木曾超新星巡天 (KISS)：巡天策略
太阳与恒星天体物理
2015-06-22 v1 高能天体物理现象
摘要
木曾超新星巡天 (KISS) 是一项高时间分辨率的光学广域超新星 (SN) 巡天。该巡天的主要目标是捕捉超新星在激波爆发阶段的极早期光线。将超新星激波爆发的探测与其他设施获得的多波段测光相结合，可提供关于超新星前身星的详细物理信息。该巡天使用安装在 1.05 米木曾施密特望远镜上的 2.2x2.2 度视场仪器——木曾广域相机 (KWFC) 进行。我们在巡天中每小时进行一次 g 波段三分钟曝光，极限星等达到 g~20-21。自 2012 年 4 月以来，每年约有 100 个晚上的望远镜时间用于该巡天。在我们为期 3 年的项目中，预计激波爆发探测数量约为 1 次。本文总结了 KISS 项目，包括 KWFC 观测设置、巡天策略、数据还原系统以及迄今为止由 KISS 发现并已报告给 CBET 的超新星。
引用
@article{arxiv.1409.1308,
title = {Kiso Supernova Survey (KISS): Survey Strategy},
author = {Tomoki Morokuma and Nozomu Tominaga and Masaomi Tanaka and Kensho Mori and Emiko Matsumoto and Yuki Kikuchi and Takumi Shibata and Shigeyuki Sako and Tsutomu Aoki and Mamoru Doi and Naoto Kobayashi and Hiroyuki Maehara and Noriyuki Matsunaga and Hiroyuki Mito and Takashi Miyata and Yoshikazu Nakada and Takao Soyano and Ken'ichi Tarusawa and Satoshi Miyazaki and Fumiaki Nakata and Norio Okada and Yuki Sarugaku and Michael W. Richmond and Hiroshi Akitaya and Greg Aldering and Ko Arimatsu and Carlos Contreras and Takashi Horiuchi and Eric Y. Hsiao and Ryosuke Itoh and Ikuru Iwata and Koji and S. Kawabata and Nobuyuki Kawai and Yutaro Kitagawa and Mitsuru Kokubo and Daisuke Kuroda and Paolo and Mazzali and Toru Misawa and Yuki Moritani and Nidia Morrell and Rina Okamoto and Nikolay Pavlyuk and Mark M. Phillips and Elena Pian and Devendra Sahu and Yoshihiko Saito and Kei Sano and Maximilian D. Stritzinger and Yutaro Tachibana and Francesco Taddia and Katsutoshi Takaki and Ken Tateuchi and Akihiko Tomita and Dmitry Tsvetkov and Takahiro Ui and Nobuharu Ukita and Yuji Urata and Emma S. Walker and Taketoshi Yoshii},
journal= {arXiv preprint arXiv:1409.1308},
year = {2015}
}
备注
13 pages, 10 figures, 3 tables. Publications of the Astronomical Society of Japan (PASJ) in press