D-Index & Metrics Best Publications
Physics
Netherlands
2023

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 116 Citations 42,252 311 World Ranking 621 National Ranking 8

Research.com Recognitions

Awards & Achievements

2023 - Research.com Physics in Netherlands Leader Award

2022 - Research.com Physics in Netherlands Leader Award

Overview

What is he best known for?

The fields of study he is best known for:

  • Galaxy
  • Astronomy
  • Astrophysics

His scientific interests lie mostly in Astrophysics, Galaxy, Redshift, Astronomy and Luminosity. Astrophysics is a component of his Hubble Ultra-Deep Field, Star formation, Stellar mass, Galaxy formation and evolution and Galaxy cluster studies. His research investigates the connection with Galaxy and areas like Photometry which intersect with concerns in Astrometry and Point source.

His study in Redshift is interdisciplinary in nature, drawing from both Cosmology and Halo. His Luminosity research integrates issues from Extinction, James Webb Space Telescope, Universe and Halo mass function. In his study, Cosmic time is strongly linked to Lyman-break galaxy, which falls under the umbrella field of Luminosity function.

His most cited work include:

  • UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields (924 citations)
  • UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields (924 citations)
  • Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse* ** (747 citations)

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

Rychard Bouwens mostly deals with Astrophysics, Galaxy, Redshift, Astronomy and Star formation. His Astrophysics and Hubble Ultra-Deep Field, Galaxy formation and evolution, Galaxy cluster, Reionization and Stellar population investigations all form part of his Astrophysics research activities. His Hubble Ultra-Deep Field research includes themes of Wide Field Camera 3 and Surface brightness.

His studies link Stars with Galaxy. The Redshift study combines topics in areas such as Equivalent width, Emission spectrum, Photometry and Universe. His studies deal with areas such as Accretion, Extinction, Metallicity and COSMIC cancer database as well as Star formation.

He most often published in these fields:

  • Astrophysics (113.82%)
  • Galaxy (104.82%)
  • Redshift (72.59%)

What were the highlights of his more recent work (between 2016-2021)?

  • Astrophysics (113.82%)
  • Galaxy (104.82%)
  • Redshift (72.59%)

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

Rychard Bouwens mainly focuses on Astrophysics, Galaxy, Redshift, Star formation and Astronomy. The study of Astrophysics is intertwined with the study of Emission spectrum in a number of ways. His Galaxy research is multidisciplinary, incorporating perspectives in Stars and Universe.

His Redshift research is multidisciplinary, incorporating elements of Magnitude, COSMIC cancer database, Galaxy cluster and Mass ratio. Rychard Bouwens interconnects Milky Way and Infrared excess in the investigation of issues within Star formation. His Luminosity study integrates concerns from other disciplines, such as Line and Halo.

Between 2016 and 2021, his most popular works were:

  • Lyα and C iii] emission in z = 7–9 Galaxies: accelerated reionization around luminous star-forming systems? (224 citations)
  • The MUSE Hubble Ultra Deep Field Survey. I. Survey description, data reduction, and source detection (207 citations)
  • The z~6 Luminosity Function Fainter than -15 mag from the Hubble Frontier Fields: The Impact of Magnification Uncertainties (160 citations)

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

  • Galaxy
  • Astronomy
  • Astrophysics

His primary areas of study are Astrophysics, Galaxy, Redshift, Hubble Ultra-Deep Field and Astronomy. The study incorporates disciplines such as Gravitation and Emission spectrum in addition to Astrophysics. His research in Reionization, Luminosity, Luminosity function, Galaxy formation and evolution and Stellar population are components of Galaxy.

His study explores the link between Luminosity and topics such as Universe that cross with problems in Star cluster and Globular cluster. His Redshift study incorporates themes from Star formation, Stellar mass, Galaxy cluster and Continuum. While the research belongs to areas of Hubble Ultra-Deep Field, he spends his time largely on the problem of Multi Unit Spectroscopic Explorer, intersecting his research to questions surrounding Spectroscopy.

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

Cluster Lensing And Supernova survey with Hubble (CLASH): An Overview

Marc Postman;Dan Coe;Narciso Benitez;Larry Bradley.
arXiv: Cosmology and Nongalactic Astrophysics (2011)

1175 Citations

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)

1147 Citations

UV Luminosity Functions at z~4, 5, and 6 from the Hubble Ultra Deep Field and Other Deep Hubble Space Telescope ACS Fields: Evolution and Star Formation History*

Rychard J Bouwens;Garth D Illingworth;Marijn Franx;Holland Ford.
The Astrophysical Journal (2007)

1046 Citations

UV Luminosity Functions at z~4, 5, and 6 from the HUDF and other Deep HST ACS Fields: Evolution and Star Formation History

Rychard J. Bouwens;Garth D. Illingworth;Marijn Franx;Holland Ford.
arXiv: Astrophysics (2007)

1018 Citations

UV Luminosity Functions from 132 z~7 and z~8 Lyman-Break Galaxies in the ultra-deep HUDF09 and wide-area ERS WFC3/IR Observations

R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbe.
arXiv: Cosmology and Nongalactic Astrophysics (2010)

989 Citations

Confirmation of the Remarkable Compactness of Massive Quiescent Galaxies at z ~ 2.3: Early-Type Galaxies Did not Form in a Simple Monolithic Collapse* **

Pieter G. van Dokkum;Marijn Franx;Mariska Kriek;Bradford Holden.
The Astrophysical Journal (2008)

846 Citations

Ultraviolet Luminosity Functions from 132 z ~ 7 and z ~ 8 Lyman-break Galaxies in the Ultra-deep HUDF09 and Wide-area Early Release Science WFC3/IR Observations

R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbé.
The Astrophysical Journal (2011)

691 Citations

Discovery of z~8 Galaxies in the HUDF from ultra-deep WFC3/IR Observations

R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Stiavelli.
arXiv: Cosmology and Nongalactic Astrophysics (2009)

593 Citations

Galaxies in the Hubble Ultra Deep Field. I. Detection, Multiband Photometry, Photometric Redshifts, and Morphology

Dan Coe;Dan Coe;Narciso Benítez;Narciso Benítez;Sebastián F. Sánchez;Myungkook Jee.
The Astronomical Journal (2006)

544 Citations

UV Continuum Slope and Dust Obscuration from z ~ 6 to z ~ 2: The Star Formation Rate Density at High Redshift

R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;M. Franx;R.-R. Chary.
The Astrophysical Journal (2009)

532 Citations

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