His primary areas of study are Astrophysics, Galaxy, Redshift, Astronomy and Luminosity. All of his Astrophysics and Stellar mass, Metallicity, Luminosity function, Star formation and Galaxy formation and evolution investigations are sub-components of the entire Astrophysics study. His studies deal with areas such as Stars, Equivalent width, Black hole and Sky as well as Galaxy.
The Stars study which covers Line that intersects with Multi Unit Spectroscopic Explorer. His Redshift research is multidisciplinary, incorporating elements of Magnitude and Milky Way. Jarle Brinchmann works mostly in the field of Luminosity, limiting it down to topics relating to Quasar and, in certain cases, Nebula, Intergalactic travel and Surface brightness, as a part of the same area of interest.
Jarle Brinchmann spends much of his time researching Astrophysics, Galaxy, Redshift, Astronomy and Star formation. His Astrophysics research is multidisciplinary, relying on both Spectral line and Emission spectrum. His work focuses on many connections between Galaxy and other disciplines, such as Line, that overlap with his field of interest in Active galactic nucleus.
His Redshift study combines topics from a wide range of disciplines, such as Halo, Luminosity, Quasar, Photometry and Magnitude. As part of one scientific family, Jarle Brinchmann deals mainly with the area of Star formation, narrowing it down to issues related to the Dark matter, and often Dark matter halo. His research in Metallicity tackles topics such as Wolf–Rayet star which are related to areas like O-type star.
His primary areas of investigation include Astrophysics, Galaxy, Redshift, Emission spectrum and Stellar mass. In his research, Jarle Brinchmann performs multidisciplinary study on Astrophysics and Kinematics. His work investigates the relationship between Galaxy and topics such as Dark energy that intersect with problems in Structure formation.
His Redshift course of study focuses on Equivalent width and Reionization and Quasar. Jarle Brinchmann interconnects Star formation, Active galactic nucleus and Accretion in the investigation of issues within Emission spectrum. His study focuses on the intersection of Stellar mass and fields such as Spectral line with connections in the field of Stellar population, Stellar rotation and Line.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Halo and Equivalent width. His Astrophysics study frequently draws connections between adjacent fields such as Emission spectrum. His work deals with themes such as Star formation, Quasar and Dark matter, which intersect with Emission spectrum.
His Galaxy research incorporates elements of Point spread function and Statistical physics. His Velocity dispersion research is multidisciplinary, incorporating perspectives in Accretion, Active galactic nucleus, Bulge and Supermassive black hole, Black hole. His Reionization research incorporates themes from Spectroscopy, Photometry and Photon.
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.
The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS
C. A. Tremonti;T. M. Heckman;G. Kauffmann;J. Brinchmann.
arXiv: Astrophysics (2004)
The Host Galaxies of AGN
Guinevere Kauffmann;Timothy M. Heckman;Christy Tremonti;Jarle Brinchmann.
arXiv: Astrophysics (2003)
Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey
Guinevere Kauffmann;Timothy M. Heckman;Simon D.M. White;Stephane Charlot.
arXiv: Astrophysics (2002)
The Sixth Data Release of the Sloan Digital Sky Survey
Jennifer K. Adelman-McCarthy;Marcel A. Agüeros;Sahar S. Allam;Sahar S. Allam;Carlos Allende Prieto.
Astrophysical Journal Supplement Series (2008)
Present-Day Growth of Black Holes and Bulges: the SDSS Perspective
Timothy M. Heckman;Guinevere Kauffmann;Jarle Brinchmann;Stephane Charlot.
arXiv: Astrophysics (2004)
The host galaxies of radio-loud AGN: mass dependencies, gas cooling and AGN feedback
P. N. Best;G. Kauffmann;T. M. Heckman;J. Brinchmann.
arXiv: Astrophysics (2005)
Ages and metallicities of early-type galaxies in the SDSS: new insight into the physical origin of the colour-magnitude and the Mg2-sigmaV relations
A. Gallazzi;S. Charlot;J. Brinchmann;S.D.M. White.
arXiv: Astrophysics (2006)
New insights into the stellar content and physical conditions of star-forming galaxies at z = 2-3 from spectral modelling
Jarle Brinchmann;Max Pettini;Stéphane Charlot.
Monthly Notices of the Royal Astronomical Society (2008)
Hubble Space Telescope imaging of the CFRS and LDSS redshift surveys II: Structural parameter and the evolution of disk galaxies to z=1
S. J. Lilly;D. Schade;R. S. Ellis;O. Le Fevre.
arXiv: Astrophysics (1997)
Extended Lyman alpha haloes around individual high-redshift galaxies revealed by MUSE
L. Wisotzki;R. Bacon;J. Blaizot;J. Brinchmann.
arXiv: Astrophysics of Galaxies (2015)
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:
École Normale Supérieure de Lyon
Federal University of Toulouse Midi-Pyrénées
Leiden University
National Institute for Astrophysics
National Institute for Astrophysics
National Institute for Astrophysics
University of Milan
National Institute for Astrophysics
National Institute for Astrophysics
Federal University of Toulouse Midi-Pyrénées
University of Manchester
University of Virginia
Nottingham Trent University
Hong Kong University of Science and Technology
University of Warwick
Delft University of Technology
Institució Catalana de Recerca i Estudis Avançats
London School of Hygiene & Tropical Medicine
Oklahoma State University
University of Saskatchewan
University of Southern California
Sewanee: The University of the South
University of Modena and Reggio Emilia
Illinois State University
University Hospital Heidelberg
Tulane University