TeV flaring activity of the AGN PKS 0625-354 in November 2018

Aharonian, F.; Benkhali, F. Ait; Aschersleben, J.; Ashkar, H.; Backes, M.; Baktash, A.; Martins, V. Barbosa; Barnard, J.; Batzofin, R.; Becherini, Yvonne; Berge, D.; Bernloehr, K.; Bi, B.; Bottcher, M.; Boisson, C.; Bolmont, J.; de Lavergne, M. de Bony; Borowska, J.; Bradascio, F.; Breuhaus, M.; Brose, R.; Brown, A.; Brun, F.; Bruno, B.; Bulik, T.; Burger-Scheidlin, C.; Bylund, T.; Caroff, S.; Casanova, S.; Cecil, R.; Celic, J.; Cerruti, M.; Chand, T.; Chandra, S.; Chen, A.; Chibueze, J.; Chibueze, O.; Cotter, G.; Mbarubucyeye, J. Damascene; Davids, I. D.; Djuvsland, J.; Dmytriiev, A.; Doroshenko, V.; Egberts, K.; Einecke, S.; Ernenwein, J. -P; Fontaine, G.; Fuessling, M.; Funk, S.; Gabici, S.; Ghafourizadeh, S.; Giavitto, G.; Glawion, D.; Glicenstein, J. F.; Glombitza, J.; Goswami, P.; Grolleron, G.; Haerer, L.; Hinton, J. A.; Holch, T. L.; Holler, M.; Horns, D.; Jamrozy, M.; Jankowsky, F.; Joshi, V.; Jung-Richardt, I.; Kasai, E.; Katarzynski, K.; Khatoon, R.; Khelifi, B.; Kluniak, W.; Komin, Nu.; Kosack, K.; Kostunin, D.; Lang, R. G.; Le Stum, S.; Leitl, F.; Lemiere, A.; Lenain, J. -P; Leuschner, F.; Luashvili, A.; Mackey, J.; Marx, R.; Mehta, A.; Meyer, M.; Mitchell, A.; Moderski, R.; Montanari, A.; Moulin, E.; de Naurois, M.; Niemiec, J.; O'Brien, P.; Ohm, S.; Olivera-Nieto, L.; Wilhelmi, E. de Ona; Ostrowski, M.; Panny, S.; Parsons, R. D.; Pita, S.; Prokhorov, D. A.; Puehlhofer, G.; Punch, M.; Quirrenbach, A.; Reichherzer, P.; Reimer, A.; Reimer, O.; Ren, H.; Rieger, F.; Rudak, B.; Sahakian, V.; Salzmann, H.; Sanchez, D. A.; Sasaki, M.; Schuessler, F.; Schutte, H. M.; Shapopi, J. N. S.; Sol, H.; Specovius, A.; Spencer, S.; Stawarz, L.; Steenkamp, R.; Steinmassl, S.; Streil, K.; Sushch, I.; Suzuki, H.; Takahashi, T.; Tanaka, T.; van Eldik, C.; Vecchi, M.; Veh, J.; Venter, C.; Wagner, S. J.; Wierzcholska, A.; Zacharias, M.; Zargaryan, D.; Zdziarski, A. A.; Zech, A.; Zouari, S.; Zywucka, N.

lnu.sePublications

Simple search

Advanced search -
Research publications Advanced search -
Student theses Statistics

English Svenska Norsk

Change search

Cite ExportLink to record

Permanent link

https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-128813

Direct link

http://lnu.diva-portal.org/smash/record.jsf?pid=diva2:1851266

Cite

Citation style

apa
ieee
modern-language-association-8th-edition
vancouver
Other style

More styles

Language

de-DE
en-GB
en-US
fi-FI
nn-NO
nn-NB
sv-SE
Other locale

More languages

Output format

html
text
asciidoc
rtf

TeV flaring activity of the AGN PKS 0625-354 in November 2018

Aharonian, F.

Dublin Inst Adv Studies, Ireland;Max Planck Inst Kernphys, Germany;Yerevan State Univ, Armenia.

Benkhali, F. Ait

Heidelberg Univ, Germany.

Aschersleben, J.

Univ Groningen, Netherlands.

Ashkar, H.

Ecole Polytech, France.

Show others and affiliations

2024 (English)In: Astronomy and Astrophysics, ISSN 0004-6361, E-ISSN 1432-0746, Vol. 683, article id A70Article in journal (Refereed) Published

Abstract [en]

Most gamma-ray detected active galactic nuclei are blazars with one of their relativistic jets pointing towards the Earth. Only a few objects belong to the class of radio galaxies or misaligned blazars. Here, we investigate the nature of the object PKS 0625-354, its gamma-ray flux and spectral variability and its broad-band spectral emission with observations from H.E.S.S., Fermi-LAT, Swift-XRT, and UVOT taken in November 2018. The H.E.S.S. light curve above 200 GeV shows an outburst in the first night of observations followed by a declining flux with a halving time scale of 5.9 h. The gamma gamma-opacity constrains the upper limit of the angle between the jet and the line of sight to similar to 10 degrees. The broad-band spectral energy distribution shows two humps and can be well fitted with a single-zone synchrotron self Compton emission model. We conclude that PKS 0625-354, as an object showing clear features of both blazars and radio galaxies, can be classified as an intermediate active galactic nuclei. Multi-wavelength studies of such intermediate objects exhibiting features of both blazars and radio galaxies are sparse but crucial for the understanding of the broad-band emission of gamma-ray detected active galactic nuclei in general.

Place, publisher, year, edition, pages

EDP Sciences, 2024. Vol. 683, article id A70

Keywords [en]

galaxies: active, galaxies: individual: PKS 0625-354, galaxies: jets, gamma rays: galaxies

National Category

Astronomy, Astrophysics and Cosmology

Research subject

Physics, Astroparticle Physics

Identifiers

URN: urn:nbn:se:lnu:diva-128813DOI: 10.1051/0004-6361/202348063ISI: 001185071900015Scopus ID: 2-s2.0-85187160658OAI: oai:DiVA.org:lnu-128813DiVA, id: diva2:1851266

Available from: 2024-04-12 Created: 2024-04-12 Last updated: 2024-04-23Bibliographically approved

Open Access in DiVA

No full text in DiVA

Authority records

Becherini, Yvonne

Search in DiVA

doi

urn-nbn

Total: 52 hits

Cite ExportLink to record

Permanent link

https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-128813

Direct link

http://lnu.diva-portal.org/smash/record.jsf?pid=diva2:1851266

Cite

Citation style

apa
ieee
modern-language-association-8th-edition
vancouver
Other style

More styles

Language

de-DE
en-GB
en-US
fi-FI
nn-NO
nn-NB
sv-SE
Other locale

More languages

Output format

html
text
asciidoc
rtf

v. 2.46.0

WCAG

DiVA support

Linnaeus University Library

Linnaeus University Press

Publish/Register