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WIYN Open Cluster Study. LXXV. Testing the Metallicity Dependence of Stellar Lithium Depletion Using Hyades-aged Clusters. I. Hyades and Praesepe

The Astronomical journal, 2017-03, Vol.153 (3), p.128-128

2017

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A Cooling Anomaly of High-mass White Dwarfs

The Astrophysical journal, 2019-12, Vol.886 (2), p.100

2019

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The White Dwarf Initial–Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M

The Astrophysical journal, 2018-10, Vol.866 (1), p.21

2018

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Double White Dwarf Merger Products among High-mass White Dwarfs

The Astrophysical journal, 2020-03, Vol.891 (2), p.160

2020

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LITHIUM ABUNDANCES OF THE SUPER-METAL-RICH OPEN CLUSTER NGC 6253

The Astronomical journal, 2012-11, Vol.144 (5), p.1-15

2012

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A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS

Monthly notices of the Royal Astronomical Society, 2019-02, Vol.482 (4), p.4570-4591

2019

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Improved Main-sequence Turnoff Ages of Young Open Clusters: Multicolor UBV Techniques and the Challenges of Rotation

The Astronomical journal, 2018-10, Vol.156 (4), p.165

2018

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TESS Reveals that the Nearby Pisces-Eridanus Stellar Stream is only 120 Myr Old

The Astronomical journal, 2019-08, Vol.158 (2), p.77

2019

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A Fresh Look at AGB Stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial–Final Mass Relation

The Astrophysical journal. Supplement series, 2022-02, Vol.258 (2), p.43

2022

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WIYN open cluster study: The old open cluster, NGC 188, and a re-evaluation of Lithium-richness among red giants

Monthly notices of the Royal Astronomical Society, 2022-07, Vol.513 (4), p.5387-5406

2022

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Multiple Populations in NGC 1851: Abundance Variations and UV Photometric Synthesis in the Washington and HST/WFC3 Systems

The Astronomical journal, 2017-04, Vol.153 (4), p.192-192

2017

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A Novel Approach to Constrain Rotational Mixing and Convective-core Overshoot in Stars Using the Initial-Final Mass Relation

Astrophysical journal. Letters, 2019-01, Vol.871 (1), p.L18

2019

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UNCOVERING MULTIPLE POPULATIONS WITH WASHINGTON PHOTOMETRY. I. THE GLOBULAR CLUSTER NGC 1851

The Astronomical journal, 2014-08, Vol.148 (2), p.1-18

2014

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Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – IV. Evidence for multiple populations in Hodge 11 and NGC 2210

Monthly notices of the Royal Astronomical Society, 2019-07, Vol.486 (4), p.5581-5599

2019

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Carbon star formation as seen through the non-monotonic initial–final mass relation

Nature astronomy, 2020-11, Vol.4 (11), p.1102-1110

2020

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Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – V. Multiple populations in ancient globular clusters

Monthly notices of the Royal Astronomical Society, 2020-05, Vol.494 (2), p.1946-1955

2020

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Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – III. Horizontal branch morphology

Monthly notices of the Royal Astronomical Society, 2018-03, Vol.474 (4), p.4358-4365

2018

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Progress and Application of The Initial-Final Mass Relation

Proceedings of the International Astronomical Union, 2016-10, Vol.12 (S323), p.157-164

Cummings, Jeffrey D.

2016

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Lithium in the Intermediate-Age Open Cluster, NGC 3680

The Astronomical journal, 2009-10, Vol.138 (4), p.1171-1191

2009

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Wiyn Open Cluster Study. XXXIX. Abundances in NGC 6253 from Hydra Spectroscopy of the Li 6708 Å Region

The Astronomical journal, 2010-05, Vol.139 (5), p.2034-jQuery1323899675380='48'

2010

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TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL–FINAL MASS RELATION FOR PROGENITORS OF 4–6.5 M

The Astrophysical journal, 2016-02, Vol.818 (1), p.84

2016

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Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – II. Relative ages and distances for six ancient globular clusters

Monthly notices of the Royal Astronomical Society, 2017-11, Vol.471 (3), p.3347-3358

2017

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INITIAL–FINAL MASS RELATION FOR 3 TO 4 M ⊙ PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099

The Astrophysical journal, 2015-07, Vol.807 (1), p.90

2015

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The White Dwarf Initial-Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M Based on observations with the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and NASA, was made possible by the generous financial support of the W.M. Keck Foundation

The Astrophysical journal, 2018-10, Vol.866 (1)

2018

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TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL-FINAL MASS RELATION FOR PROGENITORS OF 4-6.5 M sub([middot in circle])

The Astrophysical journal, 2016-02, Vol.818 (1)

2016

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WIYN Open Cluster Study. LXXV. Testing the Metallicity Dependence of Stellar Lithium Depletion Using Hyades-aged Clusters. I. Hyades and Praesepe

A Cooling Anomaly of High-mass White Dwarfs

The White Dwarf Initial–Final Mass Relation for Progenitor Stars from 0.85 to 7.5 M

Double White Dwarf Merger Products among High-mass White Dwarfs

LITHIUM ABUNDANCES OF THE SUPER-METAL-RICH OPEN CLUSTER NGC 6253

A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS

Improved Main-sequence Turnoff Ages of Young Open Clusters: Multicolor UBV Techniques and the Challenges of Rotation

TESS Reveals that the Nearby Pisces-Eridanus Stellar Stream is only 120 Myr Old

A Fresh Look at AGB Stars in Galactic Open Clusters with Gaia: Impact on Stellar Models and the Initial–Final Mass Relation

WIYN open cluster study: The old open cluster, NGC 188, and a re-evaluation of Lithium-richness among red giants

Multiple Populations in NGC 1851: Abundance Variations and UV Photometric Synthesis in the Washington and HST/WFC3 Systems

A Novel Approach to Constrain Rotational Mixing and Convective-core Overshoot in Stars Using the Initial-Final Mass Relation

UNCOVERING MULTIPLE POPULATIONS WITH WASHINGTON PHOTOMETRY. I. THE GLOBULAR CLUSTER NGC 1851

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – IV. Evidence for multiple populations in Hodge 11 and NGC 2210

Carbon star formation as seen through the non-monotonic initial–final mass relation

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – V. Multiple populations in ancient globular clusters

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – III. Horizontal branch morphology

Progress and Application of The Initial-Final Mass Relation

Lithium in the Intermediate-Age Open Cluster, NGC 3680

Wiyn Open Cluster Study. XXXIX. Abundances in NGC 6253 from Hydra Spectroscopy of the Li 6708 Å Region

TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL–FINAL MASS RELATION FOR PROGENITORS OF 4–6.5 M

Exploring the nature and synchronicity of early cluster formation in the Large Magellanic Cloud – II. Relative ages and distances for six ancient globular clusters

INITIAL–FINAL MASS RELATION FOR 3 TO 4 M ⊙ PROGENITORS OF WHITE DWARFS FROM THE SINGLE CLUSTER NGC 2099

TWO MASSIVE WHITE DWARFS FROM NGC 2323 AND THE INITIAL-FINAL MASS RELATION FOR PROGENITORS OF 4-6.5 M sub([middot in circle])

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