AzTEC 1.1 mm observations of high-z protocluster environments : SMG overdensities and misalignment between AGN jets and SMG distribution

M. Zeballos,Itziar Aretxaga,Deborah Hughes,A. Humphrey,Grant W. Wilson,Jason Austermann,James Dunlop,H. Ezawa,D. Ferrusca,Bunyo Hatsukade,Rob Ivison,Ryohei Kawabe,Sungeun Kim,Tadayuki Kodama,Kotaro Kohno,A Montana,Koichiro Nakanishi,Manolis Plionis,D. Sánchez-Argüelles,J. A. Stevens,Yoichi Tamura,M. Velazquez,Min S. Yun

AzTEC 1.1 mm observations of high-z protocluster environments : SMG overdensities and misalignment between AGN jets and SMG distribution

2018

We present observations at 1.1 mm towards 16 powerful radio galaxies and a radio-quiet quasar at 0.5square degrees with rms depths of 0.52 - 1.44 mJy and detects 728 sources above 3sigma. We find overdensities of a factor of ~2 in the source counts of 3 individual fields (4C+23.56, PKS1138-262 and MRC0355-037) over areas of ~200 sq deg. When combining all fields, the source-count analysis finds an overdensity that reaches a factor $\gtrsim 3$ at S$_{\rm{1.1mm}} \ge 4$ mJy covering a 1.5-arcmin-radius area centred on the AGN. The large size of our maps allows us to establish that beyond a radius of 1.5 arcmin, the radial surface density of SMGs falls to that of a blank field. In addition, we find a trend for SMGs to align closely to a perpendicular direction with respect to the radio jets of the powerful central radio galaxies (73$_{+13}^{-14}$ degrees). This misalignment is found over projected co-moving scales of 4-20 Mpc, departs from perfect alignment (0 deg) by ~5sigma, and apparently has no dependence on SMG luminosity. Under the assumption that the AzTEC sources are at the redshift of the central radio galaxy, the misalignment reported here can be interpreted as SMGs preferentially inhabiting mass-dominant filaments funneling material towards the protoclusters, which are also the parent structures of the radio galaxies.

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