most citedUpper limit for gamma-ray emission above 140 GeV from the dwarf spheroidal galaxy Draco

74 citations · 96 across the 6 of their papers we have counts for

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astro-ph2007

Science with the new generation high energy gamma- ray experiments

M. Alvarez, D. D'Armiento, G. Agnetta +197

This Conference is the fifth of a series of Workshops on High Energy Gamma- ray Experiments, following the Conferences held in Perugia 2003, Bari 2004, Cividale del Friuli 2005, El…

astro-ph200774 cited

Upper limit for gamma-ray emission above 140 GeV from the dwarf spheroidal galaxy Draco

MAGIC Collaboration, J. Albert

The nearby dwarf spheroidal galaxy Draco with its high mass to light ratio is one of the most auspicious targets for indirect dark matter searches. Annihilation of hypothetical DM…

astro-ph2007

MAGIC upper limits on the high energy emission from GRBs

D. Bastieri, N. Galante, M. Garczarczyk +4

During its cycle-1 observation period, between April 2005 and March 2006, the MAGIC telescope was able to observe nine Gamma Ray Burst (GRB) events since their early beginning. Oth…

astro-ph2007

Observation of GRBs by the MAGIC Telescope, Status and Outlook

D. Bastieri, N. Galante, M. Garczarczyk +4

Observation of Gamma Ray Bursts (GRBs) in the Very High Energy (VHE) domain will provide important information on the physical conditions in GRB outflows. The MAGIC telescope is th…

astro-ph20076 cited

A method to measure the mirror reflectivity of a prime focus telescope

R. Mirzoyan, M. Garczarczyk, J. Hose +1

We have developed a method to measure the mirror reflectivity of telescopes. While it is relatively easy to measure the local reflectivity of the mirror material, it is not so stra…

astro-ph200716 cited

Constraints on the steady and pulsed very high energy gamma-ray emission from observations of PSR B1951+32/CTB 80 with the MAGIC Telescope

MAGIC Collaboration, J. Albert

We report on very high energy gamma-observations with the MAGIC Telescope of the pulsar PSR B1951+32 and its associated nebula, CTB 80. Our data constrain the cutoff energy of the…