Leiden University
Netherlands
2010 - Spinoza Prize, Dutch Research Council
2009 - Royal Netherlands Academy of Arts and Sciences
Astrophysics, Galaxy, Redshift, Astronomy and Hubble Ultra-Deep Field are his primary areas of study. M. Franx undertakes interdisciplinary study in the fields of Astrophysics and Population through his works. The concepts of his Galaxy study are interwoven with issues in Photometry and Sigma.
His work in Redshift tackles topics such as Surface brightness which are related to areas like Accretion. Many of his studies involve connections with topics such as Number density and Astronomy. As a member of one scientific family, he mostly works in the field of Star formation, focusing on Universe and, on occasion, Cosmology.
M. Franx mostly deals with Astrophysics, Galaxy, Astronomy, Redshift and Star formation. M. Franx combines Astrophysics and Population in his research. His work in Stellar population, Luminosity function, Advanced Camera for Surveys, Stellar mass and Hubble Ultra-Deep Field are all subfields of Galaxy research.
His Redshift research includes elements of Fundamental plane, Photometry, Universe and Sigma. His work carried out in the field of Star formation brings together such families of science as Metallicity, Cosmic variance and Emission spectrum. M. Franx combines subjects such as Dwarf galaxy and Velocity dispersion with his study of Elliptical galaxy.
M. Franx spends much of his time researching Astrophysics, Galaxy, Astronomy, Redshift and Luminosity function. His work on Velocity dispersion, COSMIC cancer database and Universe as part of general Astrophysics research is frequently linked to Limit and Continuum, thereby connecting diverse disciplines of science. His work in Galaxy addresses issues such as Star, which are connected to fields such as Late type.
His study in the field of Galaxy formation and evolution also crosses realms of Computer science, Art and Field. Redshift connects with themes related to Sigma in his study. His studies in Luminosity function integrate themes in fields like Magnitude, Disc, Elliptical galaxy and Luminous infrared galaxy.
His primary areas of study are Galaxy, Astrophysics, Redshift, Astronomy and Luminosity function. M. Franx studied Galaxy and Stars that intersect with Spectral energy distribution. His work on Luminosity, Star formation, Star and Cosmic variance as part of his general Astrophysics study is frequently connected to Production efficiency, thereby bridging the divide between different branches of science.
His Star research is multidisciplinary, incorporating perspectives in Universe, Quasar, Radio galaxy and Gravitational lens. His Cosmic variance research is multidisciplinary, relying on both Dark Ages, Halo, Halo mass function and Sigma. His study in Astronomy is interdisciplinary in nature, drawing from both Line and Ionization.
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.
UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Trenti.
arXiv: Cosmology and Nongalactic Astrophysics (2014)
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 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)
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)
A significant population of red, near-infrared-selected high-redshift galaxies
M. Franx;I. Labbe;G. Rudnick;P. G. van Dokkum.
The Astrophysical Journal (2003)
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)
The Morphology - Density Relation in z ~ 1 Clusters
M. Postman;M. Franx;N. Cross;B. Holden.
arXiv: Astrophysics (2005)
Galaxies at z~6: The UV Luminosity Function and Luminosity Density from 506 UDF, UDF-Ps, and GOODS i-dropouts
R.J. Bouwens;G.D. Illingworth;J.P. Blakeslee;M. Franx.
arXiv: Astrophysics (2005)
IRAC Mid-Infrared Imaging of the Hubble Deep Field South: Star Formation Histories and Stellar Masses of Red Galaxies at z>2
I. Labbe;J. Huang;M. Franx;G. Rudnick.
arXiv: Astrophysics (2005)
DISCOVERY OF z ∼ 8 GALAXIES IN THE HUBBLE ULTRA DEEP FIELD FROM ULTRA-DEEP WFC3/IR OBSERVATIONS*
R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Stiavelli.
The Astrophysical Journal (2010)
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:
Swinburne University of Technology
National Optical-Infrared Astronomy Research Lab
Space Telescope Science Institute
Johns Hopkins University
Leiden University
University of Western Australia
University of California, Santa Cruz
University of Edinburgh
University of Illinois at Urbana-Champaign
Pontificia Universidad Católica de Chile
Microsoft Research Asia (China)
University of California, Los Angeles
Agricultural University of Athens
University of Zurich
Saarland University
Goddard Institute for Space Studies
University of Tokyo
Boston University
Columbia University
University of Iowa
The Ohio State University
Qingdao University
Sapienza University of Rome
University of Minnesota
Osaka University
University of Cincinnati