M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut)

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Presentation transcript:

M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut) MAGIC M.Teshima MPI für Physik, München (Werner-Heisenberg-Institut)

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 - 576 high QE PMTs (QEmax= 30%) Analog signal transport via optical fibers IPE CE NET 3-level trigger system & 300 MHz FADC system

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

Crab Nebula Preliminary

HESS J1813-178 Dark Particle Accelerator -- SNR

HESS J1834 extended source VLA 20cm Radio Molecular Cloud 13CO

Gamma-Ray Emission Processes

Active Galactic Nucleis M87

Extragalactic sources Spectral Indices of new sources range 3~4 PKS2005 PG1553 New Sources

Mrk421 (z=0.031) AGN (Blazar)

Mrk501 Giant flare 2005 July 01, IAU Circular #8562 2min resolution Light curve

1ES1218+304 (z=0.182) Soft Energy Spectrum Preliminary

PG 1553 (z>0.25) Very Soft energy spectrum the attenuation　by pair creation or nature of SSC mechanism

GRB observation by MAGIC Uniformity MAGIC GLAST Pulse Duration “short” “long” ~10sec GRB trigger Satellite to MAGIC ~20sec MAGIC slewing time

MAGIC made an observation in the period of the main prompt emission!! But we knew later z = 6.3.

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