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Simultaneous observations of the blazar PKS 2155-304 from ultra-violet to TeV energies

Authors :
26598973 - Abdalla, Hassan
30588766 - Arcaro, Cornelia
28644743 - Backes, Michael
20574266 - Barnard, Monica
24420530 - Böttcher, Markus
30366755 - Chand, Tej B.
31125417 - Chandra, Sunil
33379009 - Kreter, Michael
26403366 - Ndiyavala, Hambeleleni
22799133 - Schutte, Hester M.
20126999 - Seyffert, Albertus Stefanus
10060499 - Van der Walt, Diederick Johannes
21106266 - Van Rensburg, Carlo
12006653 - Venter, Christo
26594080 - Wadiasingh, Zorawar
29092086 - Zacharias, Michael
34208968 - Zywucka-Hejzner, Natalia
Abdalla, H.
Arcaro, C.
Backes, M.
Barnard, M.
Böttcher, M.
Chand, T.
Chandra, S.
Kreter, M.
Ndiyavala, H.
Schutte, H.M.
Seyffert, A.S.
Van der Walt, D.J.
Van Rensburg, C.
Venter, C.
Wadiasingh, Z.
Zacharias, M.
Zywucka, N.
H.E.S.S. Collaboration
Fermi LAT
26598973 - Abdalla, Hassan
30588766 - Arcaro, Cornelia
28644743 - Backes, Michael
20574266 - Barnard, Monica
24420530 - Böttcher, Markus
30366755 - Chand, Tej B.
31125417 - Chandra, Sunil
33379009 - Kreter, Michael
26403366 - Ndiyavala, Hambeleleni
22799133 - Schutte, Hester M.
20126999 - Seyffert, Albertus Stefanus
10060499 - Van der Walt, Diederick Johannes
21106266 - Van Rensburg, Carlo
12006653 - Venter, Christo
26594080 - Wadiasingh, Zorawar
29092086 - Zacharias, Michael
34208968 - Zywucka-Hejzner, Natalia
Abdalla, H.
Arcaro, C.
Backes, M.
Barnard, M.
Böttcher, M.
Chand, T.
Chandra, S.
Kreter, M.
Ndiyavala, H.
Schutte, H.M.
Seyffert, A.S.
Van der Walt, D.J.
Van Rensburg, C.
Venter, C.
Wadiasingh, Z.
Zacharias, M.
Zywucka, N.
H.E.S.S. Collaboration
Fermi LAT
Publication Year :
2020

Abstract

Here we report the results of the first ever contemporaneous multi-wavelength observation campaign on the BL Lac object PKS 2155−304 involving Swift, NuSTAR, Fermi-LAT, and H.E.S.S. The use of these instruments allows us to cover a broad energy range, which is important for disentangling the different radiative mechanisms. The source, observed from June 2013 to October 2013, was found in a low flux state with respect to previous observations but exhibited highly significant flux variability in the X-rays. The high-energy end of the synchrotron spectrum can be traced up to 40 keV without significant contamination by high-energy emission. A one-zone synchrotron self-Compton model was used to reproduce the broadband flux of the source for all the observations presented here but failed for previous observations made in April 2013. A lepto-hadronic solution was then explored to explain these earlier observational results

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1204156794
Document Type :
Electronic Resource