ner_tags: O O O O O O O O O O O O O O O O B-ComputingFacility I-ComputingFacility O B-ComputingFacility O O B-ComputingFacility I-ComputingFacility I-ComputingFacility I-ComputingFacility B-Observatory I-Observatory I-Observatory I-Observatory I-Observatory O O B-ComputingFacility O O B-ComputingFacility I-ComputingFacility B-Organization I-Organization O O O O O O O O B-Organization B-Grant I-Grant I-Grant I-Grant B-Person B-Grant B-Person O B-Grant B-Person B-Person O O O B-Organization I-Organization I-Organization O O B-Grant O B-Grant O O O O B-Person I-Person O O O O O O O B-Person O O B-Person I-Person O O O O O O O B-Person O O O O O O B-Organization I-Organization B-Grant I-Grant I-Grant I-Grant I-Grant B-Grant O O O O O O O
tokens: ACKNOWLEDGEMENTS We thank the referee for the constructive comments. Numerical computations were carried out on the Cray XC30 and XC50 at the Center for Computational Astrophysics, National Astronomical Observatory of Japan, and the octopus at the Cybermedia Center, Osaka University. This work is supported in part by the MEXT/JSPS KAKENHI Grant Number JP17H04827 (HY), 18H04570 (HY), and JP17H01111 (KN). YL acknowledges support from National Science Foundation through grants AST-1412719 and MRI-1626251. We are grateful to Dr. Ouchi for helpful comments on the dust temperature. KN thanks to Dr. Kawamata for useful discussions on galaxy size evolution. KN acknowledges the travel support from the Kavli IPMU, World Premier Research Center Initiative (WPI), where part of this work was conducted.