Zobrazeno 1 - 10
of 37
pro vyhledávání: '"R. Serafinelli"'
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
Autor:
R. Della Ceca, G. Giani, R. Middei, Enrico Piconcelli, P. Severgnini, Francesco Tombesi, F. G. Saturni, A. Tortosa, Valentina Braito, R. Serafinelli, Massimo Gaspari, F. Vagnetti
Photoionized absorbers of outflowing gas are commonly found in the X-ray spectra of active galactic nuclei (AGN). While most of these absorbers are seldom significantly variable, some ionized obscurers have been increasingly found to substantially ch
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fa9a036392099d8afacece5950eba17e
http://arxiv.org/abs/2107.06584
http://arxiv.org/abs/2107.06584
Autor:
Maila Agostini, Marta Civitani, Marica Branchesi, Paola Severgnini, Costanzo Federico, Mauro Focardi, Giovanni Pareschi, Ashish Sharma, Stefano Covino, Alessandro Bertolini, Roberto Della Ceca, Christophe Collette, Marco Pallavicini, Nandita Khetan, Lorella Angelini, Jan Harms, Claudio Pernechele, Ho Jung Paik, Gianpiero Tagliaferri, F. Badaracco, Alessandro Pajewski, Aniello Grado, R. Serafinelli, Lorenzo Betti, Matteo Di Giovanni, Massimo Della Valle, Raffaele Votta, S. Ronchini, Luca Izzo, Joris van Heijningen, Andrea Possenti, E. Coccia, Carlo Giunchi, Gor Oganesyan, Giorgio Spada, Vladimiro Noce, Simone Dall'Osso, Riccardo Pozzobon, Marco Olivieri, Alessandro Frigeri, C. M. Mow-Lowry, Riccardo DeSalvo, Daniele Melini, Augusto Marcelli, Michael W. Coughlin, Enzo Brocato, Enrico Cappellaro, Emanuele Pace, Michelangelo Formisano, Ruggero Stanga, Giuseppe Mitri, Filippo Ambrosino, Andrea Maselli, Luca Naponiello, Cesare Dionisio, Valentina Braito, P. D'Avanzo, Eliana Palazzi
Publikováno v:
Harms, J, Ambrosino, F, Angelini, L, Braito, V, Branchesi, M, Brocato, E, Cappellaro, E, Coccia, E, Coughlin, M, Ceca, R D, Valle, M D, Dionisio, C, Federico, C, Formisano, M, Frigeri, A, Grado, A, Izzo, L, Marcelli, A, Maselli, A, Olivieri, M, Pernechele, C, Possenti, A, Ronchini, S, Serafinelli, R, Severgnini, P, Agostini, M, Badaracco, F, Bertolini, A, Betti, L, Civitani, M M, Collette, C, Covino, S, Dall'Osso, S, D'Avanzo, P, Desalvo, R, Giovanni, M D, Focardi, M, Giunchi, C, Heijningen, J V, Khetan, N, Melini, D, Mitri, G, Mow-Lowry, C, Naponiello, L, Noce, V, Oganesyan, G, Pace, E, Paik, H J, Pajewski, A, Palazzi, E, Pallavicini, M, Pareschi, G, Pozzobon, R, Sharma, A, Spada, G, Stanga, R, Tagliaferri, G & Votta, R 2021, ' Lunar Gravitational-wave Antenna ', Astrophysical Journal, vol. 910, no. 1, 1, pp. 1-22 . https://doi.org/10.3847/1538-4357/abe5a7
Astrophysical Journal, 910(1):1, 1-22. IOP Publishing Ltd.
Astrophysical Journal, 910(1):1, 1-22. IOP Publishing Ltd.
