Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Theissen, Fabian"'
Autor:
Sliusar, Vitalii, Arbet-Engels, Axel, Baack, Dominik, Balbo, Matteo, Beck, Marvin, Biland, Adrian, Blank, Michael, Bretz, Thomas, Bruegge, Kai, Bulinski, Michael, Buss, Jens, Doerr, Manuel, Dorner, Daniela, Elsaesser, Dominik, Hildebrand, Dorothee, Iotov, Roman, Klinger, Marc, Mannheim, Karl, Neise, Dominik, Noethe, Maximilian, Paravac, Aleksander, Rhode, Wolfgang, Schleicher, Bernd, Sedlaczek, Kevin, Shukla, Amit, Tani, Laurits, Theissen, Fabian, Walter, Roland
Publikováno v:
Proceedings of Science HEPRO VII, PoS(HEPRO VII) (2019) 032
Mrk 421 is a high-synchrotron-peaked blazar featuring bright and persistent GeV and TeV emission. We use the longest and densest ongoing unbiased observing campaign obtained at TeV and GeV energies during 5.5 years with the FACT telescope and the Fer
Externí odkaz:
http://arxiv.org/abs/1909.13106
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