Thierry Contini mainly focuses on Astrophysics, Galaxy, Astronomy, Redshift and Star formation. Galaxy formation and evolution, Stellar mass, Luminous infrared galaxy, Elliptical galaxy and Luminosity function are the primary areas of interest in his Astrophysics study. His Elliptical galaxy research focuses on Radio galaxy and how it relates to Disc.
Thierry Contini studied Galaxy and Emission spectrum that intersect with Metallicity. His work on Hubble Ultra-Deep Field as part of his general Redshift study is frequently connected to Population, thereby bridging the divide between different branches of science. As part of one scientific family, Thierry Contini deals mainly with the area of Star formation, narrowing it down to issues related to the Accretion, and often Interstellar medium.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Astronomy and Star formation. His work in the fields of Astrophysics, such as Stellar mass, Galaxy formation and evolution, Luminosity and Luminous infrared galaxy, intersects with other areas such as Population. His study in Emission spectrum extends to Galaxy with its themes.
His research in Redshift intersects with topics in COSMIC cancer database, Satellite galaxy, Halo, Cosmology and Velocity dispersion. The various areas that Thierry Contini examines in his Star formation study include Accretion, Extinction, Interstellar medium and Luminosity function. The Active galactic nucleus study combines topics in areas such as Line and Supermassive black hole.
His primary areas of investigation include Astrophysics, Galaxy, Redshift, Hubble Ultra-Deep Field and Star formation. His research links Astronomy with Astrophysics. His Galaxy research incorporates elements of Line and Spectral line, Emission spectrum.
His Redshift research integrates issues from Equivalent width, Low Mass and Velocity dispersion. His Hubble Ultra-Deep Field research includes themes of Luminosity, Luminosity function, Scattering and Integral field spectrograph. His Star formation study combines topics in areas such as Accretion, Surface brightness and Reionization.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Hubble Ultra-Deep Field and Star formation. In most of his Astrophysics studies, his work intersects topics such as Astronomy. His Galaxy research is multidisciplinary, incorporating elements of Spectral line and Millimeter.
His work in Redshift tackles topics such as Dark matter halo which are related to areas like Virial theorem. His Hubble Ultra-Deep Field research incorporates themes from Spectroscopy, COSMIC cancer database, Luminosity function, Galaxy formation and evolution and Emission spectrum. The concepts of his Gas depletion study are interwoven with issues in Mass relation, Interstellar medium, Initial mass function and Luminous infrared galaxy.
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.
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.
The Astrophysical Journal (2010)
A test of the nature of cosmic acceleration using galaxy redshift distortions
L. Guzzo;M. Pierleoni;B. Meneux;E. Branchini.
Nature (2008)
The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5
O. Le Fèvre;G. Vettolani;B. Garilli;L. Tresse.
Astronomy and Astrophysics (2005)
The zCOSMOS 10k-Bright Spectroscopic Sample
Simon J. Lilly;Vincent Le Brun;Christian Maier;Vincenzo Mainieri.
Astrophysical Journal Supplement Series (2009)
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)
COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS
R. Genzel;L. J. Tacconi;D. Lutz;A. Saintonge.
The Astrophysical Journal (2015)
PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
L. J. Tacconi;R. Genzel;A. Saintonge;F. Combes.
The Astrophysical Journal (2018)
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.
Astronomy and Astrophysics (2010)
The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4
C. Gruppioni;F. Pozzi;G. Rodighiero;I. Delvecchio.
Monthly Notices of the Royal Astronomical Society (2013)
The Vimos VLT deep survey - stellar mass segregation and large-scale galaxy environment in the redshift range 0.2 < z < 1.4
M. Scodeggio;D. Vergani;D. Vergani;O. Cucciati;O. Cucciati;A. Iovino.
Astronomy and Astrophysics (2009)
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