His main research concerns Astrophysics, Galaxy, Redshift, Astronomy and Stellar mass. His Astrophysics study focuses mostly on Star formation, Reionization, Hubble Ultra-Deep Field, Galaxy formation and evolution and Luminosity. The concepts of his Star formation study are interwoven with issues in Extinction and Surface brightness.
His work on Galaxy deals in particular with Luminosity function, Grism, Quasar, Luminous infrared galaxy and Wide Field Camera 3. His work deals with themes such as Dark matter halo, Doubly ionized oxygen, Emission spectrum, Spectroscopy and Cosmology, which intersect with Redshift. His research integrates issues of Hubble Deep Field and Velocity dispersion in his study of Stellar mass.
His primary areas of study are Galaxy, Astrophysics, Redshift, Astronomy and Star formation. The various areas that he examines in his Galaxy study include COSMIC cancer database and Photometry. His study connects Infrared and Astrophysics.
His Redshift research is multidisciplinary, incorporating elements of Cosmology, Equivalent width, Universe and Spectral energy distribution. His Star formation research includes elements of Accretion, Metallicity and Photometric redshift. His research investigates the link between Reionization and topics such as Wide Field Camera 3 that cross with problems in Advanced Camera for Surveys.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Star formation and Stellar mass. His study in Luminosity function, Line, Spectral energy distribution, Photometric redshift and Millimeter are all subfields of Astrophysics. He has included themes like Cosmology and Dark galaxy in his Photometric redshift study.
His studies deal with areas such as COSMIC cancer database, Equivalent width and Continuum as well as Galaxy. He combines subjects such as Luminosity, Universe and Infrared, Infrared excess with his study of Redshift. He has researched Stellar mass in several fields, including Cosmic time, Halo and Baryon.
Pascal Oesch mostly deals with Astrophysics, Galaxy, Redshift, Star formation and Hubble Ultra-Deep Field. His work in Reionization, Stellar mass, Infrared excess, Universe and Luminosity function are all subfields of Astrophysics research. His research in Luminosity function intersects with topics in Quasar, Bright star and Photon.
His Galaxy research includes themes of COSMIC cancer database, Infrared and Millimeter. His Redshift research is multidisciplinary, incorporating perspectives in Atacama Large Millimeter Array, Spectral energy distribution, Luminosity and Line. The study incorporates disciplines such as Doubly ionized oxygen, Spectral line, Galaxy formation and evolution and Interstellar medium in addition to Star formation.
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: 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)
3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts, and Stellar Masses
Rosalind E. Skelton;Katherine E. Whitaker;Ivelina G. Momcheva;Gabriel B. Brammer.
Astrophysical Journal Supplement Series (2014)
Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers
M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti.
Journal of Cosmology and Astroparticle Physics (2012)
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)
THE 3D-HST SURVEY: HUBBLE SPACE TELESCOPE WFC3/G141 GRISM SPECTRA, REDSHIFTS, AND EMISSION LINE MEASUREMENTS FOR ∼100,000 GALAXIES
Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. Van Dokkum;Rosalind E. Skelton.
Astrophysical Journal Supplement Series (2016)
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)
Reionization after Planck: The Derived Growth of the Cosmic Ionizing Emissivity now matches the Growth of the Galaxy UV Luminosity Density
R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;J. Caruana.
The Astrophysical Journal (2015)
UV-CONTINUUM SLOPES OF >4000 z ∼ 4-8 GALAXIES FROM THE HUDF/XDF, HUDF09, ERS, CANDELS-SOUTH, AND CANDELS-NORTH FIELDS
R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbé.
The Astrophysical Journal (2014)
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)
z ∼ 7 GALAXIES IN THE HUDF: FIRST EPOCH WFC3/IR RESULTS*
P. A. Oesch;R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;C. M. Carollo.
The Astrophysical Journal (2010)
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