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Published byPeter Geier Modified over 6 years ago
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M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut)
MAGIC M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut)
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Light weight Carbon fiber structure for fast repositioning
MAGIC Telescope 17 m diameter parabolic reflecting surface (240 m2 ) Light weight Carbon fiber structure for fast repositioning high reflective diamond milled aluminum mirrors Active mirror control (PSF: 90% of light in 0.1o inner pixel) - 3.5o FOV camera high QE PMTs (QEmax= 30%) Analog signal transport via optical fibers IPE CE NET 3-level trigger system & 300 MHz FADC system
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Highlights of MAGIC observations last one and a half year
Crab Nebular SZA & LZA Galactic Center HESS J1813 HESS J1834 13CO cloud GRB050713a GRB050904 (in prompt phase) Mrk421 (0.031) Mrk501 (0.034) IAU Circular #8562 1ES2344 (z=0.044) 1ES1959 (0.047) 1ES1218 (z=0.18) New Source PG 1553 (Z>0.25) New source
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Crab Nebula Preliminary
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HESS J1813-178 Dark Particle Accelerator -- SNR
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HESS J1834 extended source VLA 20cm Radio Molecular Cloud 13CO
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Gamma-Ray Emission Processes
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Active Galactic Nucleis
M87
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Extragalactic sources
Spectral Indices of new sources range 3~4 PKS2005 PG1553 New Sources
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Mrk421 (z=0.031) AGN (Blazar)
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Mrk501 Giant flare 2005 July 01, IAU Circular #8562
2min resolution Light curve
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1ES (z=0.182) Soft Energy Spectrum Preliminary
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PG 1553 (z>0.25) Very Soft energy spectrum
the attenuation by pair creation or nature of SSC mechanism
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GRB observation by MAGIC
Uniformity MAGIC GLAST Pulse Duration “short” “long” ~10sec GRB trigger Satellite to MAGIC ~20sec MAGIC slewing time
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MAGIC made an observation in the period of the
main prompt emission!! But we knew later z = 6.3.
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MAGIC one and a half year results
Source observations Galactic 4 sources are observed Extragalactic 6 sources are observed Distant sources show soft energy spectra The attenuation by e+- creation The nature of SSC mechanism The number of sources is increasing GRBs 9 fast follow-up observations are carried out 2 are in prompt phase among 9
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