D-Index & Metrics Best Publications

D-Index & Metrics D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines.

Discipline name D-index D-index (Discipline H-index) only includes papers and citation values for an examined discipline in contrast to General H-index which accounts for publications across all disciplines. Citations Publications World Ranking National Ranking
Physics D-index 118 Citations 56,082 573 World Ranking 566 National Ranking 22

Overview

What is she best known for?

The fields of study she is best known for:

  • Galaxy
  • Astronomy
  • Astrophysics

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.

Her most cited work include:

  • Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth (1468 citations)
  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function (1450 citations)
  • THE SINS SURVEY: SINFONI INTEGRAL FIELD SPECTROSCOPY OF z ∼ 2 STAR-FORMING GALAXIES* (1018 citations)

What are the main themes of her work throughout her whole career to date?

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.

She most often published in these fields:

  • Astrophysics (105.24%)
  • Galaxy (90.12%)
  • Redshift (64.72%)

What were the highlights of her more recent work (between 2018-2021)?

  • Galaxy (90.12%)
  • Astrophysics (105.24%)
  • Redshift (64.72%)

In recent papers she was focusing on the following fields of study:

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.

Between 2018 and 2021, her most popular works were:

  • The ALPINE-ALMA [CII] Survey: Data processing, catalogs, and statistical source properties (46 citations)
  • The ALPINE–ALMA [C ii] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements (41 citations)
  • The ALPINE–ALMA [C ii] Survey: Multiwavelength Ancillary Data and Basic Physical Measurements (41 citations)

In her most recent research, the most cited papers focused on:

  • Galaxy
  • Astronomy
  • Astrophysics

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.

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.

Best Publications

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)

1774 Citations

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)

1748 Citations

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)

1173 Citations

AMAZE - I. The evolution of the mass–metallicity relation at z $>$ 3

R. Maiolino;T. Nagao;A. Grazian;F. Cocchia.
Astronomy and Astrophysics (2008)

1100 Citations

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)

994 Citations

The Lesser Role of Starbursts in Star Formation at z = 2

G. Rodighiero;E. Daddi;I. Baronchelli;A. Cimatti.
The Astrophysical Journal (2011)

928 Citations

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)

876 Citations

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)

875 Citations

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)

848 Citations

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)

756 Citations

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