His primary areas of investigation include Astrophysics, Galaxy, Redshift, Astronomy and Galaxy formation and evolution. His is involved in several facets of Astrophysics study, as is seen by his studies on Redshift survey, Luminosity, Active galactic nucleus, Cosmology and Luminosity function. His work in Galaxy is not limited to one particular discipline; it also encompasses Universe.
His Redshift study incorporates themes from Magnitude, Spectral line, ROSAT and Stars. His Astronomy study frequently draws connections between adjacent fields such as Sample. His work on Peculiar galaxy is typically connected to High density as part of general Galaxy formation and evolution study, connecting several disciplines of science.
His primary areas of study are Astrophysics, Galaxy, Redshift, Astronomy and Redshift survey. All of his Astrophysics and Galaxy formation and evolution, Star formation, Luminosity, Luminosity function and Active galactic nucleus investigations are sub-components of the entire Astrophysics study. His studies deal with areas such as Extinction and Spectral energy distribution as well as Star formation.
His study of Stellar mass is a part of Galaxy. His work carried out in the field of Redshift brings together such families of science as Magnitude, Universe, Dark matter and Emission spectrum. His Redshift survey study integrates concerns from other disciplines, such as COSMIC cancer database, Limiting magnitude, Very Large Telescope and Sigma.
D. Maccagni mainly investigates Astrophysics, Galaxy, Redshift, Redshift survey and Astronomy. His study in Star formation, Galaxy formation and evolution, Very Large Telescope, Reionization and Extinction falls within the category of Astrophysics. In general Galaxy study, his work on Stellar mass and Luminosity often relates to the realm of Context, thereby connecting several areas of interest.
His Stellar mass research is multidisciplinary, incorporating elements of Accretion and Billion years. His research in Redshift intersects with topics in Spectral energy distribution, Stars, Photometry, Active galactic nucleus and Sigma. His Redshift survey research incorporates elements of Cosmology, Satellite galaxy, Telescope and Spectral density.
His primary scientific interests are in Astrophysics, Galaxy, Redshift, Astronomy and Star formation. In his research, Spectrograph, Sky and Data reduction is intimately related to Data set, which falls under the overarching field of Astrophysics. He mostly deals with Galaxy formation and evolution in his studies of Galaxy.
His Redshift research includes elements of Spectral energy distribution, Stars, Very Large Telescope, Active galactic nucleus and Stellar mass. Specifically, his work in Astronomy is concerned with the study of Luminous infrared galaxy. His studies in Star formation integrate themes in fields like Spectroscopy and Emission spectrum.
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)
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)
Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey
M. Polletta;M. Tajer;L. Maraschi;G. Trinchieri.
arXiv: Astrophysics (2007)
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)
Spectral Energy Distributions of Hard X-Ray Selected Active Galactic Nuclei in the XMM-Newton Medium Deep Survey
M. Polletta;M. Tajer;L. Maraschi;G. Trinchieri.
The Astrophysical Journal (2007)
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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