The redshift and the host galaxy of the neutrino candidate 4FGL J0955.1+3551 (3HSP J095507.9+355101)
arXiv:2003.03634 · doi:10.1093/mnrasl/slaa056
Abstract
The BL Lac object 4FGLJ0955.1+3551 has been suggested as a possible source of ultra energetic neutrinos detected by the Icecube observatory. The target was observed in January 2020 at the Large Binocular Telescope. Our spectroscopy (4100-8500 Ang) yields a firm redshift z = 0.557 as deduced by the absorption lines of the host galaxy. The upper limit of the minimum equivalent width on emission lines is 0.3 Ang. From the source image we are able to resolve the host galaxy for which we measure an absolute magnitude M(R) = -22.9 and Re = 8 kpc, that is values which are typical of the host galaxies of BL Lacs.
4 pages, 4 figures, accepted to MNRAS
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Cited by in corpus (8)
- 3HSP J095507.9+355101: a flaring extreme blazar coincident in space and time with IceCube-200107A
- Time-dependent lepto-hadronic modeling of the emission from blazar jets with SOPRANO: the case of TXS 0506+056, 3HSP J095507.9+355101 and 3C 279
- A two-zone blazar radiation model for "orphan" neutrino flares
- Comprehensive Multimessenger Modeling of the Extreme Blazar 3HSP J095507.9+355101 and Predictions for IceCube
- The Spectra of IceCube Neutrino (SIN) candidate sources -- II. Source Characterisation
- LeHaMoC: a versatile time-dependent lepto-hadronic modeling code for high-energy astrophysical sources
- Hadronic X-ray Flares from Blazars
- The spectra of IceCube neutrino candidate sources -- I. Optical spectroscopy of blazars