Her scientific interests lie mostly in Astrophysics, Galaxy, Astronomy, Redshift and Galaxy formation and evolution. Her Astrophysics study focuses mostly on Star formation, Luminous infrared galaxy, Elliptical galaxy, Stellar mass and Lenticular galaxy. Andrea Cimatti works mostly in the field of Stellar mass, limiting it down to topics relating to Luminosity function and, in certain cases, Satellite galaxy, as a part of the same area of interest.
Her studies deal with areas such as Stars and Photometry as well as Galaxy. The Redshift study combines topics in areas such as Cosmology, COSMIC cancer database, Infrared and Cosmic background radiation. The study incorporates disciplines such as Spectroscopy and Metallicity in addition to Galaxy formation and evolution.
Andrea Cimatti spends much of her time researching Astrophysics, Galaxy, Redshift, Astronomy and Star formation. As part of the same scientific family, Andrea Cimatti usually focuses on Astrophysics, concentrating on Emission spectrum and intersecting with Line. The concepts of her Galaxy study are interwoven with issues in Cosmology and Spectral line.
Andrea Cimatti interconnects Stars, Dark energy, Infrared and COSMIC cancer database in the investigation of issues within Redshift. Lenticular galaxy, Radio galaxy, Quasar, Galaxy merger and Peculiar galaxy are the core of her Astronomy study. Her Star formation study incorporates themes from Accretion, Metallicity, Spectroscopy, Luminosity function and Extinction.
Her primary scientific interests are in Galaxy, Astrophysics, Redshift, Star formation and Stellar mass. Her study in Galaxy focuses on Galaxy formation and evolution in particular. Her Astrophysics study integrates concerns from other disciplines, such as Spectral line and Emission spectrum.
She has researched Redshift in several fields, including Spectral energy distribution, Atacama Large Millimeter Array, Interstellar medium and Equivalent width. Andrea Cimatti studied Star formation and Photometric redshift that intersect with Cosmic infrared background. Her work carried out in the field of Stellar mass brings together such families of science as Surface brightness and Bulge.
Andrea Cimatti focuses on Galaxy, Astrophysics, Redshift, Star formation and Stellar mass. Her work in the fields of Methods statistical, Metallicity and Submillimeter Array overlaps with other areas such as Velocity gradient. Her Astrophysics study combines topics from a wide range of disciplines, such as Spectral evolution and Emission spectrum.
Her biological study spans a wide range of topics, including Spectral line, Spectral energy distribution and Atacama Large Millimeter Array. Her research in Star formation intersects with topics in Line, Equivalent width and Galaxy formation and evolution. Her Galaxy formation and evolution research is multidisciplinary, relying on both Doubly ionized oxygen, Flattening, Interstellar medium and Balmer series.
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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)
Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
E. Daddi;M. Dickinson;G. Morrison;R. Chary.
The Astrophysical Journal (2007)
THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OF z ∼ 2 STAR-FORMING GALAXIES*
N. M. Förster Schreiber;R. Genzel;N. Bouché;G. Cresci.
The Astrophysical Journal (2009)
AMAZE - I. The evolution of the mass–metallicity relation at z $>$ 3
R. Maiolino;T. Nagao;A. Grazian;F. Cocchia.
Astronomy and Astrophysics (2008)
PASSIVELY EVOLVING EARLY-TYPE GALAXIES AT 1.4 z 2.5 IN THE HUBBLE ULTRA DEEP FIELD
E. Daddi;A. Renzini;N. Pirzkal;Andrea Cimatti.
The Astrophysical Journal (2005)
The Lesser Role of Starbursts in Star Formation at z = 2
G. Rodighiero;E. Daddi;I. Baronchelli;A. Cimatti.
The Astrophysical Journal (2011)
GMASS Ultradeep Spectroscopy of Galaxies at 1.4<z<2. II. Superdense passive galaxies: how did they form and evolve ?
A. Cimatti;P. Cassata;L. Pozzetti;J. Kurk.
arXiv: Astrophysics (2008)
A New Photometric Technique for the Joint Selection of Star-forming and Passive Galaxies at 1.4 <~ z <~ 2.5
E. Daddi;Andrea Cimatti;A. Renzini;A. Fontana.
The Astrophysical Journal (2004)
Submillimeter Galaxies at z ~ 2: Evidence for Major Mergers and Constraints on Lifetimes, IMF, and CO-H2 Conversion Factor*
L. J. Tacconi;R. Genzel;I. Smail;R. Neri.
web science (2008)
From Rings to Bulges: Evidence for Rapid Secular Galaxy Evolution at z ~ 2 from Integral Field Spectroscopy in the SINS Survey
R. Genzel;A. Burkert;N. Bouché;G. Cresci.
The Astrophysical Journal (2008)
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