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CLOSE COMPANIONS TO TWO HIGH-REDSHIFT QUASARS
Journal article   Open access

CLOSE COMPANIONS TO TWO HIGH-REDSHIFT QUASARS

Ian D. McGreer, Xiaohui Fan, Michael A. Strauss, Zoltan Haiman, Gordon T. Richards, Linhua Jiang, Fuyan Bian and Donald P. Schneider
The Astronomical journal, v 148(4), pp 1-12
01 Oct 2014
url
http://arxiv.org/abs/1404.2297View
Submitted Open

Abstract

Astronomy & Astrophysics Physical Sciences Science & Technology
We report the serendipitous discoveries of companion galaxies to two high-redshift quasars. SDSS J025617.7+001904 is a z = 4.79 quasar included in our recent survey of faint quasars in the SDSS Stripe 82 region. The initial MMT slit spectroscopy shows excess Ly alpha emission extending well beyond the quasar's light profile. Further imaging and spectroscopy with LBT/MODS1 confirms the presence of a bright galaxy (i(AB) = 23.6) located 2 '' (12 kpc projected) from the quasar with strong Ly alpha emission (EW0 approximate to 100 angstrom) at the redshift of the quasar, as well as faint continuum. The second quasar, CFHQS J005006.6+344522 (z = 6.25), is included in our recent HST SNAP survey of z similar to 6 quasars searching for evidence of gravitational lensing. Deep imaging with ACS and WFC3 confirms an optical dropout similar to 4.5 mag fainter than the quasar (Y-AB = 25) at a separation of 0 ''.9. The red i(775)-Y-105 color of the galaxy and its proximity to the quasar (5 kpc projected if at the quasar redshift) strongly favor an association with the quasar. Although it is much fainter than the quasar, it is remarkably bright when compared to field galaxies at this redshift, while showing no evidence for lensing. Both systems may represent late-stage mergers of two massive galaxies, with the observed light for one dominated by powerful ongoing star formation and for the other by rapid black hole growth. Observations of close companions are rare; if major mergers are primarily responsible for high-redshift quasar fueling then the phase when progenitor galaxies can be observed as bright companions is relatively short.

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