C. M. Raiteri focuses on Astrophysics, Blazar, Astronomy, Light curve and Gamma ray. His work in Astrophysics addresses subjects such as Spectral line, which are connected to disciplines such as Synchrotron. His biological study spans a wide range of topics, including Luminosity and Galaxy.
His research in Astronomy focuses on subjects like Fermi Gamma-ray Space Telescope, which are connected to Black hole. In his work, Line and Doppler effect is strongly intertwined with Brightness, which is a subfield of Light curve. The various areas that C. M. Raiteri examines in his Spectral energy distribution study include Emission spectrum and MAGIC.
His scientific interests lie mostly in Astrophysics, Blazar, Astronomy, Light curve and Quasar. Gamma ray, BL Lac object, Telescope, Active galactic nucleus and Flare are the subjects of his Astrophysics studies. His Telescope research includes themes of Observatory and Satellite.
His Blazar study also includes fields such as
C. M. Raiteri spends much of his time researching Astrophysics, Blazar, Astronomy, Light curve and Telescope. His is doing research in MAGIC, BL Lac object, Spectral energy distribution, Gamma ray and Flare, both of which are found in Astrophysics. The study incorporates disciplines such as Swift and X-ray in addition to Gamma ray.
His study looks at the intersection of Blazar and topics like Active galactic nucleus with Radio spectrum. His research in the fields of Radio galaxy and Elliptical galaxy overlaps with other disciplines such as Context. His studies deal with areas such as Exoplanet and Swift Gamma-Ray Burst Mission as well as Telescope.
C. M. Raiteri mainly focuses on Astrophysics, Blazar, Astronomy, Spectral energy distribution and MAGIC. His research in Astrophysics intersects with topics in Spectral line and Synchrotron. His Blazar research is multidisciplinary, relying on both Brightness, Fermi Gamma-ray Space Telescope, Quasar, Photometry and Light curve.
His study in Active galactic nucleus and Observatory falls under the purview of Astronomy. His Spectral energy distribution research includes elements of Flare, Radio telescope and Optical polarization. C. M. Raiteri has researched MAGIC in several fields, including Crab Nebula, Cherenkov radiation and Astroparticle physics.
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.
THE SPECTRAL ENERGY DISTRIBUTION OF FERMI BRIGHT BLAZARS
A. A. Abdo;A. A. Abdo;M. Ackermann;I. Agudo;M. Ajello.
The Astrophysical Journal (2010)
Radiative C-13 burning in asymptotic giant branch stars and s-processing
O. Straniero;R. Gallino;M. Busso;A. Chiefei.
The Astrophysical Journal (1995)
Fermi Large Area Telescope Observations of Markarian 421: The Missing Piece of its Spectral Energy Distribution
A. A. Abdo;A. A. Abdo;M. Ackermann;M. Ajello;L. Baldini.
The Astrophysical Journal (2011)
Multiwavelength Observations of a Dramatic High-Energy Flare in the Blazar 3C 279
A. E. Wehrle;E. Pian;C. M. Urry;L. Maraschi.
The Astrophysical Journal (1998)
Insights into the high-energy γ-ray emission of Markarian 501 from extensive multifrequency observations in the Fermi era
A. A. Abdo;A. A. Abdo;Markus Ackermann;Marco Ajello;A. Allafort.
The Astrophysical Journal (2011)
The Weak s-Component and Nucleosynthesis in Massive Stars
C. M. Raiteri;R. Gallino;M. Busso;D. Neuberger.
The Astrophysical Journal (1993)
The structure and emission model of the relativistic jet in the quasar 3C 279 inferred from radio to high-energy gamma-ray observations in 2008-2010
M. Hayashida;G. M. Madejski;K. Nalewajko;M. Sikora.
arXiv: High Energy Astrophysical Phenomena (2012)
Optical and radio variability of the BL Lac object AO 0235+16: a possible 5-6 year periodicity
C.M. Raiteri;M. Villata;H.D. Aller;M.F. Aller.
arXiv: Astrophysics (2001)
S-Process Nucleosynthesis: Classical Approach and Asymptotic Giant Branch Models for Low-Mass Stars
F. Kaeppeler;R. Gallino;M. Busso;G. Picchio.
The Astrophysical Journal (1990)
Optical and radio variability of the BL Lacertae object AO 0235+16: A possible 5-6 year periodicity
C. M Raiteri;M Villata;H. D Aller;M. F Aller.
Astronomy and Astrophysics (2001)
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