Her scientific interests lie mostly in Galaxy, Astrophysics, Redshift, Astronomy and Luminosity. Her Galaxy research is multidisciplinary, incorporating perspectives in Stars and Spectroscopy. Hubble Ultra-Deep Field, Star formation, Stellar mass, Stellar population and Universe are the core of her Astrophysics study.
Her biological study deals with issues like Sigma, which deal with fields such as Lambda. Her study looks at the intersection of Halo and topics like Cosmic variance with Halo mass function and Dark Ages. Her work deals with themes such as Optical depth and Initial mass function, which intersect with Reionization.
Her primary areas of investigation include Astrophysics, Galaxy, Redshift, Astronomy and Reionization. Her Star formation, Luminosity, Luminosity function, Stellar mass and Metallicity investigations are all subjects of Astrophysics research. Her Star formation study integrates concerns from other disciplines, such as Gamma-ray burst and COSMIC cancer database.
Her research in Galaxy tackles topics such as Stars which are related to areas like James Webb Space Telescope. Her studies in Redshift integrate themes in fields like Stellar population, Halo, Dark matter and Emission spectrum. Her Reionization research incorporates elements of Strong gravitational lensing, Equivalent width, Optical depth and Photometry.
Her main research concerns Astrophysics, Galaxy, Redshift, Reionization and Star formation. Michele Trenti has researched Galaxy in several fields, including Line, COSMIC cancer database and Photometry. Her Redshift study combines topics in areas such as Stellar population, Spectral energy distribution, Luminosity and Universe.
Her Luminosity research incorporates themes from Halo and Quasar. Her study on Reionization also encompasses disciplines like
Her primary areas of study are Galaxy, Astrophysics, Reionization, Redshift and Spitzer Space Telescope. Her Galaxy research includes themes of Line, Spatially resolved and Photometry. Her study in Astrophysics concentrates on Luminosity function, Star formation, Metallicity, COSMIC cancer database and Stellar mass.
Her research in the fields of Dark Ages overlaps with other disciplines such as Population. Her Redshift research integrates issues from Stellar population, Equivalent width, Universe and Mass distribution. Within one scientific family, Michele Trenti focuses on topics pertaining to Cluster under Spitzer Space Telescope, and may sometimes address concerns connected to Lens.
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)
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)
UV-continuum Slopes at z ~ 4-7 from the HUDF09+ERS+CANDELS Observations: Discovery of a Well-defined UV Color-Magnitude Relationship for z ≥ 4 Star-forming Galaxies
R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P.A. Oesch;M. Franx.
The Astrophysical Journal (2012)
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)
The Most Luminous z~9-10 Galaxy Candidates yet Found: The Luminosity Function, Cosmic Star-Formation Rate, and the First Mass Density Estimate at 500 Myr
P. A. Oesch;R. J. Bouwens;G. D. Illingworth;I. Labbe.
arXiv: Cosmology and Nongalactic Astrophysics (2013)
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)
A candidate redshift z ≈ 10 galaxy and rapid changes in that population at an age of 500 Myr
R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;I. Labbe;P. A. Oesch.
Nature (2011)
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