Redshift determination of the BL Lac object 3C66A by the detection of its host galaxy cluster at $z=0.340$

Abstract

The BL Lac object 3C66A is one of the most luminous extragalactic sources at TeV $\gamma$-rays (VHE, i.e. $E>100$ GeV). Since TeV $\gamma$-ray radiation is absorbed by the extragalactic background light (EBL), it is crucial to know the redshift of the source in order to reconstruct its original spectral energy distribution, as well as to constrain EBL models. However, the optical spectrum of this BL\,Lac is almost featureless, so a direct measurement of $z$ is very difficult; in fact, the published redshift value for this source ($z=0.444$) has been strongly questioned. Based on EBL absorption arguments, several constraints to its redshift, in the range $0.096<z<0.5$, were proposed. Since these AGNs are hosted, typically, in early type galaxies that are members of groups or clusters, we have analysed spectro-photometrically the environment of 3C66A, with the goal of finding the galaxy group hosting this blazar. This study was made using optical images of a $5.5\times 5.5$\,arcmin${}^2$ field centred on the blazar, and spectra of 24 sources obtained with Gemini/GMOS-N multi-object spectroscopy. We found spectroscopic evidence of two galaxy groups along the blazar's line of sight: one at $z\simeq 0.020$ and a second one at $z\simeq 0.340$. The first one is consistent with a known foreground structure, while the second group here presented has six spectroscopically confirmed members. Their location along a red sequence in the colour-magnitude diagram allows us to identify 34 additional candidate members of the more distant group. The blazar's spectrum shows broad absorption features that we identify as arising in the intergalactic medium, thus allowing us to tentatively set a redshift lower limit at $z_{3C66A}\ge 0.33$. As a consequence, we propose that 3C66A is hosted in a galaxy that belongs to a cluster at $z=0.340$.

11 pages, 7 figures, accepted for publication in MNRAS

References in corpus (7)

• New limits on the density of the extragalactic background light in the optical to the far-infrared from the spectra of all known TeV blazars
• Constraining blazar distances with combined Fermi and TeV data: an empirical approach
• Discovery of a very high energy gamma-ray signal from the 3C 66A/B region
• Galaxy populations in the Antlia cluster. I. Photometric properties of early-type galaxies
• Spectroscopy of BL Lac objects of extraordinary luminosity
• Redshift Limits of BL Lacertae Objects from Optical Spectroscopy
• The BL-Lac gamma-ray blazar PKS 0447-439 as a probable member of a group of galaxies at z=0.343

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• Variability and evolution of the optical polarization of a sample of gamma-ray blazars