arXiv · 0911.1258
Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae
Abstract
We present spectra of high-redshift supernovae (SNe) that were taken with the Subaru low resolution optical spectrograph, FOCAS. These SNe were found in SN surveys with Suprime-Cam on Subaru, the CFH12k camera on the Canada-France-Hawaii Telescope (CFHT), and the Advanced Camera for Surveys (ACS) on the Hubble Space Telescope (HST). These SN surveys specifically targeted z>1 Type Ia supernovae (SNe Ia). From the spectra of 39 candidates, we obtain redshifts for 32 candidates and spectroscopically identify 7 active candidates as probable SNe Ia, including one at z=1.35, which is the most distant SN Ia to be spectroscopically confirmed with a ground-based telescope. An additional 4 candidates are identified as likely SNe Ia from the spectrophotometric properties of their host galaxies. Seven candidates are not SNe Ia, either being SNe of another type or active galactic nuclei. When SNe Ia are observed within a week of maximum light, we find that we can spectroscopically identify most of them up to z=1.1. Beyond this redshift, very few candidates were spectroscopically identified as SNe Ia. The current generation of super red-sensitive, fringe-free CCDs will push this redshift limit higher.
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Tomoki Morokuma, Kouichi Tokita, Christopher Lidman, Mamoru Doi, Naoki Yasuda, Greg Aldering, Rahman Amanullah, Kyle Barbary, Kyle Dawson, Vitaliy Fadeyev, Hannah K. Fakhouri, Gerson Goldhaber, Ariel Goobar, Takashi Hattori, Junji Hayano, Isobel M. Hook, D. Andrew Howell, Hisanori Furusawa, Yutaka Ihara, Nobunari Kashikawa, Rob A. Knop, Kohki Konishi, Joshua Meyers, Takeshi Oda, Reynald Pain, Saul Perlmutter, David Rubin, Anthony L. Spadafora, Nao Suzuki, Naohiro Takanashi, Tomonori Totani, Hiroyuki Utsunomiya, Lifan Wang. 2009-11-06. Subaru FOCAS Spectroscopic Observations of High-Redshift Supernovae. https://doi.org/10.1093/pasj%2F62.1.19
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