Lyα view around a z = 2.84 hyperluminous QSO at a node of the cosmic web†. (5th June 2019)

• Record Type: Journal Article
• Authors: Kikuta, Satoshi; Matsuda, Yuichi; Cen, Renyue; Steidel, Charles C; Yagi, Masafumi; Hayashino, Tomoki; Imanishi, Masatoshi; Komiyama, Yutaka; Momose, Rieko; Saito, Tomoki
• Is Part Of: Publications of the Astronomical Society of Japan. Volume 71:Number 3(2019:Jun.)
• Publication Date: 2019-06-05
• Subjects: galaxies: formation -- galaxies: high-redshift -- intergalactic medium -- quasars: individual (HS 1549+1919); Astronomy -- Periodicals; 520.5
• DOI: 10.1093/pasj/psz055
• Languages: English
• ISSNs: 0004-6264

Abstract

Abstract: We report on the results of deep and wide-field (1.1 deg 2 ) narrow-band observations with Subaru/Hyper Suprime-Cam (HSC) of a field around a hyperluminous QSO (HLQSO), HS$\, 1549+$ 1919, residing in a protocluster at z = 2.84, to map the large-scale structure of Lyα emitters (LAEs). One HSC pointing enables us to detect 3490 LAEs and 76 extended Lyα blobs (LABs), probing diverse environments from voids to protoclusters. The HLQSO is found to be near the center of the protocluster, which corresponds to the intersection of $\sim \, $ 100 comoving Mpc-scale structures of LAEs. LABs are basically distributed along the large-scale structure, with larger ones particularly clustering around the HLQSO, confirming a previously noted tendency of LABs to prefer denser environments. Moreover, the shapes of LABs near the HLQSO appear to be aligned with the large-scale structure. Finally, a deep Lyα image reveals a diffuse Lyα nebula along a filamentary structure with no luminous UV/sub-mm counterpart. We suggest that the diffuse nebula is due to a cold filament with high clumping factor illuminated by the QSO, with the required high clumpiness provided by unresolved residing halos of mass $\le 10^{9-10}\, M_\odot$ .