68 citations · 144 across the 5 of their papers we have counts for
7 papers
Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ~ 4
Hisakazu Uchiyama, Masayuki Akiyama, Jun Toshikawa +16
Characterizing high-z quasar environments is key to understanding the co-evolution of quasars and the surrounding galaxies. To restrict their global picture, we statistically exami…
The Subaru HSC Galaxy Clustering with Photometric Redshift I: Dark Halo Masses Versus Baryonic Properties of Galaxies at 0.3<z<1.4
Shogo Ishikawa, Nobunari Kashikawa, Masayuki Tanaka +8
We present the clustering properties of low- galaxies selected by the Hyper Suprime-Cam Subaru Strategic Program Wide layer over deg. The wide-field and…
Discovery of Protoclusters at z~3.7 & 4.9: Embedded in Primordial Superclusters
Jun Toshikawa, Matthew A. Malkan, Nobunari Kashikawa +5
We have carried out follow-up spectroscopy on three overdense regions of - and -dropout galaxies in the Canada-France-Hawaii Telescope Legacy Survey Deep Fields, finding two…
The brightest UV-selected galaxies in protoclusters at : Ancestors of Brightest Cluster Galaxies?
Kei Ito, Nobunari Kashikawa, Jun Toshikawa +13
We present the results of a survey of the brightest UV-selected galaxies in protoclusters. These proto-brightest cluster galaxy (proto-BCG) candidates are drawn from 179 overdense…
Suppression of Low-mass Galaxy Formation around Quasars at z~2-3
H. Uchiyama, N. Kashikawa, R. Overzier +7
We have carried out deep and wide field imaging observations with narrow bands targeting 11 quasar fields to systematically study the possible photoevaporation effect of quasar rad…
Lyman-Break Galaxies at in the Subaru Deep Field: Luminosity Function, Clustering and [OIII] Emission
Matthew A. Malkan, Daniel P. Cohen, Miyoko Maruyama +6
We combined deep U-band imaging from the KPNO-4m/MOSAIC camera with very deep multi-waveband data from the optical to infrared, to select Lyman Break Galaxies (LBGs) at z~3 using U…