Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Magic, For The Collaboration"'
Autor:
Eisenacher Glawion, Dorit, Sitarek, Julian, Mannheim, Karl, Colin, Pierre, Magic, For The Collaboration, Matthias Kadler, Schulz, Robert, Ros, Eduardo, Bach, Uwe, Krauß, Felicia, Wilms, Jörn
Publikováno v:
arXiv.org e-Print Archive
NASA Astrophysics Data System
NASA Astrophysics Data System
The nearby active galaxy IC 310, located in the outskirts of the Perseus cluster of galaxies is a bright and variable multi-wavelength emitter from the radio regime up to very high gamma-ray energies above 100 GeV. Originally, the nucleus of IC 310 h
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::11088640ac05008d600868018fde100b
http://arxiv.org/abs/1508.05031
http://arxiv.org/abs/1508.05031
Autor:
Garrido, Daniel, Gaug, Markus, Michele Doro, Font, Lluís, López-Oramas, Alicia, Moralejo, Abelardo, Magic, For The Collaboration
Publikováno v:
arXiv.org e-Print Archive
NASA Astrophysics Data System
NASA Astrophysics Data System
We investigate the performance of the MAGIC telescopes under three simulated atmospheric conditions: an increased aerosol content in the lower part of the troposphere, the presence of thin aerosol over-densities at different heights, and an extremely
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::04e297f6f8ad2cdea5dbadd8bd8eb062
http://arxiv.org/abs/1308.0473
http://arxiv.org/abs/1308.0473
Autor:
Lombardi, Saverio, Lindfors, Elina, Becerra Gonzalez, Josefa, Colin, Pierre, Sitarek, Julian, Antonio Stamerra, Magic, For The Collaboration
Publikováno v:
arXiv.org e-Print Archive
NASA Astrophysics Data System
NASA Astrophysics Data System
The two BL Lac objects, 1ES 1215+303 and 1ES 1218+304, separated by 0.8 degree, were observed with the MAGIC Cherenkov telescopes in 2010-2011. The January 2011 observations resulted in the first detection above 100 GeV of 1ES 1215+303 (known also as
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::fc1496f0c9091caf50c44cac49a8e428
http://arxiv.org/abs/1110.6786
http://arxiv.org/abs/1110.6786
Autor:
Elisa Prandini, Tavecchio, F., Magic, For The Collaboration, Buson, S., Larsson, S., Lat, For The Fermi Collaboration
Publikováno v:
arXiv.org e-Print Archive
NASA Astrophysics Data System
NASA Astrophysics Data System
We present the results of five years (2005-2009) of MAGIC observations of the BL Lac object PG 1553+113 at very high energies (VHEs). Adding the new data set (2007-2009) to previous observations, this source becomes one of the best long-term followed
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::6859a47a0aff858f6ea3509ccce4c0a6
http://arxiv.org/abs/1110.6780
http://arxiv.org/abs/1110.6780
Autor:
Rügamer, S., Angelakis, E., Bastieri, D., Dorner, D., Fuhrmann, L., Kovalev, Yu A., Kovalev, Y. Y., Lähteenmäki, A., Lindfors, E., Longo, F., Lucarelli, F., Pittori, C., Reinthal, R., Sbarra, C., Sokolovsky, K., Antonio Stamerra, Ungerechts, H., Magic, For The Collaboration, F-Gamma Program, The, Fermi-Lat, The, RATAN, MOJAVE, AGILE, Iram, Teams
Publikováno v:
arXiv.org e-Print Archive
NASA Astrophysics Data System
NASA Astrophysics Data System
Simultaneous multi-wavelength (MW) campaigns are the most promising approaches to investigate the still unrevealed nature of blazars, active galactic nuclei which are variable on all time scales from radio to TeV energies. In 2008, two MW campaigns o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::db7b45e2450b56f93a70a741c833034e
http://arxiv.org/abs/1109.6808
http://arxiv.org/abs/1109.6808
Autor:
