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1
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM
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Large Magellanic Cloud Cepheid Standards Provide a 1% Foundation for the Determination of the Hubble Constant and Stronger Evidence for Physics beyond ΛCDM

The Astrophysical journal, 2019-05, Vol.876 (1), p.85 [Peer Reviewed Journal]

2019. The American Astronomical Society. ;Copyright IOP Publishing May 01, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab1422

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2
KLLR: A Scale-dependent, Multivariate Model Class for Regression Analysis
KLLR: A Scale-dependent, Multivariate Model Class for Regression Analysis
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KLLR: A Scale-dependent, Multivariate Model Class for Regression Analysis

The Astrophysical journal, 2022-06, Vol.931 (2), p.166 [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/ac6ac7

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3
Metallicities of Classical Cepheids in the Inner Galactic Disk
Metallicities of Classical Cepheids in the Inner Galactic Disk
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Metallicities of Classical Cepheids in the Inner Galactic Disk

The Astrophysical journal, 2023-09, Vol.954 (2), p.198 [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/aced93

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4
Binary Interaction Dominates Mass Ejection in Classical Novae
Binary Interaction Dominates Mass Ejection in Classical Novae
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Binary Interaction Dominates Mass Ejection in Classical Novae

The Astrophysical journal, 2022-10, Vol.938 (1), p.31 [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/ac9136

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5
The Gaia-ASAS-SN Classical Cepheid Sample. I. Sample Selection
The Gaia-ASAS-SN Classical Cepheid Sample. I. Sample Selection
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The Gaia-ASAS-SN Classical Cepheid Sample. I. Sample Selection

The Astrophysical journal, 2021-06, Vol.914 (2), p.127 [Peer Reviewed Journal]

2021 The Author(s). Published by The American Astronomical Society. ;Copyright IOP Publishing Jun 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/abf940

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6
A Probabilistic Approach to Fitting Period-luminosity Relations and Validating Gaia Parallaxes
A Probabilistic Approach to Fitting Period-luminosity Relations and Validating Gaia Parallaxes
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A Probabilistic Approach to Fitting Period-luminosity Relations and Validating Gaia Parallaxes

The Astrophysical journal, 2017-04, Vol.838 (2), p.107 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Apr 01, 2017 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aa643b

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7
A Sub-2% Distance to M31 from Photometrically Homogeneous Near-infrared Cepheid Period–Luminosity Relations Measured with the Hubble Space Telescope
A Sub-2% Distance to M31 from Photometrically Homogeneous Near-infrared Cepheid Period–Luminosity Relations Measured with the Hubble Space Telescope
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A Sub-2% Distance to M31 from Photometrically Homogeneous Near-infrared Cepheid Period–Luminosity Relations Measured with the Hubble Space Telescope

The Astrophysical journal, 2021-10, Vol.920 (2), p.84 [Peer Reviewed Journal]

2021. The Author(s). Published by the American Astronomical Society. ;Copyright IOP Publishing Oct 01, 2021 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ac1597

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8
A Long-period Pre-ELM System Discovered from the LAMOST Medium-resolution Survey
A Long-period Pre-ELM System Discovered from the LAMOST Medium-resolution Survey
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A Long-period Pre-ELM System Discovered from the LAMOST Medium-resolution Survey

The Astrophysical journal, 2022-07, Vol.933 (2), p.193 [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/ac75b6

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9
A Surprising Periodicity Detected during a Super-outburst of V844 Herculis by TESS
A Surprising Periodicity Detected during a Super-outburst of V844 Herculis by TESS
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A Surprising Periodicity Detected during a Super-outburst of V844 Herculis by TESS

The Astrophysical journal, 2023-10, Vol.955 (2), p.150 [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/acf21b

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10
Swift J0503.7−2819: a Short-period Asynchronous Polar or Stream-fed Intermediate Polar
Swift J0503.7−2819: a Short-period Asynchronous Polar or Stream-fed Intermediate Polar
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Swift J0503.7−2819: a Short-period Asynchronous Polar or Stream-fed Intermediate Polar

The Astrophysical journal, 2022-08, Vol.934 (2), p.123 [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/ac7d50

