Zobrazeno 1 - 5
of 5
pro vyhledávání: '"von Willert, Elan"'
Autor:
Arbet-Engels, Axel, Baack, Dominik, Balbo, Matteo, Biland, Adrian, Blank, Michael, Bretz, Thomas, Bruegge, Kai, Bulinski, Michael, Buss, Jens, Doerr, Manuel, Dorner, Daniela, Elsaesser, Dominik, Hildebrand, Dorothee, Mannheim, Karl, Mueller, Sebastian, Neise, Dominik, Noethe, Maximilian, Paravac, Aleksander, Rhode, Wolfgang, Schleicher, Bernd, Sedlaczek, Kevin, Shukla, Amit, Sliusar, Vitalii, Walter, Roland, von Willert, Elan
Publikováno v:
A&A 647, A88 (2021)
The origin of the gamma-ray emission of the blazar Mrk 421 is still a matter of debate. We used 5.5 years of unbiased observing campaign data, obtained using the FACT telescope and the Fermi LAT detector at TeV and GeV energies, the longest and dense
Externí odkaz:
http://arxiv.org/abs/2101.10651
Autor:
Sliusar, Vitalii, Arbet-Engels, Axel, Baack, Dominik, Balbo, Matteo, Biland, Adrian, Blank, Michael, Bretz, Tomas, Bruegge, Kai, Bulinski, Michael, Buss, Jens, Doerr, Manuel, Dorner, Daniela, Elsaesser, Dominik, Hildebrand, Dorothee, Mannheim, Karl, mueller, Sebastian, Neise, Dominik, Noethe, Maximilian, Paravac, Aleksander, Rhode, Wolfgang, Schleicher, Bernd, Sedlaczek, Kevin, Shukla, Amit, Walter, Roland, von Willert, Elan
Publikováno v:
36th International Cosmic Ray Conference, Proceedings of Science 358 (2018) 796
Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use multi-wavelength light curves of Mrk 421 spanning 5.5 years with FACT (TeV) and Fermi LAT (GeV) in the gamma rays, Swift BAT, Swift XRT and MAXI
Externí odkaz:
http://arxiv.org/abs/1908.09770
Autor:
Sliusar, Vitalii, Arbet Engels, Axel, Baack, Dominik, Balbo, Matteo, Beck, Marvin, Biland, Adrian, Blank, Michael, Bretz, Tomas, Bruegge, Kai, Bulinski, Michael, Buss, Jens, Doerr, Manuel, Dorner, Daniela, Elsaesser, Dominik, Hildebrand, Dorothée, Iotov, Roman, Klinger, Marc, Mannheim, Karl, Mueller, Sebastian, Neise, Dominik, Noethe, Maximilian, Paravac, Aleksander, Rhode, Wolfgang, Schleicher, Bernd, Sedlaczek, Kevin, Shukla, Amit, Tani, Laurits, Theissen, Fabian, Walter, Roland, von Willert, Elan
Publikováno v:
PoS: Proceedings of Science, 358
Proceedings of th 36th International Cosmic Ray Conference (ICRC 2019)
Proceedings of th 36th International Cosmic Ray Conference (ICRC 2019)
Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use multi-wavelength light curves of Mrk 421 spanning 5.5 years with FACT (TeV) and Fermi LAT (GeV) in the gamma rays, Swift BAT, Swift XRT and MAXI
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0958268a1ae914772585c68b0cf7579f
https://hdl.handle.net/20.500.11850/549808
https://hdl.handle.net/20.500.11850/549808
Autor:
FACT Collaboration, Dorner, Daniela, Arbet-Engels, Axel, Baack, Dominik, Balbo, Matteo, Beck, Marvin, Biland, Adrian, Blank, Michael, Bretz, Thomas, Bruegge, Kai, Bulinski, Michael, Buss, Jens, Doerr, Manuel, Elsaesser, Dominik, Hildebrand, Dorothée, Iotov, Roman, Klinger, Marc, Mannheim, Karl, Neise, Dominik, Mueller, Sebastian A., Neronov, Andrii, Noethe, Maximilian, Paravac, Aleksander, Rhode, Wolfgang, Schleicher, Bernd, Sedlaczek, Kevin, Shukla, Amit, Sliusar, Vitalii, Tani, Laurits, Theissen, Fabian, Walter, Roland, von Willert, Elan
Publikováno v:
PoS: Proceedings of Science, 358
36th International Cosmic Ray Conference (ICRC 2019)-GRI-Gamma Ray Indirect
36th International Cosmic Ray Conference (ICRC 2019)-GRI-Gamma Ray Indirect
The First G-APD Cherenkov Telescope (FACT) has been monitoring TeV-blazars since October 2011. Thanks to its unbiased observing strategy, the robotic operation and the usage of solid state photosensors (SiPM, aka G-APDs), the instrument's duty cycle
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9dafdcd3b8e9d9a828051232f998b252
https://hdl.handle.net/20.500.11850/458974
https://hdl.handle.net/20.500.11850/458974
Autor:
Dorner, Daniela, Arbet-Engels, Axel, Baack, Dominik, Balbo, Matteo, Biland, Adrian, Blank, Michael, Bretz, Thomas, Bruegge, Kai, Bulinski, Michael, Buss, Jens, Doerr, Manuel, Elsaesser, Dominik, Hildebrand, Dorothée, Linhoff, Lena, Mannheim, Karl, Mueller, Sebastian A., Neise, Dominik, Neronov, Andrii, Noethe, Maximilian, Paravac, Aleksander, Rhode, Wolfgang, Schleicher, Bernd, Schulz, Florian, Sedlaczek, Kevin, Shukla, Amit, Sliusar, Vitalii, von Willert, Elan, Walter, Roland, FACT Collaboration
Publikováno v:
Galaxies, 7 (2)
Galaxies, Vol 7, Iss 2, p 57 (2019)
Galaxies : open access journal 7(2), 57 (2019). doi:10.3390/galaxies7020057
Galaxies, Vol. 7, No 2 (2019) P. 57
Galaxies
Volume 7
Issue 2
Galaxies, Vol 7, Iss 2, p 57 (2019)
Galaxies : open access journal 7(2), 57 (2019). doi:10.3390/galaxies7020057
Galaxies, Vol. 7, No 2 (2019) P. 57
Galaxies
Volume 7
Issue 2
Blazars are known to show variability on time scales from minutes to years covering a wide range of flux states. Studying the flux distribution of a source allows for various insights. The shape of the flux distribution can provide information on the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::74b7e39ab2e3497e61f055b334352b3e