2022 - Research.com Best Female Scientist Award
Her primary areas of investigation include Astrophysics, Galaxy, Astronomy, Redshift and Galaxy formation and evolution. Her study in Astrophysics focuses on Cosmology, Stars, Photometry, Galaxy merger and Universe. Her Star formation, Stellar mass, Luminosity, Active galactic nucleus and Luminosity function investigations are all subjects of Galaxy research.
Lucia Pozzetti has researched Star formation in several fields, including Extinction, Number density and Hubble Deep Field. Her biological study spans a wide range of topics, including Magnitude and Dark energy. Her study in Galaxy formation and evolution is interdisciplinary in nature, drawing from both Spectroscopy, Apparent magnitude and Spiral galaxy.
Lucia Pozzetti mainly investigates Astrophysics, Galaxy, Redshift, Astronomy and Star formation. Her study in Galaxy formation and evolution, Luminosity, Stellar mass, Luminous infrared galaxy and Redshift survey is done as part of Astrophysics. Her Galaxy study integrates concerns from other disciplines, such as Stars and Spectral line.
The various areas that Lucia Pozzetti examines in her Redshift study include COSMIC cancer database, Cosmology, Photometry, Magnitude and Emission spectrum. Her studies examine the connections between Elliptical galaxy and genetics, as well as such issues in Radio galaxy, with regards to Quasar. Her Lenticular galaxy research includes themes of Interacting galaxy and Brightest cluster galaxy.
Her primary scientific interests are in Astrophysics, Galaxy, Redshift, Star formation and Astronomy. Her work on Dark energy, Photometric redshift and Cosmology as part of general Astrophysics study is frequently linked to Context, therefore connecting diverse disciplines of science. Her studies in Stellar mass, Galaxy formation and evolution, Stellar population, Weak gravitational lensing and Metallicity are all subfields of Galaxy research.
Her work investigates the relationship between Galaxy formation and evolution and topics such as Universe that intersect with problems in Sky. The study incorporates disciplines such as Spectroscopy, COSMIC cancer database, Photometry and Emission spectrum in addition to Redshift. As part of one scientific family, Lucia Pozzetti deals mainly with the area of Star formation, narrowing it down to issues related to the Line, and often Luminosity function and Luminosity.
Lucia Pozzetti focuses on Astrophysics, Galaxy, Redshift, Stellar mass and Star formation. Photon and Scattering is closely connected to Emission spectrum in her research, which is encompassed under the umbrella topic of Astrophysics. Galaxy is a subfield of Astronomy that she tackles.
Her work carried out in the field of Redshift brings together such families of science as Line and Very Large Telescope. The various areas that she examines in her Line study include Luminosity and Luminosity function. Her research investigates the connection between Stellar mass and topics such as Dark matter that intersect with issues in Mass relation and Dark matter halo.
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)
The Star formation history of field galaxies
Piero Madau;Lucia Pozzetti;Mark Dickinson;Mark Dickinson.
The Astrophysical Journal (1998)
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)
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 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)
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)
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