What is he best known for?
The fields of study he is best known for:
- Quantum mechanics
- Galaxy
- Astronomy
His scientific interests lie mostly in Astrophysics, Galaxy, Astronomy, Redshift and Dark matter.
His study in Galaxy formation and evolution, Star formation, Cosmology, Stellar mass and Quasar is carried out as part of his studies in Astrophysics.
His studies deal with areas such as Luminosity and Density contrast as well as Star formation.
The concepts of his Galaxy study are interwoven with issues in COSMIC cancer database and Photometry.
Cristiano Porciani usually deals with Redshift and limits it to topics linked to Surface brightness and Irregular galaxy.
His Dark matter research includes elements of Halo and Mass distribution.
His most cited work include:
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function (1450 citations)
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function (1431 citations)
- Cosmology and Fundamental Physics with the Euclid Satellite (903 citations)
What are the main themes of his work throughout his whole career to date?
Cristiano Porciani mainly focuses on Astrophysics, Galaxy, Redshift, Astronomy and Halo.
Dark matter, Galaxy formation and evolution, Redshift survey, Luminosity and Quasar are among the areas of Astrophysics where the researcher is concentrating his efforts.
His Dark matter research also works with subjects such as
- Cosmology which is related to area like COSMIC cancer database,
- Dark energy which is related to area like Weak gravitational lensing.
In his work, Amplitude and Anisotropy is strongly intertwined with Field, which is a subfield of Galaxy.
His Redshift study integrates concerns from other disciplines, such as Spectral line and Surface brightness.
His work investigates the relationship between Halo and topics such as Statistical physics that intersect with problems in Gaussian and Halo effect.
He most often published in these fields:
- Astrophysics (100.90%)
- Galaxy (65.92%)
- Redshift (58.30%)
What were the highlights of his more recent work (between 2013-2021)?
- Astrophysics (100.90%)
- Redshift (58.30%)
- Statistical physics (12.11%)
In recent papers he was focusing on the following fields of study:
Cristiano Porciani mostly deals with Astrophysics, Redshift, Statistical physics, Galaxy and Halo.
His Astrophysics research incorporates elements of Field, Astronomy and Cosmic microwave background.
His study looks at the intersection of Redshift and topics like Cold dark matter with Structure formation.
His research in Statistical physics intersects with topics in Gaussian and Perturbation theory.
He specializes in Galaxy, namely Galaxy formation and evolution.
His research integrates issues of Accretion, Dark matter and Hydrogen line in his study of Halo.
Between 2013 and 2021, his most popular works were:
- PROBING THE ISOTROPY OF COSMIC ACCELERATION TRACED BY TYPE Ia SUPERNOVAE (77 citations)
- Cosmological information in the redshift-space bispectrum (59 citations)
- ZOMG - I. How the cosmic web inhibits halo growth and generates assembly bias (57 citations)
In his most recent research, the most cited papers focused on:
- Quantum mechanics
- Astronomy
- Galaxy
His primary scientific interests are in Redshift, Astrophysics, Galaxy, Dark energy and Field.
To a larger extent, Cristiano Porciani studies Astronomy with the aim of understanding Redshift.
His work in Astrophysics covers topics such as Anisotropy which are related to areas like Tidal force.
His Galaxy study frequently links to related topics such as Observable.
His research investigates the connection between Dark energy and topics such as Cosmic microwave background that intersect with issues in Cosmology, Isotropy and Galaxy group.
As a part of the same scientific family, Cristiano Porciani mostly works in the field of Field, focusing on Dark matter and, on occasion, Halo, Density contrast and Structure formation.
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