activity
20172022
most citedFirst results on the cluster galaxy population from the Subaru Hyper Suprime-Cam survey. III. Brightest cluster galaxies, stellar mass distribution, and active galaxies

45 citations · 51 across the 4 of their papers we have counts for

collaborators

5 papers

astro-ph.CO20225 cited

Strong Gravitational Lensing Parameter Estimation with Vision Transformer

Kuan-Wei Huang, Geoff Chih-Fan Chen, Po-Wen Chang +4

Quantifying the parameters and corresponding uncertainties of hundreds of strongly lensed quasar systems holds the key to resolving one of the most important scientific questions:…

astro-ph.IM20221 cited

Estimating Cluster Masses from SDSS Multi-band Images with Transfer Learning

Sheng-Chieh Lin, Yuanyuan Su, Gongbo Liang +3

The total masses of galaxy clusters characterize many aspects of astrophysics and the underlying cosmology. It is crucial to obtain reliable and accurate mass estimates for numerou…

cs.CV2020

Optical Wavelength Guided Self-Supervised Feature Learning For Galaxy Cluster Richness Estimate

Gongbo Liang, Yuanyuan Su, Sheng-Chieh Lin +3

Most galaxies in the nearby Universe are gravitationally bound to a cluster or group of galaxies. Their optical contents, such as optical richness, are crucial for understanding th…

astro-ph.GA2020

Angular clustering and host halo properties of [OII] emitters at in the Subaru HSC survey

Teppei Okumura, Masao Hayashi, I-Non Chiu +4

We study the angular correlation function of star-forming galaxies and properties of their host dark matter halos at z>1 using the Hyper-Suprime Cam (HSC) SSP survey. We use [OII]…

astro-ph.GA201745 cited

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…