University of California, Santa Cruz
United States
His primary areas of investigation include Astrophysics, Galaxy, Astronomy, Luminosity and Redshift. Galaxy cluster, ROSAT, Advanced Camera for Surveys, Stellar mass and Luminosity function are the core of his Astrophysics study. He combines subjects such as Stars and Photometry with his study of Galaxy.
His is involved in several facets of Astronomy study, as is seen by his studies on Galaxy formation and evolution and Luminous infrared galaxy. Bradford P. Holden works mostly in the field of Luminosity, limiting it down to topics relating to Radius and, in certain cases, Line-of-sight, Brightness and Radiation pressure, as a part of the same area of interest. Spitzer Space Telescope, Star and Redshift survey is closely connected to Quasar in his research, which is encompassed under the umbrella topic of Redshift.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Astronomy, Redshift and Galaxy cluster. His study in Luminosity function, Elliptical galaxy, Luminosity, Galaxy formation and evolution and ROSAT falls under the purview of Astrophysics. While the research belongs to areas of Galaxy, Bradford P. Holden spends his time largely on the problem of Stars, intersecting his research to questions surrounding Spectral line.
His study focuses on the intersection of Redshift and fields such as Magnitude with connections in the field of Epoch. His research in Galaxy cluster intersects with topics in Near-infrared spectroscopy and Velocity dispersion. His Star formation research incorporates themes from Metallicity and Disc galaxy.
His main research concerns Astrophysics, Planet, Galaxy, Astronomy and Radial velocity. His Astrophysics study combines topics from a wide range of disciplines, such as Doubly ionized oxygen, Spectroscopy and Radius. His Planet research focuses on subjects like Stars, which are linked to Star.
His study on Redshift, Star formation, Reionization and Rest frame is often connected to Spheroid as part of broader study in Galaxy. His Redshift course of study focuses on Stellar mass and Spatially resolved, Photometry and Photometry. His Wide field research extends to Astronomy, which is thematically connected.
Astrophysics, Galaxy, Astronomy, Planet and Redshift are his primary areas of study. In general Astrophysics study, his work on Terrestrial planet and Minimum mass often relates to the realm of Range, Atmospheric composition and Instability, thereby connecting several areas of interest. His work is dedicated to discovering how Galaxy, Doubly ionized oxygen are connected with Line, Spectroscopy and Luminosity function and other disciplines.
His Photometry, Galaxy group, Hubble space telescope and Star study, which is part of a larger body of work in Astronomy, is frequently linked to Field, bridging the gap between disciplines. His study in the field of Exoplanet, Super-Earth and Mean motion also crosses realms of Symplectic integrator. His Redshift research focuses on Stellar mass and how it connects with Luminosity and James Webb Space Telescope.
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.
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)
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)
The Morphology - Density Relation in z ~ 1 Clusters
M. Postman;M. Franx;N. Cross;B. Holden.
arXiv: Astrophysics (2005)
The Morphology-Density Relation in z ~ 1 Clusters
M. Postman;M. Franx;N.J.G. Cross;B. Holden.
The Astrophysical Journal (2005)
Measuring Ωm with the ROSAT Deep Cluster Survey
Stefano Borgani;Piero Rosati;Paolo Tozzi;S. A. Stanford;S. A. Stanford.
The Astrophysical Journal (2001)
From Shock Breakout to Peak and Beyond: Extensive Panchromatic Observations of the Type Ib Supernova 2008D associated with Swift X-ray Transient 080109
Maryam Modjaz;W. Li;N. Butler;R. Chornock.
arXiv: Astrophysics (2008)
Measuring $\Omega_m$ with the ROSAT Deep Cluster Survey
S. Borgani;P. Rosati;P. Tozzi;S.A. Stanford.
arXiv: Astrophysics (2001)
A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy
P.A. Oesch;G. Brammer;P.G. van Dokkum;G.D. Illingworth.
The Astrophysical Journal (2016)
STRONG-LENSING ANALYSIS OF A1689 FROM DEEP ADVANCED CAMERA IMAGES
Tom Broadhurst;Narciso Benítez;Narciso Benítez;Dan Coe;Keren Sharon.
The Astrophysical Journal (2005)
RECENT STRUCTURAL EVOLUTION OF EARLY-TYPE GALAXIES : SIZE GROWTH FROM z = 1 TO z = 0
Arjen van der Wel;Bradford P. Holden;Andrew W. Zirm;Marijn Franx.
The Astrophysical Journal (2008)
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