Spectroscopic confirmation of a galaxy cluster associated with 7C1756+6520 at z=1.416
Audrey Galametz, Daniel Stern, S. Adam Stanford, Carlos De Breuck,, Joel Vernet, Roger L. Griffith, Fiona A. Harrison

TL;DR
This study spectroscopically confirms a galaxy cluster at z=1.416 associated with the radio galaxy 7C1756+6520, demonstrating the effectiveness of BzK selection criteria and revealing detailed structure at high redshift.
Contribution
The paper provides the first spectroscopic confirmation of a galaxy cluster at z=1.416 associated with a radio galaxy, validating BzK selection and revealing the cluster's detailed structure.
Findings
Confirmed a galaxy cluster at z=1.416 near 7C1756+6520
Demonstrated robustness of BzK criteria at moderate redshifts
Identified a secondary galaxy group at z~1.437
Abstract
We present spectroscopic follow-up of an overdensity of galaxies photometrically selected to be at 1.4<z<2.5 found in the vicinity of the radio galaxy 7C1756+6520 at z=1.4156. Using the DEIMOS optical multi-object spectrograph on the Keck 2 telescope, we observed a total of 129 BzK-selected sources, comprising 82 blue, star-forming galaxy candidates (sBzK) and 47 red, passively-evolving galaxy candidates (pBzK*), as well as 11 mid-infrared selected AGN candidates. We obtain robust spectroscopic redshifts for 36 blue galaxies, 7 red galaxies and 9 AGN candidates. Assuming all foreground interlopers were identified, we find that only 16% (9%) of the sBzK (pBzK*) galaxies are at z<1.4. Therefore, the BzK criteria are shown to be relatively robust at identifying galaxies at moderate redshifts. Twenty-one galaxies, including the radio galaxy, four additional AGN candidates and three red…
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