Web of the giant: Spectroscopic confirmation of a large-scale structure around the z = 6.31 quasar SDSS J1030+0524

Marco Mignoli, Roberto Gilli, Roberto Decarli, Eros Vanzella, Barbara Balmaverde, Nico Cappelluti, Letizia P. Cassarà, Andrea Comastri, Felice Cusano, Kazushi Iwasawa, Stefano Marchesi, Isabella Prandoni, Cristian Vignali, Fabio Vito, Giovanni Zamorani, Marco Chiaberge, Colin Norman

Research output: Contribution to journalArticlepeer-review

1 Scopus citations

Abstract

We report on the spectroscopic confirmation of a large-scale structure around the luminous z = 6.31 quasi-stellar object (QSO) SDSS J1030+0524, powered by a one billion solar mass black hole. The structure is populated by at least six members, namely, four Lyman-break galaxies (LBGs), and two Lyman alpha emitters (LAEs). The four LBGs were identified among a sample of 21 i-band dropouts with zAB < 25.5 selected up to projected separations of 5 physical Mpc (15 arcmin) from the QSO. Their redshifts were determined through multi-object spectroscopic observations at 8-10 m class telescopes lasting up to eight hours. The two LAEs were identified in a 6 h VLT/MUSE observation centered on the QSO. The redshifts of the six galaxies cover the range between 6.129-6.355. Assuming that the peculiar velocities are negligible, this range corresponds to radial separations of ±5 physical Mpc from the QSO, that is comparable to the projected scale of the observed LBG distribution on the sky. We conservatively estimate that this structure is significant at a level > 3.5σ and that the level of the galaxy overdensity is at least 1.5-2 within the large volume sampled (∼780 physical Mpc3). The spectral properties of the six member galaxies (Lyα strength and UV luminosity) are similar to those of field galaxies at similar redshifts. This is the first spectroscopic identification of a galaxy overdensity around a supermassive black hole in the first billion years of the Universe. Our finding lends support to the idea that the most distant and massive black holes form and grow within massive (>1012 M) dark matter halos in large-scale structures and that the absence of earlier detections of such systems is likely due to observational limitations.

Original languageEnglish (US)
Article numberL1
JournalAstronomy and Astrophysics
Volume642
DOIs
StatePublished - Oct 1 2020

Keywords

  • Galaxies: high-redshift
  • Quasars: general
  • Quasars: individual: SDSSJ1030+0524
  • Quasars: supermassive black holes

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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