Observation of VHE Gamma Ray Sources with the MAGIC telescope

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1ES1218+304 (z=0.182) • Is it possible to derive EBL constraints from the 1ES1218 spectrum • Assuming 6 different EBL realizations, all reconstructed de-absorbed spectra do not contradict the rising slope dN/dE ∼ E -Γ , Γ > 1.5 P.Majumdar, 24 th August, IIA, India
PG1553+113 (z>0.09) • Observed 18.8h in 2005-06 • H.E.S.S.: 4.0σ evidence (A&A 448L (2006), 43) • MAGIC: astro-ph/0606161 • 8.8σ, firm detection. Alpha plot lightcurve spectrum P.Majumdar, 24 th August, IIA, India
Page 1 and 2: Observation of VHE Gamma Ray Source
Page 3 and 4: Cosmic Radiation original motivatio
Page 5 and 6: Physics Motivation for MAGIC Pulsar
Page 7 and 8: Imaging Air Cherenkov Telescopes Ga
Page 9 and 10: Standard “Hillas” Analysis LENG
Page 11 and 12: Wave front Sampling Cerenkov Telesc
Page 13 and 14: The unexplored spectrum gap • Str
Page 15 and 16: The MAGIC telescope • Largest Ima
Page 17 and 18: • October 2003: Inauguration Stat
Page 19 and 20: MAGIC HIGHLIGHTS LSI+61 303 Galacti
Page 21 and 22: Search for Pulsations in VHE data
Page 23 and 24: Galactic Center Stars around center
Page 25 and 26: HESSJ 1813-178 178 Section of shell
Page 27 and 28: • Microquasars: • Binary system
Page 29 and 30: LS I +61 303: the film Albert et al
Page 31 and 32: Contemporaneous radio observations
Page 33 and 34: Mkn 421 (z=0.030) spectrum • Dec
Page 35 and 36: • June - July 2005 • 23.1 h, ov
Page 37 and 38: Mkn 180 (z=0.045) • Whipple: F (>
Page 39: 1ES1218+304 (z=0.182) • Whipple:
Page 43 and 44: First year operation (Sep04-Sep05):
Page 45 and 46: Extension of MAGIC => MAGIC II •
Page 47 and 48: MAGIC II Monte Carlo Studies •Ste
Page 49 and 50: MAGIC II: Sensitivity gain using St

Observation of VHE Gamma Ray Sources with the MAGIC telescope

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