activity
20132019
most citedProspects for CTA observations of the young SNR RX J1713.7-3946

23 citations · 26 across the 8 of their papers we have counts for

collaborators

10 papers

astro-ph.IM2019

The Cherenkov transparency coefficient for the atmospheric monitoring and array calibration at the Cherenkov Telescope Array South

Stanislav Stefanik, Dalibor Nosek

Reconstruction of energies of very-high-energy gamma-rays observed by imaging atmospheric Cherenkov telescopes is affected by changes in the atmospheric conditions and the performa…

astro-ph.IM2017

Atmospheric monitoring and array calibration in CTA using the Cherenkov Transparency Coefficient

Stanislav Stefanik, Raquel de los Reyes, Dalibor Nosek

The Cherenkov Telescope Array (CTA) will be the next generation observatory employing different types of Cherenkov telescopes for the detection of particle showers initiated by ver…

astro-ph.IM2017

Atmospheric calibration of the Cherenkov Telescope Array

Jan Ebr, Tomasz Bulik, Lluis Font +7

Atmospheric monitoring is an integral part of the design of the Cherenkov Telescope Array (CTA), as atmospheric conditions affect the observations by Imaging Atmospheric Cherenkov…

astro-ph.HE2017★ 23 cited

Prospects for CTA observations of the young SNR RX J1713.7-3946

The CTA Consortium, :, F. Acero +381

We perform simulations for future Cherenkov Telescope Array (CTA) observations of RX~J1713.73946, a young supernova remnant (SNR) and one of the brightest sources ever discovere…

astro-ph.HE2015

Variability of VHE -ray emission from the binary PSR B1259-63/LS 2883

Stanislav Stefanik, Dalibor Nosek

We examine changes of the -ray intensity observed from the direction of the binary system PSR B1259-63/LS 2883 during campaigns around its three periastron passages. A simple an…

astro-ph.IM2015

Significance for signal changes in gamma-ray astronomy

Dalibor Nosek, Stanislav Stefanik, Jana Nosková

We describe a straightforward modification of frequently invoked methods for the determination of the statistical significance of a gamma-ray signal observed in a counting process.…

astro-ph.HE2015

Unexpected gamma-ray signal in the vicinity of 1ES 0229+200

Stanislav Stefanik, Dalibor Nosek

We report on an unidentified gamma-ray signal found in the region around the BL Lac object 1ES 0229+200. It was recognized serendipitously in our analysis of 6.2 years of Fermi-LAT…

astro-ph.HE2014★ 1 cited

Variability of VHE -ray sources

Stanislav Stefanik, Dalibor Nosek

We study changes in the -ray intensity at very high energies observed from selected active galactic nuclei. Publicly available data collected by Cherenkov telescopes were examin…

astro-ph.HE2014

Time variability of the -ray binary HESS J0632+057

Stanislav Stefanik, Dalibor Nosek

We study changes in the --ray intensity at very high energies observed from the --ray binary HESS J0632+057. Publicly available data collected by Cherenkov telescopes were ex…

astro-ph.IM2013★ 2 cited

Testing time variability of gamma-ray flux

Dalibor Nosek, Stanislav Stefanik, Jana Noskova

A way of examining a hypothetical non--zero --ray signal for the time changes is presented. The time variability of the recently observed --ray source PKS 2155--304 is discus…