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Physics

D-Index
132
Citations
57188
World Ranking
532
National Ranking
12

Overview

Pascal Oesch is affiliated with the University of Geneva in Switzerland. Their research spans the domains of Physics and Astronomy, with a total of 716 publications contributing to this broad field.

Their work is especially concentrated within several subfields, including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Atomic and Molecular Physics and Optics, and Computational Mechanics.

Key topics covered in Oesch's research include:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Astrophysics and Star Formation Studies
  • Stellar, planetary, and galactic studies
  • Astrophysical Phenomena and Observations
  • Astrophysics and Cosmic Phenomena

Their recent publications in peer-reviewed journals highlight active involvement in cutting-edge astrophysical research. Selected papers include:

  • "Two Remarkably Luminous Galaxy Candidates at z ≈ 10-12 Revealed by JWST," 2022, The Astrophysical Journal Letters
  • "Little Red Dots: An Abundant Population of Faint Active Galactic Nuclei at z ∼ 5 Revealed by the EIGER and FRESCO JWST Surveys," 2024, The Astrophysical Journal
  • "UNCOVER Spectroscopy Confirms the Surprising Ubiquity of Active Galactic Nuclei in Red Sources at z > 5," 2024, The Astrophysical Journal
  • "The ALPINE-ALMA [CII] survey," 2020, Astronomy and Astrophysics
  • "Reionization Era Bright Emission Line Survey: Selection and Characterization of Luminous Interstellar Medium Reservoirs in the z > 6.5 Universe," 2022, The Astrophysical Journal

They have published extensively in several venues, including:

  • arXiv (Cornell University)
  • Astronomy and Astrophysics
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal Letters

Frequent collaborators in Oesch's research include Gabriel Brammer, Ivo Labbé, R. J. Bouwens, Mauro Stefanon, and Rohan P. Naidu, indicating active engagement in collaborative scientific efforts.

Best Publications

  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Y. Peng;S. J. Lilly;K. Kovac;M. Bolzonella

  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Ying-jie Peng;Simon J. Lilly;Katarina Kovač;Micol Bolzonella

  • 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

  • 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

  • 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

  • 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

  • The 3D-HST Survey: Hubble Space Telescope WFC3/G141 grism spectra, redshifts, and emission line measurements for $\sim 100,000$ galaxies

    Ivelina G. Momcheva;Gabriel B. Brammer;Pieter G. van Dokkum;Rosalind E. Skelton

  • The zCOSMOS 10k-Bright Spectroscopic Sample

    Simon J. Lilly;Vincent Le Brun;Christian Maier;Vincenzo Mainieri

  • 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

  • zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift

    L. Pozzetti;M. Bolzonella;E. Zucca;G. Zamorani

  • 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

  • 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

  • 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 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

  • 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

  • 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 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

  • The Dearth of z ∼ 10 Galaxies in All HST Legacy Fields—The Rapid Evolution of the Galaxy Population in the First 500 Myr

    P.A. Oesch;R.J. Bouwens;G.D. Illingworth;I.F.L. Labbé

  • 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

  • UV Luminosity Functions at redshifts z~4 to z~10: 11000 Galaxies from HST Legacy Fields

    R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Trenti

Frequent Co-Authors

Rychard Bouwens
Rychard Bouwens Leiden University
Garth D. Illingworth
Garth D. Illingworth University of California, Santa Cruz
Michele Trenti
Michele Trenti University of Melbourne
S. Bardelli
S. Bardelli National Institute for Astrophysics
Thierry Contini
Thierry Contini Research Institute in Astrophysics and Planetology
Franz E. Bauer
Franz E. Bauer Pontificia Universidad Católica de Chile
Andrea Cimatti
Andrea Cimatti University of Bologna
Elena Zucca
Elena Zucca National Institute for Astrophysics
Peter Capak
Peter Capak California Institute of Technology
Marijn Franx
Marijn Franx Leiden University

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