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 85 Citations 22,689 203 World Ranking 1875 National Ranking 41

Overview

What is he best known for?

The fields of study he is best known for:

  • Galaxy
  • Astronomy
  • Astrophysics

His main research concerns Astrophysics, Galaxy, Redshift, Astronomy and Stellar mass. His Astrophysics study focuses mostly on Star formation, Reionization, Hubble Ultra-Deep Field, Galaxy formation and evolution and Luminosity. The concepts of his Star formation study are interwoven with issues in Extinction and Surface brightness.

His work on Galaxy deals in particular with Luminosity function, Grism, Quasar, Luminous infrared galaxy and Wide Field Camera 3. His work deals with themes such as Dark matter halo, Doubly ionized oxygen, Emission spectrum, Spectroscopy and Cosmology, which intersect with Redshift. His research integrates issues of Hubble Deep Field and Velocity dispersion in his study of Stellar mass.

His most cited work include:

  • 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses (704 citations)
  • Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers (485 citations)
  • Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers (485 citations)

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

His primary areas of study are Galaxy, Astrophysics, Redshift, Astronomy and Star formation. The various areas that he examines in his Galaxy study include COSMIC cancer database and Photometry. His study connects Infrared and Astrophysics.

His Redshift research is multidisciplinary, incorporating elements of Cosmology, Equivalent width, Universe and Spectral energy distribution. His Star formation research includes elements of Accretion, Metallicity and Photometric redshift. His research investigates the link between Reionization and topics such as Wide Field Camera 3 that cross with problems in Advanced Camera for Surveys.

He most often published in these fields:

  • Galaxy (110.85%)
  • Astrophysics (109.97%)
  • Redshift (78.59%)

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

  • Astrophysics (109.97%)
  • Galaxy (110.85%)
  • Redshift (78.59%)

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

The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Star formation and Stellar mass. His study in Luminosity function, Line, Spectral energy distribution, Photometric redshift and Millimeter are all subfields of Astrophysics. He has included themes like Cosmology and Dark galaxy in his Photometric redshift study.

His studies deal with areas such as COSMIC cancer database, Equivalent width and Continuum as well as Galaxy. He combines subjects such as Luminosity, Universe and Infrared, Infrared excess with his study of Redshift. He has researched Stellar mass in several fields, including Cosmic time, Halo and Baryon.

Between 2019 and 2021, his most popular works were:

  • The ALPINE-ALMA [CII] Survey: Data processing, catalogs, and statistical source properties (46 citations)
  • The ALPINE-ALMA [CII] Survey: Data processing, catalogs, and statistical source properties (46 citations)
  • Rapid Reionization by the Oligarchs: The Case for Massive, UV-Bright, Star-Forming Galaxies with High Escape Fractions (45 citations)

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

  • Galaxy
  • Astronomy
  • Milky Way

Pascal Oesch mostly deals with Astrophysics, Galaxy, Redshift, Star formation and Hubble Ultra-Deep Field. His work in Reionization, Stellar mass, Infrared excess, Universe and Luminosity function are all subfields of Astrophysics research. His research in Luminosity function intersects with topics in Quasar, Bright star and Photon.

His Galaxy research includes themes of COSMIC cancer database, Infrared and Millimeter. His Redshift research is multidisciplinary, incorporating perspectives in Atacama Large Millimeter Array, Spectral energy distribution, Luminosity and Line. The study incorporates disciplines such as Doubly ionized oxygen, Spectral line, Galaxy formation and evolution and Interstellar medium in addition to Star formation.

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

UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields

R.J. Bouwens;R.J. Bouwens;G.D. Illingworth;P.A. Oesch;P.A. Oesch;M. Trenti.
The Astrophysical Journal (2015)

981 Citations

3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses

Rosalind E. Skelton;Katherine E. Whitaker;Ivelina G. Momcheva;Gabriel B. Brammer.
Astrophysical Journal Supplement Series (2014)

704 Citations

Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers

M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti.
Journal of Cosmology and Astroparticle Physics (2012)

507 Citations

UV-continuum Slopes at z ~ 4-7 from the HUDF09+ERS+CANDELS Observations: Discovery of a Well-defined UV Color-Magnitude Relationship for z ≥ 4 Star-forming Galaxies

R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P.A. Oesch;M. Franx.
The Astrophysical Journal (2012)

473 Citations

THE 3D-HST SURVEY: HUBBLE SPACE TELESCOPE WFC3/G141 GRISM SPECTRA, REDSHIFTS, AND EMISSION LINE MEASUREMENTS FOR ∼100,000 GALAXIES

Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. Van Dokkum;Rosalind E. Skelton.
Astrophysical Journal Supplement Series (2016)

443 Citations

The Most Luminous z~9-10 Galaxy Candidates yet Found: The Luminosity Function, Cosmic Star-Formation Rate, and the First Mass Density Estimate at 500 Myr

P. A. Oesch;R. J. Bouwens;G. D. Illingworth;I. Labbe.
arXiv: Cosmology and Nongalactic Astrophysics (2013)

397 Citations

Reionization after Planck: The Derived Growth of the Cosmic Ionizing Emissivity now matches the Growth of the Galaxy UV Luminosity Density

R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;J. Caruana.
The Astrophysical Journal (2015)

357 Citations

UV-CONTINUUM SLOPES OF >4000 z ∼ 4-8 GALAXIES FROM THE HUDF/XDF, HUDF09, ERS, CANDELS-SOUTH, AND CANDELS-NORTH FIELDS

R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbé.
The Astrophysical Journal (2014)

323 Citations

A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

P.A. Oesch;G. Brammer;P.G. van Dokkum;G.D. Illingworth.
The Astrophysical Journal (2016)

314 Citations

z ∼ 7 GALAXIES IN THE HUDF: FIRST EPOCH WFC3/IR RESULTS*

P. A. Oesch;R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;C. M. Carollo.
The Astrophysical Journal (2010)

307 Citations

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Franz E. Bauer

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Michele Trenti

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