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  4. The simultaneous low state spectral energy distribution of 1ES 2344+514 from radio to very high energies
 
research article

The simultaneous low state spectral energy distribution of 1ES 2344+514 from radio to very high energies

Aleksic, J.
•
Antonelli, L. A.
•
Antoranz, P.
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2013
Astronomy & Astrophysics

Context. BL Lacertae objects are variable at all energy bands on time scales down to minutes. To construct and interpret their spectral energy distribution (SED), simultaneous broad-band observations are mandatory. Up to now, the number of objects studied during such campaigns is very limited and biased towards high flux states. Aims. We present the results of a dedicated multi-wavelength study of the high-frequency peaked BL Lacertae (HBL) object and known TeV emitter 1ES 2344+514 by means of a pre-organised campaign. Methods. The observations were conducted during simultaneous visibility windows of MAGIC and AGILE in late 2008. The measurements were complemented by Mets hovi, RATAN-600, KVA+Tuorla, Swift and VLBA pointings. Additional coverage was provided by the ongoing long-term F-GAMMA and MOJAVE programs, the OVRO 40-m and CrAO telescopes as well as the Fermi satellite. The obtained SEDs are modelled using a one-zone as well as a self-consistent two-zone synchrotron self-Compton model. Results. 1ES 2344+514 was found at very low flux states in both X-rays and very high energy gamma rays. Variability was detected in the low frequency radio and X-ray bands only, where for the latter a small flare was observed. The X-ray flare was possibly caused by shock acceleration characterised by similar cooling and acceleration time scales. MOJAVE VLBA monitoring reveals a static jet whose components are stable over time scales of eleven years, contrary to previous findings. There appears to be no significant correlation between the 15 GHz and R-band monitoring light curves. The observations presented here constitute the first multi-wavelength campaign on 1ES 2344+514 from radio to VHE energies and one of the few simultaneous SEDs during low activity states. The quasi-simultaneous Fermi-LAT data poses some challenges for SED modelling, but in general the SEDs are described well by both applied models. The resulting parameters are typical for TeV emitting HBLs. Consequently it remains unclear whether a so-called quiescent state was found in this campaign.

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Type
research article
DOI
10.1051/0004-6361/201220714
Web of Science ID

WOS:000323893500067

Author(s)
Aleksic, J.
Antonelli, L. A.
Antoranz, P.
Asensio, M.
Backes, M.
De Almeida, U. Barres
Barrio, J. A.
Bednarek, W.
Berger, K.
Bernardini, E.
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Corporate authors
MAGIC Collaboration; AGILE Team; Fermi-LAT Collaboration; F-GAMMA Program
Date Issued

2013

Publisher

Edp Sciences S A

Published in
Astronomy & Astrophysics
Volume

556

Start page

A67

Subjects

galaxies: active

•

BL Lacertae objects: individual: 1ES 2344+514

•

gamma rays: galaxies

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X-rays: individuals: 1ES 2344+514

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radiation mechanisms: non-thermal

Editorial or Peer reviewed

REVIEWED

Written at

EPFL

EPFL units
LPHE  
Available on Infoscience
November 4, 2013
Use this identifier to reference this record
https://infoscience.epfl.ch/handle/20.500.14299/96710
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