D-Index & Metrics Best Publications

David L. Lambert

The University of Texas at Austin
United States

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name Citations Publications World Ranking National Ranking

Physics D-index 98 Citations 36,592 597 World Ranking 1183 National Ranking 634

Research.com Recognitions

Awards & Achievements

1987 - Dannie Heineman Prize for Astrophysics, American Astronomical Society

1980 - Fellow of John Simon Guggenheim Memorial Foundation

Overview

What is he best known for?

The fields of study he is best known for:

Astronomy
Quantum mechanics
Astrophysics

David L. Lambert mostly deals with Astrophysics, Stars, Astronomy, Spectral line and Metallicity. David L. Lambert interconnects Abundance and Lithium in the investigation of issues within Astrophysics. His Stars research integrates issues from Disc and Galaxy formation and evolution.

His biological study spans a wide range of topics, including Atmosphere, Line, Spectroscopy, Halo and Ionization. David L. Lambert has included themes like Supernova, Effective temperature and White dwarf in his Metallicity study. David L. Lambert combines subjects such as Abundance of the chemical elements and Luminosity with his study of Stellar evolution.

His most cited work include:

Elemental abundance survey of the Galactic thick disc (748 citations)
Elemental Abundance Survey of The Galactic Thick Disk (735 citations)
The chemical compositions of Galactic disc F and G dwarfs (710 citations)

What are the main themes of his work throughout his whole career to date?

His primary scientific interests are in Astrophysics, Stars, Astronomy, Spectral line and Abundance. Metallicity, Astronomical spectroscopy, Line, Stellar evolution and Supergiant are the primary areas of interest in his Astrophysics study. His studies deal with areas such as Halo and Galaxy as well as Stars.

Much of his study explores Astronomy relationship to Lithium. His Spectral line research is multidisciplinary, relying on both Absorption spectroscopy, Analytical chemistry, Interstellar medium and Atomic physics. The various areas that David L. Lambert examines in his Abundance study include Atmosphere, Nitrogen, Open cluster, Cluster and Carbon.

He most often published in these fields:

Astrophysics (88.48%)
Stars (55.27%)
Astronomy (40.62%)

What were the highlights of his more recent work (between 2009-2021)?

Astrophysics (88.48%)
Stars (55.27%)
Astronomy (40.62%)

In recent papers he was focusing on the following fields of study:

David L. Lambert mainly focuses on Astrophysics, Stars, Astronomy, Spectral line and Abundance. His is doing research in Metallicity, Open cluster, Supergiant, Line and Interstellar medium, both of which are found in Astrophysics. His work carried out in the field of Metallicity brings together such families of science as Main sequence, Dwarf galaxy, Milky Way, Asymptotic giant branch and Disc.

His Stars study combines topics from a wide range of disciplines, such as Luminosity, Galaxy and Lithium. The Spectral line study combines topics in areas such as Halo, Telescope, Infrared and White dwarf. His study in Abundance is interdisciplinary in nature, drawing from both Carbon and Chemical composition.

Between 2009 and 2021, his most popular works were:

OXYGEN ABUNDANCES IN NEARBY FGK STARS AND THE GALACTIC CHEMICAL EVOLUTION OF THE LOCAL DISK AND HALO (246 citations)
THE DISTRIBUTION OF THE ELEMENTS IN THE GALACTIC DISK. III. A RECONSIDERATION OF CEPHEIDS FROM l = 30° TO 250° (181 citations)
The Distribution Of The Elements In The Galactic Disk. III. A Reconsideration Of Cepheids From L=30 Degrees To 250 Degrees (181 citations)

This overview was generated by a machine learning system which analysed the scientist’s body of work. If you have any feedback, you can contact us here.

Best Publications

Elemental Abundance Survey of The Galactic Thick Disk

Bacham E. Reddy;David L. Lambert;Carlos Allende Prieto.
arXiv: Astrophysics (2005)

1222 Citations

The Chemical Compositions of Galactic Disk F and G Dwarfs

Bacham E. Reddy;Jocelyn Tomkin;David L. Lambert;Carlos Allende Prieto.
arXiv: Astrophysics (2002)

1131 Citations

Elemental abundance survey of the Galactic thick disc

Bacham E. Reddy;David L. Lambert;Carlos Allende Prieto.
Monthly Notices of the Royal Astronomical Society (2006)

888 Citations

The chemical compositions of Galactic disc F and G dwarfs

Bacham E. Reddy;Jocelyn Tomkin;David L. Lambert;Carlos Allende Prieto.
Monthly Notices of the Royal Astronomical Society (2003)

827 Citations

Synthesis of the elements in stars: forty years of progress

George Wallerstein;Icko Iben;Peter Parker;Ann Merchant Boesgaard.
Reviews of Modern Physics (1997)

816 Citations

THE HIGH-RESOLUTION CROSS-DISPERSED ECHELLE WHITE PUPIL SPECTROMETER OF THE MCDONALD OBSERVATORY 2.7-M TELESCOPE

Robert G. Tull;Phillip J. Macqueen;Christopher Sneden;David L. Lambert.
Publications of the Astronomical Society of the Pacific (1995)

700 Citations

S4N: A Spectroscopic Survey of Stars in the Solar Neighborhood

Carlos Allende Prieto;Paul S. Barklem;David L. Lambert;Katia Cunha.
arXiv: Astrophysics (2004)

535 Citations

The chemical composition of carbon stars. I. Carbon, nitrogen, and oxygen in 30 cool carbon stars in the Galactic disk

David L. Lambert;Bengt Gustafsson;Kjell Eriksson;Kenneth H. Hinkle.
Astrophysical Journal Supplement Series (1986)

503 Citations

S4N: A spectroscopic survey of stars in the solar neighborhood: The nearest 15 pc

C. Allende Prieto;Paul Barklem;D.L Lambert;K. Cunha.
Astronomy and Astrophysics (2004)

495 Citations

Carbon, Nitrogen, and Oxygen Abundances in Early B-Type Stars

Douglas R. Gies;David L. Lambert.
The Astrophysical Journal (1992)

488 Citations

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Frequent Co-Authors

External Links

Personal Website for David L. Lambert