We report on optical spectroscopy obtained at the 10.4 m Gran Telescopio Canarias of 28 Fermi γ-ray sources that completes the study of a sample of 60 targets...
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PublicaciónOptical Spectroscopic Survey of a Sample of Unidentified Fermi Objects: II
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PublicaciónOptical spectroscopy of blazars for the Cherenkov Telescope Array
Context. Blazars are the most numerous class of high-energy (HE; E ∼ 50 MeV−100 GeV) and very high-energy (VHE; E ∼ 100 GeV−10 TeV) gamma-ray emitters...
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PublicaciónOptical spectroscopy of blazars for the Cherenkov Telescope Array - III
Context. Blazars, which include BL Lacs and flat-spectrum radio quasars, represent the brightest persistent extragalactic sources in the high-energy (HE; 10 MeV...
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PublicaciónOverview of an extensive multi-wavelength study of GX 339-4 during the 2010 outburst
Context. The microquasar GX 339-4 experienced a new outburst in 2010: it was observed simultaneously at various wavelengths from radio up to soft γ-rays. We...
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PublicaciónOverview of an extensive multi-wavelength study of GX 339-4 during the 2010 outburst (Corrigendum)
Not Available
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PublicaciónPerformance of the joint LST-1 and MAGIC observations evaluated with Crab Nebula data
Aims: Large-Sized Telescope 1 (LST-1), the prototype for the Large-Sized Telescope at the upcoming Cherenkov Telescope Array Observatory, is concluding its...
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PublicaciónPeriastron Observations of TeV Gamma-Ray Emission from a Binary System with a 50-year Period
We report on observations of the pulsar/Be star binary system PSR J2032+4127/MT91 213 in the energy range between 100 {GeV} and 20 {TeV} with the Very Energetic...
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PublicaciónPeriodic Very High Energy γ-Ray Emission from LS I +61°303 Observed with the MAGIC Telescope
The MAGIC collaboration has recently reported the discovery of γ-ray emission from the binary system LS I +61°303 in the TeV energy region. Here we present new...
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PublicaciónPG 1553+113: Five Years of Observations with MAGIC
We present the results of five years (2005-2009) of MAGIC observations of the BL Lac object PG 1553+113 at very high energies (VHEs; E > 100 GeV). Power-law...