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 82 Citations 18,149 237 World Ranking 2109 National Ranking 1085

Overview

What is he best known for?

The fields of study he is best known for:

  • Astronomy
  • Infrared
  • Planet

His scientific interests lie mostly in Exoplanet, Astrophysics, Planet, Astronomy and Hot Jupiter. David K. Sing interconnects Atmosphere, Neptune, Emission spectrum and James Webb Space Telescope in the investigation of issues within Exoplanet. His Astrophysics research is multidisciplinary, incorporating elements of Rayleigh scattering and Radius.

His Planet study combines topics in areas such as Light curve, Solar System, Transit and Exosphere. He combines subjects such as Astrobiology and Radiation pressure with his study of Transit. The various areas that David K. Sing examines in his Hot Jupiter study include Spectral line and Space Telescope Imaging Spectrograph.

His most cited work include:

  • A continuum from clear to cloudy hot-Jupiter exoplanets without primordial water depletion (659 citations)
  • Water vapour in the atmosphere of a transiting extrasolar planet (463 citations)
  • Water vapour in the atmosphere of a transiting extrasolar planet (463 citations)

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

His primary scientific interests are in Astrophysics, Exoplanet, Planet, Hot Jupiter and Astronomy. His research integrates issues of Spectral line, Atmosphere, Wavelength and Rayleigh scattering in his study of Astrophysics. His biological study spans a wide range of topics, including Planetary system, Astrobiology, Absorption and Transit.

His Planet research integrates issues from Metallicity, Solar System, Exosphere and James Webb Space Telescope. Within one scientific family, David K. Sing focuses on topics pertaining to Space Telescope Imaging Spectrograph under Hot Jupiter, and may sometimes address concerns connected to Wide Field Camera 3. His work on Radial velocity, White dwarf and Emission spectrum is typically connected to European research and Transmission as part of general Astronomy study, connecting several disciplines of science.

He most often published in these fields:

  • Astrophysics (72.50%)
  • Exoplanet (66.88%)
  • Planet (48.12%)

What were the highlights of his more recent work (between 2019-2021)?

  • Astrophysics (72.50%)
  • Exoplanet (66.88%)
  • Hot Jupiter (40.00%)

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

His main research concerns Astrophysics, Exoplanet, Hot Jupiter, Atmosphere and Planet. His Astrophysics research includes themes of Spectral line, Wavelength, Opacity and Rayleigh scattering. His Exoplanet research is classified as research in Astronomy.

His Hot Jupiter research incorporates elements of James Webb Space Telescope, Infrared, Gas giant and Computational physics. His Atmosphere research is multidisciplinary, relying on both Radiative transfer, White dwarf, Brown dwarf and Emission spectrum. David K. Sing has researched Planet in several fields, including Metallicity, Orbital period, Photometry and Astrobiology.

Between 2019 and 2021, his most popular works were:

  • Detection of Fe i in the atmosphere of the ultra-hot Jupiter WASP-121b, and a new likelihood-based approach for Doppler-resolved spectroscopy (50 citations)
  • Statistical Characterization of Hot Jupiter Atmospheres using Spitzer's Secondary Eclipses (39 citations)
  • Non-detection of TiO and VO in the atmosphere of WASP-121b using high-resolution spectroscopy (32 citations)

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

  • Astronomy
  • Infrared
  • Astrophysics

David K. Sing focuses on Astrophysics, Hot Jupiter, Exoplanet, Atmosphere and Planet. His Astrophysics research is multidisciplinary, incorporating perspectives in Rayleigh scattering and Wavelength. The study incorporates disciplines such as Chemical physics, Chemical equilibrium, Orbital period, Orbital eccentricity and Emission spectrum in addition to Hot Jupiter.

His Exoplanet study incorporates themes from Spectral line, James Webb Space Telescope, Scattering and Opacity. His studies examine the connections between Atmosphere and genetics, as well as such issues in Spectroscopy, with regards to Analytical chemistry and Jupiter. His studies deal with areas such as Brightness, Circular orbit, Infrared, Spitzer Space Telescope and Atmospheric temperature as well as Planet.

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 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

Water vapour in the atmosphere of a transiting extrasolar planet

Giovanna Tinetti;Giovanna Tinetti;Giovanna Tinetti;Alfred Vidal-Madjar;Mao-Chang Liang;Jean-Philippe Beaulieu.
Nature (2007)

613 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

Evaporation of the planet HD189733b observed in HI Lyman-alpha

A. Lecavelier des Etangs;D. Ehrenreich;A. Vidal-Madjar;G. E. Ballester.
arXiv: Earth and Planetary Astrophysics (2010)

487 Citations

Hubble Space Telescope transmission spectroscopy of the exoplanet HD 189733b: high‐altitude atmospheric haze in the optical and near‐ultraviolet with STIS

David K. Sing;F. Pont;Suzanne Aigrain;D. Charbonneau.
Monthly Notices of the Royal Astronomical Society (2011)

421 Citations

A giant comet-like cloud of hydrogen escaping the warm Neptune-mass exoplanet GJ 436b

David Ehrenreich;Vincent Bourrier;Peter J. Wheatley;Alain Lecavelier des Etangs.
Nature (2015)

412 Citations

Rayleigh scattering in the transit spectrum of HD 189733b

A. Lecavelier des Etangs;F. Pont;A. Vidal-Madjar;David K. Sing.
Astronomy and Astrophysics (2008)

398 Citations

The prevalence of dust on the exoplanet HD 189733b from Hubble and Spitzer observations

F. Pont;D. K. Sing;N. P. Gibson;N. P. Gibson;S. Aigrain.
Monthly Notices of the Royal Astronomical Society (2013)

384 Citations

Evaporation of the planet HD 189733b observed in H I Lyman-α

A. Lecavelier des Etangs;D. Ehrenreich;A. Vidal-Madjar;G. Ballester.
Astronomy and Astrophysics (2010)

344 Citations

Stellar limb-darkening coefficients for CoRot and Kepler

David K. Sing;David K. Sing.
Astronomy and Astrophysics (2010)

331 Citations

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