His primary areas of investigation include Astrophysics, Astronomy, Galaxy, Redshift and Active galactic nucleus. His study in Luminosity, Black hole, Quasar, Halo and Supermassive black hole are all subfields of Astrophysics. As part of his studies on Astronomy, he often connects relevant subjects like Particle physics.
His work investigates the relationship between Redshift and topics such as Extinction that intersect with problems in Spectral line and Luminosity function. In his research on the topic of Active galactic nucleus, Interacting galaxy is strongly related with Radio galaxy. Francesco Shankar studied Galaxy formation and evolution and Velocity dispersion that intersect with Spiral galaxy.
Francesco Shankar mainly investigates Astrophysics, Galaxy, Astronomy, Redshift and Stellar mass. His is involved in several facets of Astrophysics study, as is seen by his studies on Active galactic nucleus, Quasar, Galaxy formation and evolution, Luminosity and Halo. His studies deal with areas such as Black hole and Dark matter as well as Galaxy.
His Redshift study combines topics from a wide range of disciplines, such as Mass relation, Cosmos, Universe and Sigma. He has included themes like Stellar population, Initial mass function, Effective radius and Velocity dispersion in his Stellar mass study. His research investigates the link between Supermassive black hole and topics such as Binary black hole that cross with problems in Stellar black hole.
His main research concerns Astrophysics, Galaxy, Stellar mass, Active galactic nucleus and Redshift. Star formation, Accretion, Luminosity, Dark matter and Fundamental plane are the core of his Astrophysics study. His Supermassive black hole, Galaxy formation and evolution and Bulge study in the realm of Galaxy interacts with subjects such as Scaling.
His research integrates issues of Halo, Dark matter halo, Initial mass function and Velocity dispersion in his study of Stellar mass. His Active galactic nucleus research focuses on Light curve and how it relates to Quasar. His Redshift study is associated with Astronomy.
His primary areas of study are Astrophysics, Galaxy, Stellar mass, Redshift and Active galactic nucleus. His studies in Accretion, Virial theorem, Black hole, Halo and Dark matter halo are all subfields of Astrophysics research. His study on Satellite galaxy is often connected to Continuity equation as part of broader study in Halo.
His study in Fundamental plane and Galaxy formation and evolution is done as part of Galaxy. The study incorporates disciplines such as Supermassive black hole and Velocity dispersion in addition to Stellar mass. His work is dedicated to discovering how Redshift, Order of magnitude are connected with Accretion and other disciplines.
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.
A Physical Model for Co-evolution of QSOs and of their Spheroidal Hosts
G. De Zotti;F. Shankar;A. Lapi;G. L. Granato.
arXiv: Astrophysics (2006)
A White Paper on keV sterile neutrino Dark Matter
R. Adhikari;M. Agostini;N. Anh Ky;N. Anh Ky;T. Araki.
Journal of Cosmology and Astroparticle Physics (2017)
The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
Kirpal Nandra;Didier Barret;Xavier Barcons;Andy Fabian.
arXiv: High Energy Astrophysical Phenomena (2013)
Super-massive Black Hole Demography: the Match between the Local and Accreted Mass Functions
F. Shankar;P. Salucci;G. L. Granato;G. L. Granato;G. De Zotti;G. De Zotti.
arXiv: Astrophysics (2004)
SELF-CONSISTENT MODELS OF THE AGN AND BLACK HOLE POPULATIONS: DUTY CYCLES, ACCRETION RATES, AND THE MEAN RADIATIVE EFFICIENCY
Francesco Shankar;David H. Weinberg;Jordi Miralda-Escudé.
The Astrophysical Journal (2009)
Bolometric luminosities and Eddington ratios of X-ray selected active galactic nuclei in the XMM-COSMOS survey
E. Lusso;A. Comastri;B. D. Simmons;M. Mignoli.
Monthly Notices of the Royal Astronomical Society (2012)
Supermassive black hole demography: the match between the local and accreted mass functions
F. Shankar;P. Salucci;G. L. Granato;G. L. Granato;G. De Zotti;G. De Zotti.
Monthly Notices of the Royal Astronomical Society (2004)
AGN wind scaling relations and the co-evolution of black holes and galaxies
F. Fiore;C. Feruglio;F. Shankar;M. Bischetti.
Astronomy and Astrophysics (2017)
Black Hole growth and AGN obscuration by instability-driven inflows in high-redshift disk galaxies fed by cold streams
Frederic Bournaud;Avishai Dekel;Romain Teyssier;Marcello Cacciato.
arXiv: Cosmology and Nongalactic Astrophysics (2011)
Accreting SMBHs in the COSMOS field and the connection to their host galaxies
A. Bongiorno;A. Merloni;M. Brusa;B. Magnelli.
arXiv: Cosmology and Nongalactic Astrophysics (2012)
If you think any of the details on this page are incorrect, let us know.
We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:
University of Pennsylvania
University of Pennsylvania
University of Bologna
Université Paris Cité
National Institute for Astrophysics
National Institute for Astrophysics
Harvard University
Max Planck Society
National Institute for Astrophysics
International School for Advanced Studies
Polytechnic University of Milan
Carnegie Mellon University
McGill University
National University of Distance Education
University of Salzburg
Polytechnique Montréal
University of Tokyo
Argonne National Laboratory
European Bioinformatics Institute
University of California, Los Angeles
University of South Carolina
Bernhard Nocht Institute for Tropical Medicine
University of California, San Diego
City Of Hope National Medical Center
Flinders University
New York University