2018A&A...610A..74K


C.D.S. - SIMBAD4 rel 1.7 - 2020.04.02CEST12:59:52

2018A&A...610A..74K - Astronomy and Astrophysics, volume 610A, 74-74 (2018/2-1)

Far-infrared photometry of OJ 287 with the Herschel Space Observatory.

KIDGER M., ZOLA S., VALTONEN M., LAHTEENMAKI A., JARVELA E., TORNIKOSKI M., TAMMI J., LIAKOS A. and POYNER G.

Abstract (from CDS):

Context. The blazar OJ 287 has shown a ~=12 year quasi-periodicity over more than a century, in addition to the common properties of violent variability in all frequency ranges. It is the strongest known candidate to have a binary singularity in its central engine.
Aim. We aim to better understand the different emission components by searching for correlated variability in the flux over four decades of frequency measurements.
Methods. We combined data at frequencies from the millimetric to the visible to characterise the multifrequency light curve in April and May 2010. This includes the only photometric observations of OJ 287 made with the Herschel Space Observatory: five epochs of data obtained over 33 days at 250, 350, and 500µm with Herschel-SPIRE.
Results. Although we find that the variability at 37GHz on timescales of a few weeks correlates with the visible to near-IR spectral energy distribution, there is a small degree of reddening in the continuum at lower flux levels that is revealed by the decreasing rate of decline in the light curve at lower frequencies. However, we see no clear evidence that a rapid flare detected in the light curve during our monitoring in the visible to near-IR light curve is seen either in the Herschel data or at 37GHz, suggesting a low-frequency cut-off in the spectrum of such flares.
Conclusions. We see only marginal evidence of variability in the observations with Herschel over a month, although this may be principally due to the poor sampling. The spectral energy distribution between 37GHz and the visible can be characterised by two components of approximately constant spectral index: a visible to far-IR component of spectral index α=-0.95, and a far-IR to millimetric spectral index of α=-0.43. There is no evidence of an excess of emission that would be consistent with the 60 µmdust bump found in many active galactic nuclei.

Abstract Copyright: © ESO 2018

Journal keyword(s): Galaxies - BL Lacertae objects: individual: OJ 287

VizieR on-line data: <Available at CDS (J/A+A/610/A74): photom.dat>

Status at CDS:  

Simbad objects: 6

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Number of rows : 6

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2020
#notes
1 3C 84 Sy2 03 19 48.1597607660 +41 30 42.114155434   13.10 12.48 11.09   ~ 3508 3
2 QSO J0854+2006 BLL 08 54 48.8749311881 +20 06 30.642936668   15.91 15.43 15.56   ~ 1974 1
3 M 87 BiC 12 30 49.42338230 +12 23 28.0438581 10.16 9.59 8.63   7.49 ~ 6120 3
4 3C 345 QSO 16 42 58.8100340220 +39 48 36.999540578   16.81 16.59 16.84   ~ 1541 2
5 NGC 7027 PN 21 07 01.8 +42 14 10   9.1 10.9     ~ 2312 1
6 NAME BL Lac BLL 22 02 43.2913773726 +42 16 39.978417860   15.66 14.72     ~ 1989 1

    Equat.    Gal    SGal    Ecl

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2020.04.02-12:59:52

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