Zobrazeno 1 - 10
of 83
pro vyhledávání: '"L. Marcotulli"'
Autor:
P. G. Boorman, N. Torres-Albà, A. Annuar, S. Marchesi, R. W. Pfeifle, D. Stern, F. Civano, M. Baloković, J. Buchner, C. Ricci, D. M. Alexander, W. N. Brandt, M. Brightman, C. T. Chen, S. Creech, P. Gandhi, J. A. García, F. Harrison, R. Hickox, E. Kammoun, S. LaMassa, G. Lanzuisi, L. Marcotulli, K. Madsen, G. Matt, G. Matzeu, E. Nardini, J. M. Piotrowska, A. Pizzetti, S. Puccetti, D. Sicilian, R. Silver, D. J. Walton, D. R. Wilkins, X. Zhao, The HEX-P Collaboration
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 11 (2024)
Ever since the discovery of the first active galactic nuclei (AGN), substantial observational and theoretical effort has been invested into understanding how massive black holes have evolved across cosmic time. Circum-nuclear obscuration is now estab
Externí odkaz:
https://doaj.org/article/06e8a41e09e4449b99d01c68c15ce62e
Publikováno v:
The Astrophysical Journal, Vol 965, Iss 2, p 112 (2024)
Active galactic nuclei (AGNs) can power relativistic jets, which are called blazars when pointed close to our line of sight. Depending on the presence or absence of emission lines in their optical spectra, blazars are categorized into flat spectrum r
Externí odkaz:
https://doaj.org/article/da0b419f1b124631b79cb699d4ab5b52
Publikováno v:
The Astronomical Journal, Vol 165, Iss 2, p 42 (2023)
Active galactic nuclei with their relativistic jets pointed toward the observer are a class of luminous gamma-ray sources commonly known as blazars. The study of this source class is essential to unveil the physical processes powering these extreme j
Externí odkaz:
https://doaj.org/article/bc559219361a45b49a9dbcb433231080
Akademický článek
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Akademický článek
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Akademický článek
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Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
The under-explored MeV band has an extremely rich scientific potential. Awaiting an all-sky MeV mission, it is now the prime time to take full advantage of the capabilities of the Fermi Large Area Telescope to explore this regime. With more than 12 y
Autor:
M. Razzano, Francesco Longo, J. Zrake, S. Buson, Junyao Li, A. Franckowiak, Elisabetta Bissaldi, Diego F. Torres, N. Di Lalla, Luca Baldini, Aaron Dominguez, M. E. Monzani, Sylvain Guiriec, Mn Mazziotta, C. Karwin, Alberto Manfreda, Bindu Rani, Denis Bastieri, Nicola Omodei, F. D'Ammando, G. Jóhannesson, P. M. Saz Parkinson, A. Desai, S. Marchesi, D. Costantin, Peter F. Michelson, Marcello Giroletti, M. Orienti, Marco Ajello, Damiano Caprioli, A. Berretta, Sina Chen, A. Reimer, Igor V. Moskalenko, Olaf Reimer, Carmelo Sgrò, Riccardo Rando, Miloš Kovačević, Z. Pei, A. Morselli, Melissa Pesce-Rollins, Rebecca Diesing, Stefan Larsson, J. L. Racusin, David Paneque, G. Chiaro, M. Kuss, Vaidehi S. Paliya, P. Spinelli, L. Marcotulli, T. A. Porter, G. Principe, S. Maldera, P. Fusco, G. Martí-Devesa, F. de Palma, Francesco Giordano, M. Negro, Dario Gasparrini, J. Ballet, Roger Blandford, I. Mereu, F. Loparco, Matthew Kerr, E. Orlando, S. J. Fegan, Dieter H. Hartmann, S. Cutini, David A. Green, Stefan Funk, D. Horan, George Chartas, Massimo Persic, Regina Caputo, Ronaldo Bellazzini, D. Serini, R. A. Cameron, Nicola Giglietto, P. Lubrano, I. A. Grenier, Guido Barbiellini, P. Bruel, D. Tak, M. N. Lovellette, Ioannis Liodakis, S. Rainò, Tsunefumi Mizuno, Yasushi Fukazawa, Gabrijela Zaharijas, K. S. Wood, E. Troja, Elliott D. Bloom, R. Bonino, E. J. Siskind, D. J. Suson, Luca Latronico, C. C. Cheung, P. de la Torre Luque, F. Gargano, E. Cavazzuti, Gloria Spandre, F. Dirirsa, L. Di Venere, M. Lemoine-Goumard
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astrophys.J.
Astrophys.J., 2021, 921 (2), pp.144. ⟨10.3847/1538-4357/ac1bb2⟩
Scopus-Elsevier
instname
Astrophys.J.
Astrophys.J., 2021, 921 (2), pp.144. ⟨10.3847/1538-4357/ac1bb2⟩
Scopus-Elsevier
Massive black holes at the centers of galaxies can launch powerful wide-angle winds that, if sustained over time, can unbind the gas from the stellar bulges of galaxies. These winds may be responsible for the observed scaling relation between the mas
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05e0e675ebe11462ff0a49cf5108cce4
http://hdl.handle.net/11589/236376
http://hdl.handle.net/11589/236376
With ten years of operation and an exceptional dataset, the Fermi-Large Area Telescope allows us to unveil the detailed composition of the extragalactic $\gamma$-ray sky above $\rm 100\,MeV$. In this paper, we derive the intrinsic source-count distri
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3097d4957ea74a982362d549f1cd0dec
http://arxiv.org/abs/2006.04703
http://arxiv.org/abs/2006.04703
Autor:
Vaidehi S. Paliya, Roopesh Ojha, Grzegorz Madejski, L. Marcotulli, Stefano Marchesi, Amanpreet Kaur, Dieter H. Hartmann, Marco Ajello, Dario Gasparrini, M. Rajagopal
Publikováno v:
The astrophysical journal / 2 889(2), 164 (2020). doi:10.3847/1538-4357/ab65f5
The astrophysical journal 889(2), 164 (2020). doi:10.3847/1538-4357/ab65f5
With bolometric luminosities exceeding $10^{48}$ erg s$^{-1}$, powerful jets and supermassive black holes at their center, MeV blazars are some of the most extreme source
With bolometric luminosities exceeding $10^{48}$ erg s$^{-1}$, powerful jets and supermassive black holes at their center, MeV blazars are some of the most extreme source
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d62bc2b01b94fb76375403ec4b6bf419
http://arxiv.org/abs/2001.01956
http://arxiv.org/abs/2001.01956