2023 - Research.com Physics in Netherlands Leader Award
2022 - Research.com Physics in Netherlands Leader Award
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.
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.
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.
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.
Cluster Lensing And Supernova survey with Hubble (CLASH): An Overview
Marc Postman;Dan Coe;Narciso Benitez;Larry Bradley.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
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)
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)
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)
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)
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)
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)
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)
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)
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)
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