University of Leicester
United Kingdom
C. Pagani spends much of his time researching Astrophysics, Astronomy, Gamma-ray burst, Afterglow and Swift Gamma-Ray Burst Mission. His Astrophysics research focuses on subjects like X-ray, which are linked to Flare. His Astronomy study incorporates themes from Gamma ray and Blazar.
His research integrates issues of Swift and Redshift in his study of Gamma-ray burst. His Afterglow research includes elements of Gravitational wave, Kilonova, Neutron star and Orbital plane. His Swift Gamma-Ray Burst Mission research focuses on Telescope and how it relates to Angular resolution, Field of view, Compact star and Solar mass.
His primary areas of investigation include Astrophysics, Swift, Gamma-ray burst, Afterglow and Astronomy. Astrophysics is frequently linked to X-ray in his study. His work carried out in the field of Swift brings together such families of science as Supergiant and LIGO.
His work on Swift Gamma-Ray Burst Mission as part of general Gamma-ray burst study is frequently linked to Flux, bridging the gap between disciplines. He incorporates Afterglow and Jet in his research. Many of his studies on Astronomy involve topics that are commonly interrelated, such as Gamma ray.
C. Pagani focuses on Astrophysics, Swift, LIGO, Gamma-ray burst and Astronomy. His work on Astrometry, Afterglow, Stars and Open cluster as part of general Astrophysics study is frequently connected to Context, therefore bridging the gap between diverse disciplines of science and establishing a new relationship between them. His Astrometry research incorporates themes from Large Magellanic Cloud, Parallax, Photometry, Proper motion and Data release.
His studies in Afterglow integrate themes in fields like Compact star, Neutron star, Solar mass, Orbital plane and Kilonova. His research investigates the connection between Stars and topics such as Galaxy that intersect with issues in Radial velocity. His works in Telescope and Gravitational wave are all subjects of inquiry into Astronomy.
His scientific interests lie mostly in Astrophysics, Astrometry, Astronomy, Stars and Photometry. C. Pagani undertakes multidisciplinary studies into Astrophysics and Context in his work. His Astrometry research is multidisciplinary, incorporating perspectives in Large Magellanic Cloud, Data release, Parallax and Proper motion.
C. Pagani has researched Astronomy in several fields, including Swift and Polarization. The study incorporates disciplines such as Gamma-ray burst, Light curve and Redshift, Isotropic energy in addition to Swift. His work in the fields of Stars, such as RR Lyrae variable, overlaps with other areas such as Population.
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.
Gaia Data Release 2. Summary of the contents and survey properties
A. G. A. Brown;A. Vallenari;T. Prusti.
Astronomy and Astrophysics (2018)
The Gaia mission
T. Prusti;J. H. J. de Bruijne;A. G. A. Brown.
Astronomy and Astrophysics (2016)
The Swift X-ray Telescope
David N. Burrows;J. E. Hill;J. A. Nousek;J. A. Kennea.
arXiv: Astrophysics (2005)
The Swift X-ray telescope
David N. Burrows;J. E. Hill;J. A. Nousek;J. A. Kennea.
web science (2005)
Gaia Data Release 1 Summary of the astrometric, photometric, and survey properties
A. G. A. Brown;A. Vallenari;T. Prusti.
Astronomy and Astrophysics (2016)
Methods and results of an automatic analysis of a complete sample of Swift-XRT observations of GRBs
P. A. Evans;A. P. Beardmore;K. L. Page;J. P. Osborne.
Monthly Notices of the Royal Astronomical Society (2009)
Gaia Data Release 2: Observational Hertzsprung-Russell diagrams
C. Babusiaux;F. van Leeuwen;M.A. Barstow.
arXiv: Solar and Stellar Astrophysics (2018)
THE SPECTRAL ENERGY DISTRIBUTION OF FERMI BRIGHT BLAZARS
A. A. Abdo;A. A. Abdo;M. Ackermann;I. Agudo;M. Ajello.
The Astrophysical Journal (2010)
Broadband observations of the naked-eye gamma-ray burst GRB 080319B
J. L. Racusin;S. V. Karpov;M. Sokolowski;J. Granot.
Nature (2008)
GRB 090423 at a redshift of z ≈ 8.1
R. Salvaterra;M. Della Valle;S. Campana;G. Chincarini;G. Chincarini.
Nature (2009)
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