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

74 citations · 90 across the 2 of their papers we have counts for

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astro-ph200860 cited

Discovery of a very high energy gamma-ray signal from the 3C 66A/B region

MAGIC Collaboration, E. Aliu

The MAGIC telescope observed the region around the distant blazar 3C 66A for 54.2 h in 2007 August-December. The observations resulted in the discovery of a gamma-ray source at ene…

astro-ph2008203 cited

Observation of Pulsed Gamma-rays Above 25 GeV from the Crab Pulsar with MAGIC

The MAGIC Collaboration, E. Aliu

One fundamental question about pulsars concerns the mechanism of their pulsed electromagnetic emission. Measuring the high-end region of a pulsar's spectrum would shed light on thi…

astro-ph2008111 cited

Periodic very high energy gamma-ray emission from LS I +61 303 observed with the MAGIC telescope

MAGIC Collaboration, J. Albert

The MAGIC collaboration has recently reported the discovery of gamma-ray emission from the binary system LS I +61 303 in the TeV energy region. Here we present new observational re…

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-ph2007301 cited

VHE Gamma-Ray Observation of the Crab Nebula and its Pulsar with the MAGIC telescope

MAGIC Collaboration, J. Albert

We report about very high energy (VHE) gamma-ray observations of the Crab Nebula with the MAGIC telescope. The gamma-ray flux from the nebula was measured between 60 GeV and 9 TeV.…

astro-ph2007125 cited

Discovery of very high energy gamma-ray emission from the low-frequency peaked BL Lacertae object BL Lacertae

MAGIC Collaboration, J. Albert

The MAGIC collaboration observed BL Lacertae for 22.2 hr during 2005 August to December and for 26 hr during 2006 July to September. The source is the historical prototype and epon…