most citedHard TeV spectra of blazars and the constraints to the IR intergalactic background

118 citations · 260 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.EP2018★ 14 cited

Two planetary systems with transiting Earth-size and super-Earth planets orbiting late-type dwarf stars

E. Diez Alonso, J. I. Gonzalez Hernandez, S. L. Suarez Gomez +9

We present two new planetary systems found around cool dwarf stars with data from the K2 mission. The first system was found in K2-239 (EPIC 248545986), char- acterized in this wor…

astro-ph2006★ 44 cited

Testing the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71: II. A search for intra-day variability at millimetre wavelengths with the IRAM 30 m telescope

I. Agudo, T. P. Krichbaum, H. Ungerechts +12

We report on a densely time sampled polarimetric flux density monitoring of the BL Lac object S5 0716+71 at 86 GHz and 229 GHz with the IRAM 30 m telescope within a coordinated bro…

astro-ph2006★ 118 cited

Hard TeV spectra of blazars and the constraints to the IR intergalactic background

K. Katarzynski, G. Ghisellini, F. Tavecchio +2

Recent gamma-ray observations of the blazar 1ES 1101-232 (redshift z=0.186) reveal that the unabsorbed TeV spectrum is hard, with spectral index [$F(ν) \propto ν^{-…

astro-ph2006★ 72 cited

Testing the inverse-Compton catastrophe scenario in the intra-day variable blazar S5 0716+71. I. Simultaneous broadband observations during November 2003

L. Ostorero, S. J. Wagner, J. Gracia +6

Some intra-day variable, compact extra-galactic radio sources show brightness temperatures severely exceeding 10^{12} K, the limit set by catastrophic inverse-Compton (IC) cooling…

astro-ph2006★ 12 cited

The cyclo-synchrotron process and particle heating through the absorption of photons

K. Katarzynski, G. Ghisellini, R. Svensson +1

We propose a new approximation for the cyclo-synchrotron emissivity of a single electron. In the second part of this work, we discuss a simple application for our approximation, an…