Bram Venemans mainly focuses on Astrophysics, Quasar, Galaxy, Redshift and Astronomy. His Astrophysics study combines topics from a wide range of disciplines, such as Spectral line, Equivalent width and Emission spectrum. His Quasar research is multidisciplinary, relying on both Line, Luminosity, Observatory and Telescope.
His work carried out in the field of Galaxy brings together such families of science as Spectroscopy and Dust emission. His Redshift research is multidisciplinary, incorporating perspectives in Supermassive black hole, Black hole and Eddington luminosity. The various areas that he examines in his Radio galaxy study include Star formation, Galaxy cluster, Very Large Telescope and Velocity dispersion.
Bram Venemans spends much of his time researching Astrophysics, Quasar, Redshift, Galaxy and Astronomy. His Astrophysics study frequently draws connections between related disciplines such as Emission spectrum. His Quasar research is multidisciplinary, incorporating elements of Accretion, Spectral line, Reionization and Supermassive black hole, Black hole.
His study looks at the intersection of Redshift and topics like Sky with Infrared and Brown dwarf. His study in the field of Interstellar medium, Active galactic nucleus and Galaxy formation and evolution is also linked to topics like Continuum. The concepts of his Radio galaxy study are interwoven with issues in Spectroscopy, Galaxy cluster, Elliptical galaxy and Velocity dispersion.
His primary areas of study are Quasar, Astrophysics, Galaxy, Redshift and Supermassive black hole. He combines subjects such as Sky, Ionization, Reionization and Eddington luminosity with his study of Quasar. His Astrophysics research incorporates elements of Spectral line and Emission spectrum.
In Galaxy, Bram Venemans works on issues like Radius, which are connected to Halo. His Redshift research incorporates themes from Line, Luminosity, Brown dwarf and Active galactic nucleus. He works mostly in the field of Supermassive black hole, limiting it down to topics relating to Accretion and, in certain cases, Bolometric correction.
Bram Venemans mainly investigates Quasar, Astrophysics, Galaxy, Star formation and Redshift. His research integrates issues of Solar mass, Reionization, Supermassive black hole, Black hole and Emission spectrum in his study of Quasar. His Reionization study integrates concerns from other disciplines, such as Spectral line, Spectroscopy, Line-of-sight and Virial theorem.
Bram Venemans has researched Black hole in several fields, including Brightness, Submillimeter Array, Eddington luminosity and Luminous infrared galaxy. His studies deal with areas such as Radius, Surface brightness, Interstellar medium and Continuum as well as Emission spectrum. In his papers, Bram Venemans integrates diverse fields, such as Astrophysics and Blueshift.
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A luminous quasar at a redshift of z = 7.085
Daniel J. Mortlock;Stephen J. Warren;Bram P. Venemans;Mitesh Patel.
Nature (2011)
An 800-million-solar-mass black hole in a significantly neutral Universe at a redshift of 7.5
Eduardo Bañados;Bram P. Venemans;Chiara Mazzucchelli;Emanuele P. Farina.
Nature (2018)
Protoclusters associated with z > 2 radio galaxies - I. Characteristics of high redshift protoclusters
B. P. Venemans;H. J. A. Röttgering;G. K. Miley;W. J. M. Van Breugel;W. J. M. Van Breugel.
Astronomy and Astrophysics (2007)
Discovery of Three z > 6.5 Quasars in the VISTA Kilo-Degree Infrared Galaxy (VIKING) Survey
B. P. Venemans;J. R. Findlay;W. J. Sutherland;G. De Rosa.
The Astrophysical Journal (2013)
Evidence of patchy hydrogen reionization from an extreme Lyα trough below redshift six
George D. Becker;James S. Bolton;Piero Madau;Max Pettini.
Monthly Notices of the Royal Astronomical Society (2015)
The Most Distant Structure of Galaxies Known: A Protocluster at z = 4.1*
B. P. Venemans;J. D. Kurk;G. K. Miley;H. J. A. Röttgering.
The Astrophysical Journal (2002)
Detection of atomic carbon [CII] 158 micron and dust emission from a z=7.1 quasar host galaxy
B. P. Venemans;R. G. McMahon;F. Walter;R. Decarli.
arXiv: Cosmology and Nongalactic Astrophysics (2012)
Detection of Atomic Carbon [C II] 158 μm and Dust Emission from a z = 7.1 Quasar Host Galaxy
B. P. Venemans;B. P. Venemans;R. G. McMahon;F. Walter;R. Decarli.
The Astrophysical Journal (2012)
Black hole mass estimates and emission-line properties of a sample of redshift z > 6.5 quasars
Gisella De Rosa;Bram P. Venemans;Roberto Decarli;Mario Gennaro.
The Astrophysical Journal (2014)
Black hole mass estimates and emission-line properties of a sample of redshift z>6.5 quasars
G. De Rosa;B. P. Venemans;R. Decarli;M. Gennaro.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
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