His primary areas of investigation include Astrophysics, Galaxy, Redshift, Astronomy and Galaxy formation and evolution. His Astrophysics study is mostly concerned with Active galactic nucleus, Luminosity, Redshift survey, Luminosity function and Cosmology. The various areas that S. Bardelli examines in his Galaxy study include Stars and Universe.
His studies in Redshift integrate themes in fields like Magnitude, Spectral line and Photometry. His Galaxy formation and evolution study deals with Apparent magnitude intersecting with Data reduction. The concepts of his Star formation study are interwoven with issues in Number density and Accretion.
S. Bardelli mainly focuses on Astrophysics, Galaxy, Redshift, Astronomy and Star formation. All of his Astrophysics and Galaxy formation and evolution, Stellar mass, Luminosity, Galaxy cluster and Redshift survey investigations are sub-components of the entire Astrophysics study. S. Bardelli has researched Galaxy in several fields, including Stars and Spectral line.
His work is dedicated to discovering how Redshift, Emission spectrum are connected with Line and other disciplines. Luminous infrared galaxy, Radio galaxy, Elliptical galaxy, X-shaped radio galaxy and Brightest cluster galaxy are among the areas of Astronomy where he concentrates his study. His work carried out in the field of Star formation brings together such families of science as Extinction, Spectral energy distribution and Universe.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Star formation and Stellar mass. S. Bardelli frequently studies issues relating to Spectral line and Astrophysics. As a part of the same scientific study, S. Bardelli usually deals with the Galaxy, concentrating on Equivalent width and frequently concerns with Cosmic time.
His study on Redshift is covered under Astronomy. His study looks at the relationship between Star formation and fields such as Baryon, as well as how they intersect with chemical problems. His biological study spans a wide range of topics, including Cosmology, Dark energy and Cluster analysis.
The scientist’s investigation covers issues in Astrophysics, Galaxy, Redshift, Star formation and Galaxy formation and evolution. His Astrophysics study combines topics from a wide range of disciplines, such as Spectral line and Algorithm. His Galaxy study results in a more complete grasp of Astronomy.
His Redshift study integrates concerns from other disciplines, such as Equivalent width, Emission spectrum, Sky, Continuum and Line. His Star formation research is multidisciplinary, relying on both Low Mass, Baryon, Photometry and Dwarf galaxy. His work deals with themes such as Extinction, Cosmic variance, QSOS and Line-of-sight, which intersect with Galaxy formation and evolution.
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
Y. Peng;S. J. Lilly;K. Kovac;M. Bolzonella.
arXiv: Cosmology and Nongalactic Astrophysics (2010)
Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey
O. Ilbert;S. Arnouts;H.J. McCracken;M. Bolzonella.
arXiv: Astrophysics (2006)
Euclid Definition Study Report
N. Shane;J.~-. Starck;C. Surace;A. Taylor.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
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)
Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey
O. Ilbert;O. Ilbert;S. Arnouts;H. J. Mccracken;M. Bolzonella.
Astronomy and Astrophysics (2006)
COSMOS Photometric Redshifts with 30-bands for 2-deg2
O. Ilbert;P. Capak;M. Salvato;H. Aussel.
The Astrophysical Journal (2009)
zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 < z < 3 in the COSMOS Field*
S. J. Lilly;O. Le Fèvre;A. Renzini;G. Zamorani.
Astrophysical Journal Supplement Series (2007)
The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5
O. Le Fevre;G. Vettolani;B. Garilli;L. Tresse.
arXiv: Astrophysics (2004)
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)
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