TY - JOUR
T1 - Organized autotelescopes for serendipitous event survey (OASES)
T2 - Design and performance
AU - Arimatsu, Ko
AU - Tsumura, Kohji
AU - Ichikawa, Kohei
AU - Usui, Fumihiko
AU - Ootsubo, Takafumi
AU - Kotani, Takayuki
AU - Sarugaku, Yuki
AU - Wada, Takehiko
AU - Nagase, Koichi
AU - Watanabe, Junichi I.
N1 - Funding Information:
We thank the personnel of Miyakojima City Museum and of Miyako open-air school (Miyako Seishonen no Ie) for cooperating on the OASES observations at Miyako Island. We also thank the people of Miyako Island for supporting our observations. We appreciate Dr. Matthew Lehner for his thorough review and constructive comments. This research has been partly supported by JSPS grants (JP26247074, 15J10278, 26800112, and 16K17796).
Publisher Copyright:
© The Authors 2017. Published by Oxford University Press on behalf of the Astronomical Society of Japan. All rights reserved.
PY - 2017/8/1
Y1 - 2017/8/1
N2 - Organized Autotelescopes for Serendipitous Event Survey (OASES) is an optical observation project that aims to detect and investigate stellar occultation events by kilometer-sized trans-Neptunian objects (TNOs). In this project, multiple low-cost observation systems for wide-field and high-speed photometry were developed in order to detect rare and short-timescale stellar occultation events. The observation system consists of commercial off-the-shelf 0.28 m aperture f/1.58 optics providing a 2◦.3 × 1◦.8 field of view. A commercial CMOS camera is coupled to the optics to obtain full-frame imaging with a frame rate greater than 10 Hz. As of 2016 September, this project exploits two observation systems, which are installed on Miyako Island, Okinawa, Japan. Recent improvements in CMOS technology in terms of high-speed imaging and low readout noise mean that the observation systems are capable of monitoring ∼2000 stars in the Galactic plane simultaneously with magnitudes down to V ∼ 13.0, providing ∼20% photometric precision in light curves with a sampling cadence of 15.4 Hz. This number of monitored stars is larger than for any other existing instruments for coordinated occultation surveys. In addition, a precise time synchronization method needed for simultaneous occultation detection is developed using faint meteors. The two OASES observation systems are executing coordinated monitoring observations of a dense stellar field in order to detect occultations by kilometer-sized TNOs for the first time.
AB - Organized Autotelescopes for Serendipitous Event Survey (OASES) is an optical observation project that aims to detect and investigate stellar occultation events by kilometer-sized trans-Neptunian objects (TNOs). In this project, multiple low-cost observation systems for wide-field and high-speed photometry were developed in order to detect rare and short-timescale stellar occultation events. The observation system consists of commercial off-the-shelf 0.28 m aperture f/1.58 optics providing a 2◦.3 × 1◦.8 field of view. A commercial CMOS camera is coupled to the optics to obtain full-frame imaging with a frame rate greater than 10 Hz. As of 2016 September, this project exploits two observation systems, which are installed on Miyako Island, Okinawa, Japan. Recent improvements in CMOS technology in terms of high-speed imaging and low readout noise mean that the observation systems are capable of monitoring ∼2000 stars in the Galactic plane simultaneously with magnitudes down to V ∼ 13.0, providing ∼20% photometric precision in light curves with a sampling cadence of 15.4 Hz. This number of monitored stars is larger than for any other existing instruments for coordinated occultation surveys. In addition, a precise time synchronization method needed for simultaneous occultation detection is developed using faint meteors. The two OASES observation systems are executing coordinated monitoring observations of a dense stellar field in order to detect occultations by kilometer-sized TNOs for the first time.
KW - Instrumentation: detectors
KW - Kuiper belt: general
KW - Methods: observational
KW - Occultations
UR - http://www.scopus.com/inward/record.url?scp=85031915578&partnerID=8YFLogxK
UR - http://www.scopus.com/inward/citedby.url?scp=85031915578&partnerID=8YFLogxK
U2 - 10.1093/pasj/psx048
DO - 10.1093/pasj/psx048
M3 - Article
AN - SCOPUS:85031915578
SN - 0004-6264
VL - 69
JO - Publication of the Astronomical Society of Japan
JF - Publication of the Astronomical Society of Japan
IS - 4
M1 - 68
ER -