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11
Absolute Calibration of Cepheid Period–Luminosity Relations in NGC 4258
Absolute Calibration of Cepheid Period–Luminosity Relations in NGC 4258
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Absolute Calibration of Cepheid Period–Luminosity Relations in NGC 4258

The Astrophysical journal, 2022-11, Vol.940 (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/ac51db

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12
Gravity Modes on Rapidly Rotating Accreting White Dwarfs and Their Variation after Dwarf Novae
Gravity Modes on Rapidly Rotating Accreting White Dwarfs and Their Variation after Dwarf Novae
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Gravity Modes on Rapidly Rotating Accreting White Dwarfs and Their Variation after Dwarf Novae

The Astrophysical journal, 2023-07, Vol.951 (2), p.122 [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/acd1df

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13
Orbital Period Variations in HT Cas: Evidence for Additional Angular Momentum Loss and a High-eccentricity Giant Planet
Orbital Period Variations in HT Cas: Evidence for Additional Angular Momentum Loss and a High-eccentricity Giant Planet
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Orbital Period Variations in HT Cas: Evidence for Additional Angular Momentum Loss and a High-eccentricity Giant Planet

The Astrophysical journal, 2023-08, Vol.953 (1), p.63 [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/acdd6e

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14
Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant
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Milky Way Cepheid Standards for Measuring Cosmic Distances and Application to Gaia DR2: Implications for the Hubble Constant

The Astrophysical journal, 2018-07, Vol.861 (2), p.126 [Peer Reviewed Journal]

2018. The American Astronomical Society. ;Copyright IOP Publishing Jul 10, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aac82e

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15
SRGeJ045359.9+622444: A 55 Minute Period Eclipsing AM Canum Venaticorum Star Discovered from a Joint SRG/eROSITA + ZTF Search
SRGeJ045359.9+622444: A 55 Minute Period Eclipsing AM Canum Venaticorum Star Discovered from a Joint SRG/eROSITA + ZTF Search
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SRGeJ045359.9+622444: A 55 Minute Period Eclipsing AM Canum Venaticorum Star Discovered from a Joint SRG/eROSITA + ZTF Search

The Astrophysical journal, 2023-09, Vol.954 (1), p.63 [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/ace698

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16
Calibrating the Cepheid Period–Wesenheit Relation in the Gaia Bands Using Galactic Open-cluster Cepheids
Calibrating the Cepheid Period–Wesenheit Relation in the Gaia Bands Using Galactic Open-cluster Cepheids
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Calibrating the Cepheid Period–Wesenheit Relation in the Gaia Bands Using Galactic Open-cluster Cepheids

The Astrophysical journal, 2022-10, Vol.938 (1), p.33 [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/ac9051

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17
The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period-Luminosity Relations
The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period-Luminosity Relations
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The Near-infrared Optimal Distances Method Applied to Galactic Classical Cepheids Tightly Constrains Mid-infrared Period-Luminosity Relations

The Astrophysical journal, 2018-01, Vol.852 (2), p.78 [Peer Reviewed Journal]

2018. The American Astronomical Society. ;Copyright IOP Publishing Jan 10, 2018 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/aa9d99

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18
Discovery of Two Polars from a Crossmatch of ZTF and the SRG/eFEDS X-Ray Catalog
Discovery of Two Polars from a Crossmatch of ZTF and the SRG/eFEDS X-Ray Catalog
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Discovery of Two Polars from a Crossmatch of ZTF and the SRG/eFEDS X-Ray Catalog

The Astrophysical journal, 2023-03, Vol.945 (2), p.141 [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/acbb6f

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19
White Dwarf Photospheric Abundances in Cataclysmic Variables—II. White Dwarfs with and without a Mask
White Dwarf Photospheric Abundances in Cataclysmic Variables—II. White Dwarfs with and without a Mask
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White Dwarf Photospheric Abundances in Cataclysmic Variables—II. White Dwarfs with and without a Mask

The Astrophysical journal, 2022-03, Vol.928 (1), p.26 [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/ac524e

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20
Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope Photometry
Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope Photometry
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Cluster Cepheids with High Precision Gaia Parallaxes, Low Zero-point Uncertainties, and Hubble Space Telescope Photometry

The Astrophysical journal, 2022-10, Vol.938 (1), p.36 [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/ac8f24

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