Zobrazeno 1 - 10
of 36
pro vyhledávání: '"Brügge, Kai"'
Autor:
Donath, Axel, Terrier, Régis, Remy, Quentin, Sinha, Atreyee, Nigro, Cosimo, Pintore, Fabio, Khélifi, Bruno, Olivera-Nieto, Laura, Ruiz, Jose Enrique, Brügge, Kai, Linhoff, Maximilian, Contreras, Jose Luis, Acero, Fabio, Aguasca-Cabot, Arnau, Berge, David, Bhattacharjee, Pooja, Buchner, Johannes, Boisson, Catherine, Fidalgo, David Carreto, Chen, Andrew, de Lavergne, Mathieu de Bony, Cardoso, José Vinícius de Miranda, Deil, Christoph, Füßling, Matthias, Funk, Stefan, Giunti, Luca, Hinton, Jim, Jouvin, Léa, King, Johannes, Lefaucheur, Julien, Lemoine-Goumard, Marianne, Lenain, Jean-Philippe, López-Coto, Rubén, Mohrmann, Lars, Morcuende, Daniel, Panny, Sebastian, Regeard, Maxime, Saha, Lab, Siejkowski, Hubert, Siemiginowska, Aneta, Sipőcz, Brigitta M., Unbehaun, Tim, van Eldik, Christopher, Vuillaume, Thomas, Zanin, Roberta
Publikováno v:
A&A 678, A157 (2023)
In this article, we present Gammapy, an open-source Python package for the analysis of astronomical $\gamma$-ray data, and illustrate the functionalities of its first long-term-support release, version 1.0. Built on the modern Python scientific ecosy
Externí odkaz:
http://arxiv.org/abs/2308.13584
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
The Metropolis algorithm is arguably the most fundamental Markov chain Monte Carlo (MCMC) method. But the algorithm is not guaranteed to converge to the desired distribution in the case of multivariate binary distributions (e.g., Ising models or stoc
Externí odkaz:
http://arxiv.org/abs/2006.14999
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, 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
Once completed, the Cherenkov Telescope Array (CTA) will be able to map the gamma-ray sky in a wide energy range from several tens of GeV to some hundreds of TeV and will be more sensitive than previous experiments by an order of magnitude. It opens
Externí odkaz:
http://arxiv.org/abs/1809.00581
Autor:
Dorner, Daniela, Lauer, Robert J., Adam, Jan, Ahnen, Max, Baack, Dominik, Balbo, Matteo, Bergmann, Matthias, Biland, Adrian, Blank, Michael, Bretz, Thomas, Brügge, Kai, Buss, Jens, Dmytiiev, Anton, Einecke, Sabrina, Hempfling, Christina, Hildebrand, Dorothee, Hughes, Gareth, Linhoff, Lena, Mannheim, Karl, Müller, Sebastian, Neise, Dominik, Neronov, Andrii, Noethe, Maximilian, Paravac, Aleksander, Pauss, Felicitas, Rhode, Wolfgang, Shukla, Amit, Temme, Fabian, Thaele, Julia, Walter, Roland
For studying variable sources like blazars, it is crucial to achieve unbiased monitoring, either with dedicated telescopes in pointing mode or survey instruments. At TeV energies, the High Altitude Water Cherenkov (HAWC) observatory monitors approxim
Externí odkaz:
http://arxiv.org/abs/1610.06627
Autor:
Deil, Christoph, Boisson, Catherine, Kosack, Karl, Perkins, Jeremy, King, Johannes, Eger, Peter, Mayer, Michael, Wood, Matthew, Zabalza, Victor, Knödlseder, Jürgen, Hassan, Tarek, Mohrmann, Lars, Ziegler, Alexander, Khelifi, Bruno, Dorner, Daniela, Maier, Gernot, Pedaletti, Giovanna, Rosado, Jaime, Contreras, José Luis, Lefaucheur, Julien, Brügge, Kai, Servillat, Mathieu, Terrier, Régis, Walter, Roland, Lombardi, Saverio
In gamma-ray astronomy, a variety of data formats and proprietary software have been traditionally used, often developed for one specific mission or experiment. Especially for ground-based imaging atmospheric Cherenkov telescopes (IACTs), data and so
Externí odkaz:
http://arxiv.org/abs/1610.01884
Publikováno v:
EPJ Web of Conferences, Vol 207, p 03002 (2019)
With very high energy (VHE) gamma-ray astronomy becoming a mature branch of observational astrophysics, and the multi-messenger sky being opened up by neutrino observatories and gravitational wave detectors, we here propose to set up a ring of imagin
Externí odkaz:
https://doaj.org/article/de19c285414545f0b37d5273645aa2e6
Publikováno v:
EPJ Web of Conferences, Vol 144, p 01004 (2017)
Atmospheric monitoring is a field of special importance for astroparticle physics, especially for Imaging Atmospheric Cherenkov Telescopes (IACTs) as clouds will absorb and scatter the Cherenkov photons of air showers. Conventional tools used for atm
Externí odkaz:
https://doaj.org/article/a3e2d199dc454609914fc2910c3d98cd