2022PASJ...74L..27U


Query : 2022PASJ...74L..27U

2022PASJ...74L..27U - Publ. Astron. Soc. Jap., 74, L27-L32 (2022/February-1)

A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). IX. The most overdense region at z ∼ 5 inhabited by a massive radio galaxy.

UCHIYAMA H., YAMASHITA T., NAGAO T., ONO Y., TOSHIKAWA J., ICHIKAWA K., KAWAKATU N., KAJISAWA M., TOBA Y., MATSUOKA Y., KUBO M., IMANISHI M., ITO K., KAWAGUCHI T., LEE C.-H. and SAITO T.

Abstract (from CDS):

We report on the galaxy density environment around a high-z radio galaxy (HzRG) at z = 4.72, HSC J083913.17+011308.1 (HSC J0839+0113), probed using an r-dropout Lyman break galaxy (LBG) sample from the Hyper Suprime-Cam Subaru Strategic Program data. We find that HSC J0839+0113 resides in the outskirts of an overdense region identified by the r-dropout galaxies at a 4.7σ significance level. The projected distance between HSC J0839+0113 and the peak position of the overdense region is 0.4 physical Mpc, which is shorter than the typical protocluster radius in this epoch. According to the extended Press-Schechter and the light cone models, the HSC J0839+0113-hosted overdense region is expected to evolve into a halo >1014 ${M_{\odot}}$ at z = 0 with a high probability of $>\!\! 80\%$. These findings suggest that HSC J0839+0113 is associated with a protocluster. The HSC J0839+0113 rich-system is the most overdense region of LBGs among the known protoclusters with LBGs in the same cosmic epoch.

Abstract Copyright: © The Author(s) 2022. Published by Oxford University Press on behalf of the Astronomical Society of Japan.

Journal keyword(s): galaxies: active - galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: jets

Simbad objects: 3

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Number of rows : 3
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 NVSS J083913+011308 rG 08 39 13.170 +01 13 08.37           ~ 4 1
2 GLEAM J092419-220140 QSO 09 24 19.92000 -22 01 41.4984       25.850   ~ 90 1
3 COSMOS2015 245166 G 09 58 58.270 +01 39 20.19           ~ 13 0

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