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1
Constraining the Metallicities, Ages, Star Formation Histories, and Ionizing Continua of Extragalactic Massive Star Populations∗ ∗ Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555
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Constraining the Metallicities, Ages, Star Formation Histories, and Ionizing Continua of Extragalactic Massive Star Populations∗ ∗ Based on observations made with the NASA/ESA Hubble Space Telescope, obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555

The Astrophysical journal, 2019-09, Vol.882 (2) [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab3104

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2
SPECKLE INTERFEROMETRY AT SOAR IN 2015 Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope
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SPECKLE INTERFEROMETRY AT SOAR IN 2015 Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope

The Astronomical journal, 2016-05, Vol.151 (6) [Peer Reviewed Journal]

2016. The American Astronomical Society. All rights reserved. ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.3847/0004-6256/151/6/153

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3
SPECKLE INTERFEROMETRY AT SOAR IN 2014 Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU)
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SPECKLE INTERFEROMETRY AT SOAR IN 2014 Based on observations obtained at the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, e Inovação (MCTI) da República Federativa do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU)

The Astronomical journal, 2015-07, Vol.150 (2) [Peer Reviewed Journal]

2015. The American Astronomical Society. All rights reserved. ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.1088/0004-6256/150/2/50

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4
RADIAL VELOCITIES OF SOUTHERN VISUAL MULTIPLE STARS Based on observations at the LCO 100 inch Du Pont telescope and at the CTIO 1.5 m telescope
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RADIAL VELOCITIES OF SOUTHERN VISUAL MULTIPLE STARS Based on observations at the LCO 100 inch Du Pont telescope and at the CTIO 1.5 m telescope

The Astronomical journal, 2014-12, Vol.149 (1) [Peer Reviewed Journal]

2015. The American Astronomical Society. All rights reserved. ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.1088/0004-6256/149/1/8

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5
A sequence of Type Ib, IIb, II-L, and II-P supernovae from binary-star progenitors with varying initial separations
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A sequence of Type Ib, IIb, II-L, and II-P supernovae from binary-star progenitors with varying initial separations

Astronomy and astrophysics (Berlin), 2024-05, Vol.685 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/202349066

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6
The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars
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The NANOGrav 11-year Data Set: High-precision Timing of 45 Millisecond Pulsars

The Astrophysical journal. Supplement series, 2018-04, Vol.235 (2), p.37 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Apr 2018 ;ISSN: 0067-0049 ;ISSN: 1538-4365 ;EISSN: 1538-4365 ;DOI: 10.3847/1538-4365/aab5b0

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7
Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in bpass
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Understanding the high-mass binary black hole population from stable mass transfer and super-Eddington accretion in bpass

Monthly notices of the Royal Astronomical Society, 2023-02, Vol.520 (4), p.5724-5745 [Peer Reviewed Journal]

2023 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. 2023 ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/stad399

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8
The Updated Multiple Star Catalog
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The Updated Multiple Star Catalog

The Astrophysical journal. Supplement series, 2018-03, Vol.235 (1), p.6 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Mar 2018 ;ISSN: 0067-0049 ;EISSN: 1538-4365 ;DOI: 10.3847/1538-4365/aaa1a5

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9
UNDERSTANDING THE EFFECTS OF STELLAR MULTIPLICITY ON THE DERIVED PLANET RADII FROM TRANSIT SURVEYS: IMPLICATIONS FOR KEPLER, K2, AND TESS
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UNDERSTANDING THE EFFECTS OF STELLAR MULTIPLICITY ON THE DERIVED PLANET RADII FROM TRANSIT SURVEYS: IMPLICATIONS FOR KEPLER, K2, AND TESS

The Astrophysical journal, 2015-05, Vol.805 (1), p.1-9 [Peer Reviewed Journal]

2015. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/805/1/16

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10
Tests of Gravitational Symmetries with Pulsar Binary J1713+0747
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Tests of Gravitational Symmetries with Pulsar Binary J1713+0747

Monthly notices of the Royal Astronomical Society, 2019-01, Vol.482 (3), p.3249-3260 [Peer Reviewed Journal]

Copyright Determination: MAY_INCLUDE_COPYRIGHT_MATERIAL ;Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/sty2905

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11
The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc
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The Solar Neighborhood. XLV. The Stellar Multiplicity Rate of M Dwarfs Within 25 pc

The Astronomical journal, 2019-06, Vol.157 (6), p.216 [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 2019 ;ISSN: 0004-6256 ;EISSN: 1538-3881 ;DOI: 10.3847/1538-3881/ab05dc

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12
Does the Black Hole Merger Rate Evolve with Redshift?
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Does the Black Hole Merger Rate Evolve with Redshift?

