We present an overview of a deep transient survey of the COSMOS field with the Subaru Hyper Suprime-Cam (HSC). The survey was performed for the 1.77 deg2 ultra-deep layer and 5.78 deg2 deep layer in the Subaru Strategic Program over 6- and 4-month periods from 2016 to 2017, respectively. The ultra-deep layer shows a median depth per epoch of 26.4, 26.3, 26.0, 25.6, and 24.6 mag in g, r, i, z, and y bands, respectively; the deep layer is ∼0.6 mag shallower. In total, 1,824 supernova candidates were identified. Based on light curve fitting and derived light curve shape parameter, we classified 433 objects as Type Ia supernovae (SNe); among these candidates, 129 objects have spectroscopic or COSMOS2015 photometric redshifts and 58 objects are located at z>1. Our unique dataset doubles the number of Type Ia SNe at z>1 and enables various time-domain analyses of Type II SNe, high redshift superluminous SNe, variable stars, and active galactic nuclei.
@article{arxiv.1904.09697,
title = {The Hyper Suprime-Cam SSP Transient Survey in COSMOS: Overview},
author = {Naoki Yasuda and Masaomi Tanaka and Nozomu Tominaga and Ji-an Jiang and Takashi J. Moriya and Tomoki Morokuma and Nao Suzuki and Ichiro Takahashi and Masaki S. Yamaguchi and Keiichi Maeda and Masao Sako and Shiro Ikeda and Akisato Kimura and Mikio Morii and Naonori Ueda and Naoki Yoshida and Chien-Hsiu Lee and Sherry H. Suyu and Yutaka Komiyama and Nicolas Regnault and David Rubin},
journal= {arXiv preprint arXiv:1904.09697},
year = {2019}
}
Comments
17 pages, 17 figures, accepted for publication in PASJ