Monitoring of vibrational eigenmodes of an elastic body excited by gravitational waves was one of the first concepts proposed for the detection of gravitational waves. At laboratory scale, these experiments became known as resonant-bar detectors firs
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f5cc178cbfb3534d4303fcd7d69ff7c6
https://hdl.handle.net/1871.1/fa1a0d79-960e-4fac-94af-e8ce49750ed7
https://hdl.handle.net/1871.1/fa1a0d79-960e-4fac-94af-e8ce49750ed7
Autor:
Marco Landoni, D. Paris, Cristian Vignali, P. Severgnini, C. Cicone, Lucía Ballo, Valentina Braito, Felice Cusano, Paolo Saracco, R. Della Ceca, A. Zaino, R. Serafinelli, G. Pruto, Massimo Dotti
Although thousands of galaxy mergers are known, only a handful of sub-kiloparsec-scale supermassive black hole (SMBH) pairs have been confirmed so far, leaving a huge gap between the observed and predicted numbers of such objects. In this work, we pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e42cab61746ba0e6432c6830b7145b30
http://hdl.handle.net/20.500.12386/32257
http://hdl.handle.net/20.500.12386/32257
Autor:
G. A. Matzeu, A. Zaino, A. Marinucci, R. Serafinelli, Giovanni Miniutti, Francesco Tombesi, Francesco Ursini, Stefano Bianchi, Fausto Vagnetti, P.-O. Petrucci, R. Middei
Publikováno v:
DIGITAL.INTA Repositorio Digital del Instituto Nacional de Técnica Aeroespacial
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A18. ⟨10.1051/0004-6361/201936701⟩
Astron.Astrophys.
Astron.Astrophys., 2020, 635, pp.A18. ⟨10.1051/0004-6361/201936701⟩
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
instname
Astronomy and Astrophysics-A&A
Astronomy and Astrophysics-A&A, EDP Sciences, 2020, 635, pp.A18. ⟨10.1051/0004-6361/201936701⟩
Astron.Astrophys.
Astron.Astrophys., 2020, 635, pp.A18. ⟨10.1051/0004-6361/201936701⟩
Instituto Nacional de Técnica Aeroespacial (INTA)
Digital.CSIC. Repositorio Institucional del CSIC
The soft X-ray band of many active galactic nuclei (AGNs) is affected by obscuration due to partially ionised matter crossing our line of sight. In this context, two past XMM-Newton observations (6 months apart) and a simultaneous NuSTAR-Swift ($\sim
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::42ab72028029315e1d1dda28f686c44a
http://arxiv.org/abs/2001.03979
http://arxiv.org/abs/2001.03979
Autor:
Valentina La Parola, Lucía Ballo, Paola Severgnini, Alberto Sesana, G. Matzeu, R. Serafinelli, C. Cicone, Valentina Braito, A. Zaino, Filippo Ambrosino, Vittoria E. Gianolli, Massimo Dotti, Cristian Vignali, Roberto Della Ceca
Publikováno v:
The Astrophysical Journal
Elusive supermassive black hole binaries (SMBHBs) are thought to be the penultimate stage of galaxy mergers, preceding a final coalescence phase. SMBHBs are sources of continuous gravitational waves, possibly detectable by pulsar timing arrays; the i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::fb83a17ea09b228af4e3213c101fed22
http://hdl.handle.net/20.500.12386/31338
http://hdl.handle.net/20.500.12386/31338
Autor:
Mattia Sirressi, C. Cicone, J. N. Reeves, Lucía Ballo, Valentina Braito, Paola Severgnini, G. Matzeu, R. Serafinelli, R. Della Ceca
Past Suzaku, XMM and NuSTAR observations of the nearby (z=0.0323) bright Seyfert 2 galaxy MCG-03-58-007 revealed the presence of two deep and blue-shifted Fe K-shell absorption line profiles. These could be explained with the presence of two phases o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::48fc92e5db4d58968631a86fba73e1af
http://hdl.handle.net/10852/81946
http://hdl.handle.net/10852/81946
Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.
The study of the brightest cluster galaxy (BCG) coronae embedded in noncool core (NCC) galaxy clusters is crucial to understand the BCG's role in galaxy cluster evolution as well as the activation of the self-regulated cooling and heating mechanism i
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a08deb4bf396c271cc75ebfb78212b25
http://hdl.handle.net/20.500.12386/29256
http://hdl.handle.net/20.500.12386/29256