NuSTAR Detection of the Blazar B2 1023+25 at Redshift 5.3

T. Sbarrato, G. Tagliaferri, G. Ghisellini, M. Perri, S. Puccetti, M. Balokovi, M. Nardini, D. Stern, S.~E. Boggs, W.~N. Brandt, F.~E. Christensen, P. Giommi, J. Greiner, C.~J. Hailey, F.~A. Harrison, T. Hovatta, G.~M. Madejski, A. Rau, P. Schady, V. SudilovskyC.~M. Urry, W.~W. Zhang

Research output: Contribution to journalArticlepeer-review

31 Citations (Scopus)

Abstract

B2 1023+25 is an extremely radio-loud quasar at z = 5.3 that was first identified as a likely high-redshift blazar candidate in the SDSS+FIRST quasar catalog. Here, we use the Nuclear Spectroscopic Telescope Array (NuSTAR) to investigate its non-thermal jet emission, whose high-energy component we detected in the hard X-ray energy band. The X-ray flux is (5-10 keV) and the photon spectral index is ΓX 1.3-1.6. Modeling the full spectral energy distribution, we find that the jet is oriented close to the line of sight, with a viewing angle of ~3°, and has significant Doppler boosting, with a large bulk Lorentz factor ~13, which confirms the identification of B2 1023+25 as a blazar. B2 1023+25 is the first object at redshift larger than 5 detected by NuSTAR, demonstrating the ability of NuSTAR to investigate the early X-ray universe and to study extremely active supermassive black holes located at very high redshift.
Original languageEnglish
Pages (from-to)147
Number of pages1
JournalAstrophysical Journal
Volume777
Issue number2
DOIs
Publication statusPublished - 23 Oct 2013

Keywords

  • galaxies: active, quasars: general, quasars: individual: B2 1023+25, X-rays: general, Astrophysics - Cosmology and Nongalactic Astrophysics, Astrophysics - High Energy Astrophysical Phenomena

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