Subaru Hyper Suprime-Cam excavates colossal over- and under-dense structures over 360 deg2 out to z=1
Rhythm Shimakawa, Yuichi Higuchi, Masato Shirasaki, Masayuki Tanaka,, Yen-Ting Lin, Masao Hayashi, Rieko Momose, Chien-Hsiu Lee, Haruka Kusakabe,, Tadayuki Kodama, Naoaki Yamamoto

TL;DR
This study utilizes Subaru's Hyper Suprime-Cam data to identify and analyze massive over- and under-dense cosmic structures up to redshift 1 over 360 square degrees, confirming known superclusters and discovering new colossal regions.
Contribution
It presents the first large-scale detection and characterization of extensive over- and under-dense structures at z=0.3-1 using wide-field photometric data, including weak lensing analysis.
Findings
Confirmed known superclusters
Identified new colossal over- and under-dense regions
Weak lensing signals correlate with density peaks and troughs
Abstract
Subaru Strategic Program with the Hyper-Suprime Cam (HSC-SSP) has proven to be successful with its extremely-wide area coverage in past years. Taking advantages of this feature, we report initial results from exploration and research of expansive over- and under-dense structures at 0.3-1 based on the second Public Data Release where optical 5-band photometric data for eight million sources with mag are available over square degrees. We not only confirm known superclusters but also find candidates of titanic over- and under-dense regions out to . The mock data analysis suggests that the density peaks would involve one or more massive dark matter haloes ( M) of the redshift, and the density troughs tend to be empty of massive haloes over comoving Mpc. Besides, the density peaks and troughs at are in part identified as…
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