2023 - Research.com Physics in Denmark Leader Award
2022 - Research.com Physics in Denmark Leader Award
Gabriel B. Brammer mainly focuses on Astrophysics, Galaxy, Redshift, Astronomy and Stellar mass. Galaxy formation and evolution, Photometry, Number density, Red shift and Active galactic nucleus are the subjects of his Astrophysics studies. In his work, Photometric redshift is strongly intertwined with Stars, which is a subfield of Galaxy.
His studies in Redshift integrate themes in fields like Spectral line, Emission spectrum and Spectral density. His study looks at the relationship between Stellar mass and fields such as Luminosity, as well as how they intersect with chemical problems. His Star formation research is multidisciplinary, incorporating elements of Balmer series, Luminosity function, Disc galaxy, Sersic profile and Low Mass.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Astronomy and Star formation. Astrophysics is a component of his Stellar mass, Galaxy formation and evolution, Stellar population, Luminous infrared galaxy and Metallicity studies. His Stellar mass research is multidisciplinary, relying on both Spectral energy distribution, Luminosity, Effective radius, Universe and Velocity dispersion.
Telescope is closely connected to Photometry in his research, which is encompassed under the umbrella topic of Galaxy. As a part of the same scientific family, Gabriel B. Brammer mostly works in the field of Redshift, focusing on Galaxy cluster and, on occasion, Supernova. The concepts of his Star formation study are interwoven with issues in Milky Way, Balmer series, Luminosity function and Disc galaxy.
His primary scientific interests are in Galaxy, Astrophysics, Redshift, Star formation and Stellar mass. His Galaxy study introduces a deeper knowledge of Astronomy. In the subject of general Astronomy, his work in Spitzer Space Telescope, Infrared and Telescope is often linked to Field, thereby combining diverse domains of study.
His studies examine the connections between Redshift and genetics, as well as such issues in Spectral line, with regards to Active galactic nucleus. His study focuses on the intersection of Star formation and fields such as Sigma with connections in the field of Stellar rotation. His Stellar mass research integrates issues from Number density, Halo, Galaxy formation and evolution, Dark matter and Black hole.
Astrophysics, Galaxy, Redshift, Star formation and Stellar mass are his primary areas of study. His work in Astrophysics is not limited to one particular discipline; it also encompasses Astronomy. His research integrates issues of Stars, Photometry, Supernova and Star in his study of Redshift.
The various areas that he examines in his Photometry study include Wide Field Camera 3, Universe, Black hole and Advanced Camera for Surveys. In his study, Galaxy rotation curve, Scalar field dark matter, Hot dark matter and Dark matter halo is inextricably linked to Dark matter, which falls within the broad field of Galaxy formation and evolution. His work deals with themes such as Active galactic nucleus and Emission spectrum, which intersect with Metallicity.
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.
EAZY: A Fast, Public Photometric Redshift Code
Gabriel B. Brammer;Pieter G. van Dokkum;Paolo Coppi.
The Astrophysical Journal (2008)
3D-HST+CANDELS: THE EVOLUTION OF THE GALAXY SIZE–MASS DISTRIBUTION SINCE z = 3
A. van der Wel;M. Franx;P.G. van Dokkum;R.E. Skelton.
The Astrophysical Journal (2014)
The Star Formation Mass Sequence Out to z = 2.5
Katherine E. Whitaker;Pieter G. van Dokkum;Gabriel Brammer;Marijn Franx.
The Astrophysical Journal (2012)
THE EVOLUTION OF THE STELLAR MASS FUNCTIONS OF STAR-FORMING AND QUIESCENT GALAXIES TO z = 4 FROM THE COSMOS/UltraVISTA SURVEY*
Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx.
The Astrophysical Journal (2013)
The Growth of Massive Galaxies Since z = 2
Pieter G. van Dokkum;Pieter G. van Dokkum;Katherine E. Whitaker;Katherine E. Whitaker;Gabriel Brammer;Gabriel Brammer;Marijn Franx.
The Astrophysical Journal (2010)
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)
The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies
Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. van Dokkum;Rosalind E. Skelton.
arXiv: Astrophysics of Galaxies (2015)
CONSTRAINING THE LOW-MASS SLOPE OF THE STAR FORMATION SEQUENCE AT 0.5 < z < 2.5
Katherine E. Whitaker;Marijn Franx;Joel Leja;Pieter G. van Dokkum.
The Astrophysical Journal (2014)
3D-HST: a wide-field grism spectroscopic survey with the Hubble Space Telescope
Gabriel B. Brammer;Pieter G. Van Dokkum;Marijn Franx;Mattia Fumagalli.
Astrophysical Journal Supplement Series (2012)
A PUBLIC K-s-SELECTED CATALOG IN THE COSMOS/ULTRAVISTA FIELD: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR POPULATION PARAMETERS
Adam Muzzin;Danilo Marchesini;Mauro Stefanon;Marijn Franx.
Astrophysical Journal Supplement Series (2013)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
Yale University
Tufts University
University of California, Berkeley
Leiden University
Leiden University
Swinburne University of Technology
The Open University
University of California, Los Angeles
Leiden University
University of Bath
The Ohio State University
University of California, Los Angeles
University of Washington
International Monetary Fund
Siksha O Anusandhan University
Graz University of Technology
Grenoble Alpes University
Institute for Infocomm Research
University of California, Davis
University of Burgundy
Washington State University
Atmospheric and Environmental Research
Helmholtz Centre for Environmental Research
University of Bordeaux
City University of New York
University of Massachusetts Boston