring supergiant fast X-ray transients with Swift: results from the first year
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Monitoring supergiant fast X-ray transients with Swift: results from the first year

Monthly notices of the Royal Astronomical Society, 2009-11, Vol.399 (4), p.2021-2032 [Peer Reviewed Journal]

2009 The Authors. Journal compilation © 2009 RAS 2009 ;2009 The Authors. Journal compilation © 2009 RAS ;2009 INIST-CNRS ;Journal compilation © 2009 RAS ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1111/j.1365-2966.2009.15356.x ;CODEN: MNRAA4

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18
A Comprehensive X-Ray Report on AT2019wey
A Comprehensive X-Ray Report on AT2019wey
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A Comprehensive X-Ray Report on AT2019wey

The Astrophysical journal, 2021-10, Vol.920 (2), p.121 [Peer Reviewed Journal]

2021. The American Astronomical Society. All rights reserved. ;Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;Copyright IOP Publishing Oct 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac15f8

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19
Evidence for Precession due to Supercritical Accretion in Ultraluminous X-Ray Sources
Evidence for Precession due to Supercritical Accretion in Ultraluminous X-Ray Sources
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Evidence for Precession due to Supercritical Accretion in Ultraluminous X-Ray Sources

The Astrophysical journal, 2018-02, Vol.853 (2), p.115 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Feb 01, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aaa45c

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20
Supernova Archaeology with X-Ray Binary Winds: The Case of GRO J1655−40
Supernova Archaeology with X-Ray Binary Winds: The Case of GRO J1655−40
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Supernova Archaeology with X-Ray Binary Winds: The Case of GRO J1655−40

The Astrophysical journal, 2024-05, Vol.966 (2), p.211 [Peer Reviewed Journal]

2024. The Author(s). Published by the American Astronomical Society. This work is published under http://creativecommons.org/licenses/by/4.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ad3803

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