Abstract: Since October 2011, the First G-APD Cherenkov Telescope (FACT) is operated successfully on the Canary Island of La Palma. Apart from the proof of principle for the use of G-APDs in Cherenkov telescopes, the major goal of the project is the dedicated long-term monitoring of a small sample of bright TeV blazars. The unique properties of G-APDs permit stable observations also during strong moon light. Thus a superior sampling density is provided on time scales at which the blazar variability amplitudes are expected to be largest, as exemplified by the spectacular variations of Mrk 501 observed in June 2012. While still in commissioning, FACT monitored bright blazars like Mrk 421 and Mrk 501 during the past 1.5 years so far. Prelimina...
Mrk 421 and Mrk 501 are two close bright and well-studied high-synchrotron-peaked blazars, which fea...
Markarian 421 and Markarian 501 are Active Galactic Nuclei and two of the most prominent sources of ...
The BL Lac type object Mrk 501 was observed at very high energies (E > 100 GeV) in 2014 with the upg...
The First G-APD Cherenkov Telescope (FACT), located on the Canary Island of La Palma, has been takin...
Abstract: The First G-APD Cherenkov Telescope (FACT) is the first Cherenkov telescope equipped with ...
The First G-APD Cherenkov Telescope (FACT) has been monitoring blazars at TeV energies for more than...
Blazars like Markarian 421 or Markarian 501 are active galactic nuclei (AGN), with their jets orient...
Blazars like Markarian 421 or Markarian 501 are active galactic nuclei (AGN), with their jets orient...
FACT is the first imaging Cherenkov telescope based on a camera using solid state photosensors (Geig...
The First G-APD Cherenkov Telescope (FACT) is monitoring blazars at TeV energies. Thanks to the obse...
The First G-APD Cherenkov Telescope (FACT) has been monitoring TeV-blazars since October 2011. Thank...
Abstract: We have been operating a 7 element atmospheric Cherenkov telescope array called HAGAR at v...
Active galactic nuclei show variability on time scales ranging from minutes to decades. The radiatio...
International audienceThe BL Lac type object Mrk 501 was observed at very high energies (E>100 GeV) ...
Abstract: As the most active blazars, Mrk421 and Mrk 501 are excellent candidates for the study of t...
Mrk 421 and Mrk 501 are two close bright and well-studied high-synchrotron-peaked blazars, which fea...
Markarian 421 and Markarian 501 are Active Galactic Nuclei and two of the most prominent sources of ...
The BL Lac type object Mrk 501 was observed at very high energies (E > 100 GeV) in 2014 with the upg...
The First G-APD Cherenkov Telescope (FACT), located on the Canary Island of La Palma, has been takin...
Abstract: The First G-APD Cherenkov Telescope (FACT) is the first Cherenkov telescope equipped with ...
The First G-APD Cherenkov Telescope (FACT) has been monitoring blazars at TeV energies for more than...
Blazars like Markarian 421 or Markarian 501 are active galactic nuclei (AGN), with their jets orient...
Blazars like Markarian 421 or Markarian 501 are active galactic nuclei (AGN), with their jets orient...
FACT is the first imaging Cherenkov telescope based on a camera using solid state photosensors (Geig...
The First G-APD Cherenkov Telescope (FACT) is monitoring blazars at TeV energies. Thanks to the obse...
The First G-APD Cherenkov Telescope (FACT) has been monitoring TeV-blazars since October 2011. Thank...
Abstract: We have been operating a 7 element atmospheric Cherenkov telescope array called HAGAR at v...
Active galactic nuclei show variability on time scales ranging from minutes to decades. The radiatio...
International audienceThe BL Lac type object Mrk 501 was observed at very high energies (E>100 GeV) ...
Abstract: As the most active blazars, Mrk421 and Mrk 501 are excellent candidates for the study of t...
Mrk 421 and Mrk 501 are two close bright and well-studied high-synchrotron-peaked blazars, which fea...
Markarian 421 and Markarian 501 are Active Galactic Nuclei and two of the most prominent sources of ...
The BL Lac type object Mrk 501 was observed at very high energies (E > 100 GeV) in 2014 with the upg...