D-Index & Metrics Best Publications

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 88 Citations 25,072 306 World Ranking 1748 National Ranking 47

Overview

What is she best known for?

The fields of study she is best known for:

  • Galaxy
  • Astrophysics
  • Astronomy

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 most cited work include:

  • UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields (924 citations)
  • UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields (882 citations)
  • 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 (619 citations)

What are the main themes of her work throughout her whole career to date?

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.

She most often published in these fields:

  • Astrophysics (98.33%)
  • Galaxy (81.86%)
  • Redshift (56.80%)

What were the highlights of her more recent work (between 2017-2021)?

  • Astrophysics (98.33%)
  • Galaxy (81.86%)
  • Redshift (56.80%)

In recent papers she was focusing on the following fields of study:

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

  • Cluster together with Astronomy, Spitzer Space Telescope, Lens and Planck,
  • Strong gravitational lensing together with James Webb Space Telescope,
  • Dark matter which intersects with area such as Magnification. Her study in Star formation is interdisciplinary in nature, drawing from both Lambda and Grism.

Between 2017 and 2021, her most popular works were:

  • The Universe Is Reionizing at z ~ 7: Bayesian Inference of the IGM Neutral Fraction Using Lyα Emission from Galaxies (125 citations)
  • Globular cluster formation and evolution in the context of cosmological galaxy assembly: open questions (64 citations)
  • Inferences on the timeline of reionization at z ∼ 8 from the KMOS Lens-Amplified Spectroscopic Survey (63 citations)

In her most recent research, the most cited papers focused on:

  • Galaxy
  • Astronomy
  • Astrophysics

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.

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.
arXiv: Cosmology and Nongalactic Astrophysics (2014)

1572 Citations

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)

1147 Citations

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)

989 Citations

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)

691 Citations

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)

593 Citations

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)

502 Citations

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)

492 Citations

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)

421 Citations

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)

391 Citations

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)

385 Citations

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