Astrophysical journal. Letters, 2018-08, Vol.863 (2), p.L41 [Peer Reviewed Journal]

2018. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Aug 20, 2018 ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8213/aad800

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13
Hydrodynamic Torques in Circumbinary Accretion Disks
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Hydrodynamic Torques in Circumbinary Accretion Disks

The Astrophysical journal, 2019-04, Vol.875 (1), p.66 [Peer Reviewed Journal]

2019. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Apr 10, 2019 ;ISSN: 0004-637X ;EISSN: 1538-4357 ;DOI: 10.3847/1538-4357/ab09ee

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14
Close stellar conjunctions of α Centauri A and B until 2050: An mK = 7.8 star may enter the Einstein ring of α Cen A in 2028
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Close stellar conjunctions of α Centauri A and B until 2050: An mK = 7.8 star may enter the Einstein ring of α Cen A in 2028

Astronomy and astrophysics (Berlin), 2016-10, Vol.594 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201629201

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15
Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars
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Mind Your Ps and Qs: The Interrelation between Period (P) and Mass-ratio (Q) Distributions of Binary Stars

The Astrophysical journal. Supplement series, 2017-06, Vol.230 (2), p.15 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Jun 2017 ;ISSN: 0067-0049 ;EISSN: 1538-4365 ;DOI: 10.3847/1538-4365/aa6fb6

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16
Cannibals in the thick disk: the young α-rich stars as evolved blue stragglers
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Cannibals in the thick disk: the young α-rich stars as evolved blue stragglers

Astronomy and astrophysics (Berlin), 2016-11, Vol.595, p.A60 [Peer Reviewed Journal]

ISSN: 0004-6361 ;EISSN: 1432-0746 ;DOI: 10.1051/0004-6361/201629356

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17
The dependence of theoretical synthetic spectra on α-enhancement in young, binary stellar populations
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The dependence of theoretical synthetic spectra on α-enhancement in young, binary stellar populations

Monthly notices of the Royal Astronomical Society, 2022-04, Vol.512 (4), p.5329-5338 [Peer Reviewed Journal]

The Author(s) 2022. Published by Oxford University Press on behalf of Royal Astronomical Society 2022 ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/stac807

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18
Where Are LIGO's Big Black Holes?
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Where Are LIGO's Big Black Holes?

Astrophysical journal. Letters, 2017-12, Vol.851 (2), p.L25 [Peer Reviewed Journal]

2017. The American Astronomical Society. All rights reserved. ;Copyright IOP Publishing Dec 20, 2017 ;ISSN: 2041-8205 ;EISSN: 2041-8213 ;DOI: 10.3847/2041-8213/aa9bf6

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19
THE KOZAI-LIDOV MECHANISM IN HYDRODYNAMICAL DISKS. II. EFFECTS OF BINARY AND DISK PARAMETERS
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THE KOZAI-LIDOV MECHANISM IN HYDRODYNAMICAL DISKS. II. EFFECTS OF BINARY AND DISK PARAMETERS

The Astrophysical journal, 2015-07, Vol.807 (1), p.1-14 [Peer Reviewed Journal]

2015. The American Astronomical Society. All rights reserved. ;ISSN: 0004-637X ;ISSN: 1538-4357 ;EISSN: 1538-4357 ;DOI: 10.1088/0004-637X/807/1/75

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20
Discovery of an equal-mass `twin' binary population reaching 1000 + au separations
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Discovery of an equal-mass `twin' binary population reaching 1000 + au separations

Monthly notices of the Royal Astronomical Society, 2019-11, Vol.489, p.5822-5857 [Peer Reviewed Journal]

Distributed under a Creative Commons Attribution 4.0 International License ;ISSN: 0035-8711 ;EISSN: 1365-2966 ;DOI: 10.1093/mnras/stz2480

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