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First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. III. Brightest cluster galaxies, stellar mass distribution, and active galaxies
Yen-Ting Lin, Bau-Ching Hsieh, Sheng-Chieh Lin +12
The unprecedented depth and area surveyed by the Subaru Strategic Program with the Hyper Suprime-Cam (HSC-SSP) have enabled us to construct and publish the largest distant cluster…
Probing the kinematic morphology-density relation of early-type galaxies with MaNGA
J. E. Greene, A. Leauthaud, E. Emsellem +17
The "kinematic" morphology-density relation for early-type galaxies posits that those galaxies with low angular momentum are preferentially found in the highest-density regions of…
SDSS-IV MaNGA: Uncovering the Angular Momentum Content of Central and Satellite Early-type Galaxies
Jenny E. Greene, Alexie Leauthaud, Eric Emsellem +18
We study 379 central and 159 satellite early-type galaxies with two-dimensional kinematics from the integral-field survey Mapping Nearby Galaxies at APO (MaNGA) to determine how th…
First results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. I. The role of group or cluster environment in star formation quenching from z = 0.2 to 1.1
Hung-Yu Jian, Lihwai Lin, Masamune Oguri +6
We utilize the HSC CAMIRA cluster catalog and the photo- galaxy catalog constructed in the HSC wide field (S16A), covering 174 deg, to study the star formation acti…
GOLDRUSH. II. Clustering of Galaxies at Revealed with the Half-Million Dropouts Over the 100 deg Area Corresponding to 1 Gpc
Yuichi Harikane, Masami Ouchi, Yoshiaki Ono +15
We present clustering properties from 579,492 Lyman break galaxies (LBGs) at z~4-6 over the 100 deg^2 sky (corresponding to a 1.4 Gpc^3 volume) identified in early data of the Hype…
The FMOS-COSMOS survey of star-forming galaxies at . V: Properties of dark matter halos containing H emitting galaxies
Daichi Kashino, Surhud More, John D. Silverman +11
We study the properties of dark matter halos that contain star-forming galaxies at using the FMOS-COSMOS survey. The sample consists of 516 objects with a det…