His primary areas of study are Astrophysics, Astronomy, Gamma ray, Blazar and Synchrotron. His research integrates issues of Spectral line and Photon in his study of Astrophysics. He is interested in Spectral energy distribution, which is a field of Astronomy.
His Gamma ray research incorporates elements of Galaxy, Telescope and Emission spectrum. His Blazar study incorporates themes from Relativistic plasma, Sky and Relativistic beaming. His work in Synchrotron covers topics such as Electron which are related to areas like Observatory.
L. Maraschi spends much of his time researching Astrophysics, Astronomy, Blazar, Gamma ray and Spectral line. L. Maraschi conducts interdisciplinary study in the fields of Astrophysics and Flux through his works. The Active galactic nucleus, Spectral energy distribution and Ultraviolet astronomy research L. Maraschi does as part of his general Astronomy study is frequently linked to other disciplines of science, such as Power law, therefore creating a link between diverse domains of science.
His study in Blazar is interdisciplinary in nature, drawing from both ROSAT, Amplitude, Fermi Gamma-ray Space Telescope, Luminosity and Synchrotron. His study explores the link between Synchrotron and topics such as Photon that cross with problems in Cosmic microwave background. He has researched Light curve in several fields, including Flare and X-ray astronomy.
The scientist’s investigation covers issues in Astrophysics, Blazar, Gamma ray, Fermi Gamma-ray Space Telescope and Astronomy. His study in MAGIC, Quasar, Telescope, Flare and Active galactic nucleus falls under the purview of Astrophysics. In his work, Extragalactic background light is strongly intertwined with Crab Nebula, which is a subfield of MAGIC.
In Blazar, L. Maraschi works on issues like Photon, which are connected to Synchrotron. He has included themes like X-ray, Spectral line, Galaxy and Black hole in his Gamma ray study. The concepts of his Fermi Gamma-ray Space Telescope study are interwoven with issues in Spectral energy distribution and Spitzer Space Telescope.
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 jet model for the gamma-ray emitting blazar 3C 279
L. Maraschi;G. Ghisellini;A. Celotti.
The Astrophysical Journal (1992)
Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey
M. Polletta;M. Tajer;L. Maraschi;G. Trinchieri.
arXiv: Astrophysics (2007)
Relativistic bulk motion in active galactic nuclei
G. Ghisellini;P. Padovani;A. Celotti;L. Maraschi.
The Astrophysical Journal (1993)
Very-High-Energy Gamma Rays from a Distant Quasar: How Transparent Is the Universe?
J Albert;E Aliu;H Anderhub.
Science (2008)
MAGIC discovery of VHE Emission from the FSRQ PKS 1222+21
J. Aleksić;L. Antonelli;P. Antoranz;M. Backes.
arXiv: High Energy Astrophysical Phenomena (2011)
Radio-Loud Narrow-Line Seyfert 1 as a New Class of Gamma-Ray AGN
G. Ghisellini;L. Maraschi.
arXiv: High Energy Astrophysical Phenomena (2009)
The power of relativistic jets is larger than the luminosity of their accretion disks
G. Ghisellini;F. Tavecchio;L. Maraschi;A. Celotti.
Nature (2014)
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)
Radio Imaging of the Very-High-Energy gamma-Ray Emission Region in the Central Engine of a Radio Galaxy
V.A. Acciari;E. Aliu;T. Arlen;M. Bautista.
Science (2009)
Multiwavelength Observations of a Dramatic High Energy Flare in the Blazar 3C 279
A. E. Wehrle;E. Pian;C. M. Urry;L. Maraschi.
arXiv: Astrophysics (1997)
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