Observation of VHE Gamma Ray Sources with the MAGIC telescope
Observation of VHE Gamma Ray Sources with the MAGIC telescope
Observation of VHE Gamma Ray Sources with the MAGIC telescope
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Mkn 421 (z=0.030)<br />
SED<br />
SSC constraints<br />
log(B)<br />
A<br />
B<br />
C<br />
log(B)<br />
D<br />
E<br />
F<br />
• In case <strong>of</strong> 1-day<br />
variability scale, <strong>the</strong><br />
model provides similar<br />
parameters as from <strong>the</strong><br />
1994 flare: D=9, B=0.3G<br />
log(D)<br />
log(D)<br />
astro-ph/0603478<br />
P.Majumdar, 24 th August, IIA, India
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