4
Conferences
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ICN-UNAM
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3
icrc2007@icrc2007.unam.mx
30th International Cosmic Ray Conference
The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.
True
Merida, Mexico
2007-07-03T08:00:00
2007-07-11T19:00:00
2005-09-26T05:04:53
2024-04-12T17:46:55
Mexico/General
Dr.
IGeof-UNAM
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657
false
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0
Oral
Observations of a systematic selected sample of X-ray bright HBL objects with the MAGIC telescope
Mr.
Institut fuer Theoretische Physik und Astrophysik, Universitaet Wuerzburg
49c09932e773345385a049967da3f749
Mr.
Institut fuer Theoretische Physik und Astrophysik, Universitaet Wuerzburg
49c09932e773345385a049967da3f749
Dr.
Institut fuer Theoretische Physik und Astrophysik, Universitaet Wuerzburg
d41d8cd98f00b204e9800998ecf8427e
Ms.
Institut fuer Theoretische Physik und Astrophysik, Universitaet Wuerzburg
d41d8cd98f00b204e9800998ecf8427e
Merida, Mexico
Uxmal + Tulum (Holiday Inn)
2007-07-09T08:42:00
2007-07-09T08:54:00
00:12
Up to now, nearly all the detected extragalactic VHE gamma-ray sources belong to the
class of high-frequency peaked BL Lac objects (HBL), which show a pronounced peak in
the hard X-ray band. All detected VHE sources show a comparable luminosity at TeV
energies.
MAGIC has started a systematic scan on X-ray bright HBL objects in the northern sky
during its cycle1 observations from January 2005 to March 2006. Following the blazar
compilation by Donato et al. (2001), 13 HBLs were selected with the criteria of low
redshift (< 0.3), high X-ray flux (F(1keV) > 2uJy) and visibility under small zenith
distances (< 30deg at culmination, leading to sources with a declination between -2
and +58).
In that campaign 1ES 1218+30.4 was discovered and 1ES 2344+51.4 was detected in a low
flux state with high significance. For another 10 sources upper limits on the
integral flux above ~200GeV will be presented at the conference.
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1
More information about the venue
http://www.icrc2007.unam.mx/
link
http://www.icrc2007.unam.mx/
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