FRINK Linked Data Fragments server

Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100849393> ?p ?o ?g. }

• W3100849393 endingPage "43" @default.
• W3100849393 startingPage "43" @default.
• W3100849393 abstract "Intergalactic space is believed to contain nonzero magnetic fields (the Intergalactic Magnetic Field: IGMF), which at scales of megaparsecs would have intensities below 10−9 G. Very high energy (VHE > 100 GeV) gamma-rays coming from blazars can produce e+e− pairs when interacting with the extragalactic background light (EBL) and the cosmic microwave background, generating an electromagnetic cascade of megaparsec scale. The IGMF may produce a detectable broadening of the emission beam that could lead to important constrains both on the IGMF intensity and its coherence length. Using the Monte Carlo–based Elmag code, we simulate the electromagnetic cascade corresponding to two detected TeV sources: PKS 2155-304 visible from the south and H1426+428 visible from the north. Assuming an EBL model and intrinsic spectral properties of the sources, we obtain the spectral and angular distribution of photons when they arrive at Earth. We include the response of the next generation Cherenkov telescopes by using simplified models for Cherenkov Telescope Array (CTA)-south and CTA-north based on a full simulation of each array performance. Combining the instrument properties with the simulated source fluxes, we calculate the telescope point-spread function for null and non-null IGMF intensities and develop a method to test the statistical feasibility of detecting IGMF imprints by comparing the resulting angular distributions. Our results show that for the analyzed source PKS 2155-304 corresponding to the southern site, CTA should be able to detect IGMF with intensities stronger than 10−14.5 G within an observation time of ∼100 hr." @default.
• W3100849393 created "2020-11-23" @default.
• W3100849393 creator A5039583454 @default.
• W3100849393 creator A5040005080 @default.
• W3100849393 creator A5087036414 @default.
• W3100849393 date "2018-12-10" @default.
• W3100849393 modified "2023-09-23" @default.
• W3100849393 title "Probing the IGMF with the Next Generation of Cherenkov Telescopes" @default.
• W3100849393 cites W1870194148 @default.
• W3100849393 cites W1908731306 @default.
• W3100849393 cites W1910027932 @default.
• W3100849393 cites W1961022487 @default.
• W3100849393 cites W1987386374 @default.
• W3100849393 cites W1988365750 @default.
• W3100849393 cites W2000775663 @default.
• W3100849393 cites W2007414583 @default.
• W3100849393 cites W2011255110 @default.
• W3100849393 cites W2015853838 @default.
• W3100849393 cites W2038183147 @default.
• W3100849393 cites W2063219550 @default.
• W3100849393 cites W2064378914 @default.
• W3100849393 cites W2077044031 @default.
• W3100849393 cites W2099269353 @default.
• W3100849393 cites W2104721808 @default.
• W3100849393 cites W2127444529 @default.
• W3100849393 cites W2128416925 @default.
• W3100849393 cites W2138003640 @default.
• W3100849393 cites W2150864365 @default.
• W3100849393 cites W2162367553 @default.
• W3100849393 cites W2170572195 @default.
• W3100849393 cites W2170807451 @default.
• W3100849393 cites W2300573172 @default.
• W3100849393 cites W2579155888 @default.
• W3100849393 cites W2949421289 @default.
• W3100849393 cites W3098670504 @default.
• W3100849393 cites W3099193611 @default.
• W3100849393 cites W3100111518 @default.
• W3100849393 cites W3103428427 @default.
• W3100849393 cites W3103990726 @default.
• W3100849393 cites W3122712798 @default.
• W3100849393 cites W3125587661 @default.
• W3100849393 doi "https://doi.org/10.3847/1538-4357/aae976" @default.
• W3100849393 hasPublicationYear "2018" @default.
• W3100849393 type Work @default.
• W3100849393 sameAs 3100849393 @default.
• W3100849393 citedByCount "6" @default.
• W3100849393 countsByYear W31008493932019 @default.
• W3100849393 countsByYear W31008493932020 @default.
• W3100849393 countsByYear W31008493932021 @default.
• W3100849393 crossrefType "journal-article" @default.
• W3100849393 hasAuthorship W3100849393A5039583454 @default.
• W3100849393 hasAuthorship W3100849393A5040005080 @default.
• W3100849393 hasAuthorship W3100849393A5087036414 @default.
• W3100849393 hasBestOaLocation W31008493931 @default.
• W3100849393 hasConcept C100752510 @default.
• W3100849393 hasConcept C105795698 @default.
• W3100849393 hasConcept C111309251 @default.
• W3100849393 hasConcept C120665830 @default.
• W3100849393 hasConcept C121332964 @default.
• W3100849393 hasConcept C1276947 @default.
• W3100849393 hasConcept C159317903 @default.
• W3100849393 hasConcept C182107563 @default.
• W3100849393 hasConcept C19499675 @default.
• W3100849393 hasConcept C207297109 @default.
• W3100849393 hasConcept C2778336740 @default.
• W3100849393 hasConcept C2780848835 @default.
• W3100849393 hasConcept C33024259 @default.
• W3100849393 hasConcept C33923547 @default.
• W3100849393 hasConcept C44870925 @default.
• W3100849393 hasConcept C522846370 @default.
• W3100849393 hasConcept C534381523 @default.
• W3100849393 hasConcept C55047584 @default.
• W3100849393 hasConcept C72591435 @default.
• W3100849393 hasConcept C7910260 @default.
• W3100849393 hasConcept C85725439 @default.
• W3100849393 hasConcept C94915269 @default.
• W3100849393 hasConcept C98444146 @default.
• W3100849393 hasConceptScore W3100849393C100752510 @default.
• W3100849393 hasConceptScore W3100849393C105795698 @default.
• W3100849393 hasConceptScore W3100849393C111309251 @default.
• W3100849393 hasConceptScore W3100849393C120665830 @default.
• W3100849393 hasConceptScore W3100849393C121332964 @default.
• W3100849393 hasConceptScore W3100849393C1276947 @default.
• W3100849393 hasConceptScore W3100849393C159317903 @default.
• W3100849393 hasConceptScore W3100849393C182107563 @default.
• W3100849393 hasConceptScore W3100849393C19499675 @default.
• W3100849393 hasConceptScore W3100849393C207297109 @default.
• W3100849393 hasConceptScore W3100849393C2778336740 @default.
• W3100849393 hasConceptScore W3100849393C2780848835 @default.
• W3100849393 hasConceptScore W3100849393C33024259 @default.
• W3100849393 hasConceptScore W3100849393C33923547 @default.
• W3100849393 hasConceptScore W3100849393C44870925 @default.
• W3100849393 hasConceptScore W3100849393C522846370 @default.
• W3100849393 hasConceptScore W3100849393C534381523 @default.
• W3100849393 hasConceptScore W3100849393C55047584 @default.
• W3100849393 hasConceptScore W3100849393C72591435 @default.
• W3100849393 hasConceptScore W3100849393C7910260 @default.
• W3100849393 hasConceptScore W3100849393C85725439 @default.

• next