Elisa Prandini, Dorner, Daniela, Mankuzhiyil, Nijil, Mariotti, Mosè, Mazin, Daniel, Magic, For The Collaboration
Publikováno v:
arXiv.org e-Print Archive
NASA Astrophysics Data System
NASA Astrophysics Data System
Very high energy gamma ray emission from the active galactic nucleus PG 1553+113 was observed during 2005 and 2006 by the MAGIC collaboration, for a total observation time of 18.8 hours. Here we present the results of follow up observations: more tha
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::2186468e34eaae55e2fbdea83ea775d9
http://arxiv.org/abs/0907.0157
http://arxiv.org/abs/0907.0157
Autor:
Elisa Prandini, Pedaletti, G., Da Vela, P., Ona Wilhelmi, E., Colin, P., Fruck, C., Strzys, M., Vovk, Ie, Magic, For The Collaboration
Publikováno v:
Università degli Studi di Padova-IRIS
arXiv.org e-Print Archive
NASA Astrophysics Data System
arXiv.org e-Print Archive
NASA Astrophysics Data System
The MAGIC telescopes are an array of two imaging atmospheric Cherenkov telescopes (IACTs) studying the gamma ray sky at very high-energies (VHE; E>100 GeV). The observations are performed in stereoscopic mode, with both telescopes pointing at the sam
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::3a95541af1f6e922e583b2ee8b69d644
https://www.research.unipd.it/handle/11577/3260154
https://www.research.unipd.it/handle/11577/3260154
Autor:
Sitarek, J., Eisenacher Glawion, D., Mannheim, K., Colin, P., Magic, For The Collaboration, Kadler, M., Schultz, R., Krauß, F., Ros, E., Bach, U., Joern Wilms
Publikováno v:
NASA Astrophysics Data System
arXiv.org e-Print Archive
arXiv.org e-Print Archive
IC 310 has recently been identified as a gamma-ray emitter based on observations at GeV energies with Fermi-LAT and at very high energies (VHE, E > 100 GeV) with the MAGIC telescopes. Despite IC 310 having been classified as a radio galaxy with the j
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::26e3fe70fde935c4df24e9f2d22ea01c
https://ui.adsabs.harvard.edu/#abs/2015arXiv150201126S
https://ui.adsabs.harvard.edu/#abs/2015arXiv150201126S
Autor:
Becerra-González, J., Stamerra, A., Saito, K., Mazin, D., Tavecchio, F., Maraschi, L., Elisa Prandini, Sitarek, J., Berger, K., Magic, For The Collaboration
Publikováno v:
NASA Astrophysics Data System
arXiv.org e-Print Archive
arXiv.org e-Print Archive
The MAGIC telescopes discovered very high energy (VHE, E>100 GeV) gamma-ray emission coming from the distant Flat Spectrum Radio Quasar (FSRQ) PKS 1222+21 (4C +21.35, z=0.432). It is the second most distant VHE gamma-ray source, with well measured re
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::1fc0ac96430a156ded8d03d1e3b840d3
https://ui.adsabs.harvard.edu/#abs/2011arXiv1109.6446B
https://ui.adsabs.harvard.edu/#abs/2011arXiv1109.6446B
Autor:
Gaug, Markus, Covino, Stefano, Garczarczyk, Markus, Lucio Angelo Antonelli, Bastieri, Denis, La Barbera, Antonio, Becerra-Gonzalez, Josefa, Carosi, Alessandro, Galante, Nicola, Longo, Francesco, Scapin, Valeria, Spiro, Susanna, Magic, For The Collaboration
Publikováno v:
NASA Astrophysics Data System
arXiv.org e-Print Archive
arXiv.org e-Print Archive
On January 2, the MAGIC-I Telescope observed GRB090102 (z=1.55) under particularly good observation conditions. Using the recently upgraded MAGIC-1 sum trigger system, upper limits down to below 50 GeV have been obtained. This is the first time that
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::08c9c8db4b9d1bf17682c03a1beb3d21
https://ui.adsabs.harvard.edu/#abs/2009arXiv0907.0996G
https://ui.adsabs.harvard.edu/#abs/2009arXiv0907.0996G