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SUMMARY:MAGIC detection of very-high-energy gamma-ray emission from the z 
 = 0.94 blazar PKS 1441+25
DTSTART;VALUE=DATE-TIME:20151026T061500Z
DTEND;VALUE=DATE-TIME:20151026T063000Z
DTSTAMP;VALUE=DATE-TIME:20260412T054937Z
UID:indico-contribution-822@indico.icrr.u-tokyo.ac.jp
DESCRIPTION:Speakers: Miguel Nievas-Rosillo (Universidad Complutense de Ma
 drid\, Grupo de Altas Energías)\nVery-high-energy (VHE\, E > 100 GeV) gam
 ma-ray emission from the very distant flat spectrum radio quasar PKS 1441+
 25 (z = 0.940) was detected in April 2015 with the MAGIC telescopes. Aside
  from the gravitationally lensed VHE blazar QSO B0218+357 (z = 0.944)\, al
 so detected by MAGIC\, PKS 1441+25 is the most distant VHE blazar detected
  to date. The VHE detection occurred in April 2015 during enhanced activit
 y of the source at high energy (HE\, 0.1 GeV \n\nhttps://indico.icrr.u-tok
 yo.ac.jp/event/23/contributions/822/
LOCATION: Room 5.6
URL:https://indico.icrr.u-tokyo.ac.jp/event/23/contributions/822/
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