D-Index & Metrics Best Publications

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 D-index 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. Citations Publications World Ranking National Ranking
Physics D-index 93 Citations 30,484 552 World Ranking 1448 National Ranking 773

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Astrophysics
  • Planet

His primary areas of investigation include Astrophysics, Astronomy, Planet, Exoplanet and Planetary system. Gregory W. Henry combines subjects such as Spectral line and Radius with his study of Astrophysics. His Astronomy and Observatory, Transit, Light curve, Photometry and Stellar rotation investigations all form part of his Astronomy research activities.

Gregory W. Henry has included themes like Photosphere and Radial velocity in his Planet study. His work focuses on many connections between Exoplanet and other disciplines, such as Atmosphere, that overlap with his field of interest in Solar System and Gas giant. His research in Planetary system intersects with topics in Orbit, Orbital period, Main sequence and Eclipse.

His most cited work include:

  • A Transiting "51 Peg-like" Planet. (768 citations)
  • No planet for HD 166435 (735 citations)
  • No planet for HD 166435 (722 citations)

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

Gregory W. Henry focuses on Astrophysics, Astronomy, Planet, Stars and Radial velocity. His study in Photometry, Light curve, Orbital period, Starspot and Variable star falls under the purview of Astrophysics. His research brings together the fields of Transit and Planet.

His Stars study incorporates themes from Brightness, Rotation and Spectrograph. His Radial velocity research includes elements of Orbital elements, Super-Earth, Minimum mass and Orbital eccentricity. His work carried out in the field of Exoplanet brings together such families of science as Spectral line, Metallicity and Radius.

He most often published in these fields:

  • Astrophysics (79.83%)
  • Astronomy (59.08%)
  • Planet (36.46%)

What were the highlights of his more recent work (between 2017-2021)?

  • Astrophysics (79.83%)
  • Planet (36.46%)
  • Exoplanet (24.78%)

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

Astrophysics, Planet, Exoplanet, Hot Jupiter and Radial velocity are his primary areas of study. The various areas that Gregory W. Henry examines in his Astrophysics study include Spectral line, Atmosphere and Transit. His research integrates issues of Amplitude, Stellar rotation, Solar System and Orbital period in his study of Planet.

Exoplanet is a subfield of Astronomy that Gregory W. Henry studies. His Radial velocity research is multidisciplinary, relying on both Planetary system, Super-Earth and Noise. His Stars research integrates issues from Light curve, Observatory and Spectrograph.

Between 2017 and 2021, his most popular works were:

  • Helium in the eroding atmosphere of an exoplanet (174 citations)
  • Global Climate and Atmospheric Composition of the Ultra-Hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations (134 citations)
  • Global Climate and Atmospheric Composition of the Ultra-hot Jupiter WASP-103b from HST and Spitzer Phase Curve Observations (131 citations)

In his most recent research, the most cited papers focused on:

  • Astronomy
  • Astrophysics
  • Planet

His primary areas of study are Astrophysics, Planet, Hot Jupiter, Exoplanet and Atmosphere. His biological study spans a wide range of topics, including Brightness and Exosphere. His Planet research includes themes of Stars, Photometry, Radial velocity and Transit.

The study incorporates disciplines such as Spectral line, Light curve and Infrared in addition to Hot Jupiter. His research on Exoplanet concerns the broader Astronomy. His study in the field of Planetary system and Eridanus is also linked to topics like European research, Transit time and Atmospheric model.

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

A Transiting "51 Peg-like" Planet.

Gregory W. Henry;Geoffrey W. Marcy;R. Paul Butler;Steven S. Vogt.
The Astrophysical Journal (2000)

1293 Citations

No planet for HD 166435

D. Queloz;G. W. Henry;J. P. Sivan;S. L. Baliunas.
arXiv: Astrophysics (2001)

1208 Citations

No planet for HD 166435

D. Queloz;G. W. Henry;J. P. Sivan;S. L. Baliunas;S. L. Baliunas.
Astronomy and Astrophysics (2001)

940 Citations

A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion

David K. Sing;Jonathan J. Fortney;Nikolay Nikolov;Hannah R. Wakeford.
Nature (2016)

810 Citations

THE STELLAR ACTIVITY-ROTATION RELATIONSHIP AND THE EVOLUTION OF STELLAR DYNAMOS

Nicholas J. Wright;Jeremy J. Drake;Eric E. Mamajek;Gregory W. Henry.
The Astrophysical Journal (2011)

634 Citations

A ~7.5 M⊕ Planet Orbiting the Nearby Star, GJ 876*

Eugenio J. Rivera;Eugenio J. Rivera;Eugenio J. Rivera;Jack J. Lissauer;R. Paul Butler;Geoffrey W. Marcy.
The Astrophysical Journal (2005)

606 Citations

A Neptune-Mass Planet Orbiting the Nearby M Dwarf GJ 436

R. Paul Butler;Steven S. Vogt;Geoffrey W. Marcy;Debra A. Fischer;Debra A. Fischer.
The Astrophysical Journal (2004)

595 Citations

A ~ 7.5 Earth-Mass Planet Orbiting the Nearby Star, GJ 876

E. J. Rivera;J. J. Lissauer;R. P. Butler;G. W. Marcy.
arXiv: Astrophysics (2005)

593 Citations

Hubble Space Telescope Transmission Spectroscopy of the Exoplanet HD 189733b: High-altitude atmospheric haze in the optical and near-UV with STIS

D. K. Sing;F. Pont;S. Aigrain;D. Charbonneau.
arXiv: Earth and Planetary Astrophysics (2011)

544 Citations

The N2K Consortium. II. A Transiting Hot Saturn Around HD 149026 With a Large Dense Core

B. Sato;D. A. Fischer;G. W. Henry;G. Laughlin.
arXiv: Astrophysics (2005)

513 Citations

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