We have been performing a wide-field photometric monitoring program, named SPVS (Short-Period Variability Survey), at the Bohyunsan Optical Astronomy Observatory (BOAO). The observation system consists of a small refracting telescope (D = 155 mm, f = 1050 mm) and a 2k×3k CCD Camera. The field of view is 1.0°×1.5°. Detection limit is about V = 13 for short-period small amplitude variables such as δ Scuti-type pulsating stars, and about V = 15 for long-period large amplitude variables such as eclipsing binaries and RR Lyrae stars. The instrument is designed to be remote-controlled through internet. The primary purpose of this project is to search for variable objects in bright Galactic open clusters. We present results of test observations conducted towards NGC 7092.

• 전영범(한국천문연구원) | YOUNG-BEOM JEON (Korea Astronomy and Space Science Institute)
• 김승리(한국천문연구원) | SEUNG-LEE KIM (Korea Astronomy and Space Science Institute)
• 박윤호(한국천문연구원) | YOON-HO PARK (Korea Astronomy and Space Science Institute)
• 박병곤(한국천문연구원) | BYEONG-GON PARK (Korea Astronomy and Space Science Institute)
• 이충욱(한국천문연구원) | CHUNG-UK LEE (Korea Astronomy and Space Science Institute)
• 이은정(한국천문연구원, 한국교원대학교) | EUN-JEONG LEE (Korea Astronomy and Space Science Institute, Korea National University of Education)
• 김민수(한국천문연구원) | MIN-SU KIM (Korea Astronomy and Space Science Institute)
• 이경훈(한국과학영재학교) | KYUNG-HOON LEE (Korea Science Academy)