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Physics

D-Index
95
Citations
31199
World Ranking
1936
National Ranking
50

Overview

Michele Trenti is affiliated with the University of Melbourne in Australia and works in the field of Physics and Astronomy. Their research interests span several subfields of study, including Astronomy and Astrophysics, Instrumentation, Aerospace Engineering, Atomic and Molecular Physics and Optics, and Computational Mechanics.

The scientist's academic work covers a range of topics such as Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, Gamma-ray Bursts and Supernovae, Stellar, Planetary, and Galactic Studies, Astrophysical Phenomena and Observations, Adaptive Optics and Wavefront Sensing, and Astrophysics and Star Formation Studies.

Among recent publications, Michele Trenti has contributed to papers including:

  • Early Results from GLASS-JWST. III. Galaxy Candidates at z ∼9-15, 2022, The Astrophysical Journal Letters
  • The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans, 2022, The Astrophysical Journal
  • The brightest galaxies at cosmic dawn, 2023, Monthly Notices of the Royal Astronomical Society
  • A highly magnified star at redshift 6.2, 2022, Nature
  • Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region, 2023, The Astrophysical Journal Letters

Michele Trenti frequently publishes in the following venues:

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

The scientist collaborates regularly with several co-authors, including Tommaso Treu, Takahiro Morishita, Guido Roberts-Borsani, Maruša Bradač, and Nicha Leethochawalit.

Best Publications

  • 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

  • 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

  • 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

  • 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

  • Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High-z Surveys

    M. Trenti;M. Stiavelli;M. Stiavelli

  • 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

  • Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: Evidence for extremely low metallicities?

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

  • Structure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imaging of the HUDF

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

  • 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

  • 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

  • LOWER-LUMINOSITY GALAXIES COULD REIONIZE THE UNIVERSE: VERY STEEP FAINT-END SLOPES TO THE UV LUMINOSITY FUNCTIONS AT z ⩾ 5-8 FROM THE HUDF09 WFC3/IR OBSERVATIONS*

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

  • Probing the Dawn of Galaxies at z ~{} 9-12 : New Constraints from HUDF12/XDF and CANDELS data

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

  • The HST eXtreme Deep Field (XDF): Combining All ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever

    G. D. Illingworth;D. Magee;P. A. Oesch;R. J. Bouwens

  • 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

  • Gravitational N-body Simulations

    M. Trenti;P. Hut

Frequent Co-Authors

Tommaso Treu
Tommaso Treu University of California, Los Angeles
Rychard Bouwens
Rychard Bouwens Leiden University
Massimo Stiavelli
Massimo Stiavelli Space Telescope Science Institute
Pascal Oesch
Pascal Oesch University of Geneva
Garth D. Illingworth
Garth D. Illingworth University of California, Santa Cruz
Ivo Labbe
Ivo Labbe Swinburne University of Technology
Gabriel B. Brammer
Gabriel B. Brammer University of Copenhagen
Masami Ouchi
Masami Ouchi University of Tokyo
Keiichi Umetsu
Keiichi Umetsu Institute of Astronomy and Astrophysics, Academia Sinica
Daniel P. Stark
Daniel P. Stark University of Arizona

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