천문학회지 (Journal of The Korean Astronomical Society)

  • 제44권4호
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  • Pages.115-123
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  • 2011
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  • 1225-4614(pISSN)
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  • 2288-890X(eISSN)
한국천문학회 (The Korean Astronomical Society)
권호 표지
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AUTO-GUIDING SYSTEM FOR CQUEAN (CAMERA FOR QUASARS IN EARLY UNIVERSE)

  • Kim, Eun-Bin (School of Space Research, Kyung Hee University) ;
  • Park, Won-Kee (CEOU/Dept. of Physics and Astronomy, Seoul National University) ;
  • Jeong, Hyeon-Ju (School of Space Research, Kyung Hee University) ;
  • Kim, Jin-Young (School of Space Research, Kyung Hee University) ;
  • Kuehne, John (McDonald Observatory, Univ. of Texas at Austin) ;
  • Kim, Dong-Han (Department of Electrical Engineering, Kyung Hee University) ;
  • Kim, Han-Geun (Department of Electrical Engineering, Kyung Hee University) ;
  • Odoms, Peter S. (McDonald Observatory, Univ. of Texas at Austin) ;
  • Chang, Seung-Hyuk (Samsung Electronics) ;
  • Im, Myung-Shin (CEOU/Dept. of Physics and Astronomy, Seoul National University) ;
  • Pak, Soo-Jong (School of Space Research, Kyung Hee University)
  • 투고 : 2011.01.07
  • 심사 : 2011.07.20
  • 발행 : 2011.08.31
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초록

To perform imaging observations of optically red objects such as high redshift quasars and brown dwarfs, the Center for the Exploration of the Origin of the Universe (CEOU) recently developed an optical CCD camera, Camera for QUasars in EArly uNiverse (CQUEAN), which is sensitive at 0.7-1.1 ${\mu}m$. To enable observations with long exposures, we develop an auto-guiding system for CQUEAN. This system consists of an off-axis mirror, a baffle, a CCD camera, a motor and a differential decelerator. To increase the number of available guiding stars, we design a rotating mechanism for the off-axis guiding camera. The guiding field can be scanned along the 10 arcmin ring offset from the optical axis of the telescope. Combined with the auto-guiding software of the McDonald Observatory, we confirm that a stable image can be obtained with an exposure time as long as 1200 seconds.

키워드

참고문헌

  1. Abbott, T. 1990, An Off-the-Shelf Autoguider for Mc- Donald Observatory, Proc. SPIE, 1235, 770 https://doi.org/10.1117/12.19141
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  6. Iseki, A., Tomono, D., Tajitsu, A., Itoh, N. & Miki, S. 2008, Improved Guiding Accuracy through Silt Viewer of Subaru Telescope, Proc. SPIE, 7019, 70192D-1
  7. Jeong, W., Lee, S. -G., & Pak, S. 1999, Development of Control Software for Improvement of Tracking Efficiency of the 1600 telescope of Seoul National University Observatory, PKAS, 14, 47
  8. Kanzawa, T., Tomono, D., Usua, T., Takato, N., Negishi, S., Sugahara, S. & Itoh, N. 2006, Improvement of the Pointing Accuracy of the Subaru Telescope by Suppressing Vibrations, Proc. SPIE, 6267, 62673J-1
  9. Lee, J. H. 2007, Discrete Time Dynamic Model for Telescope Auto-Guiding System, JA&SS, 24, 431
  10. Mun, B.-S, Kim, S.-J., Jang, M., Min, S.-W., Seol, K.-H., & Moon, K.-S. 2006, Development of the Software for 30 Inch Telescope Control System at KHAO, PKAS, 21, 81
  11. Park, W.-K., Jeong, H., Kim, J., Jeon, Y., Choi, C., Lim, J., Kim, E., Pak, S., & Im, M. 2011, in preparation
  12. Yoon, J.-N., Lee, C.-U., Cha, S.-M., & Kim, Y. 2006, A Construction of an Automatic Observation System for Bright and Long Period Variable Stars, JA&SS, 23, 143

피인용 문헌

  1. FOCAL REDUCER FOR CQUEAN (Camera for QUasars in EArly uNiverse) vol.46, pp.4, 2013, https://doi.org/10.5303/JKAS.2013.46.4.161
  2. Camera for Quasars in Early Universe (CQUEAN)1 vol.124, pp.918, 2012, https://doi.org/10.1086/667390
  3. VARIABILITY AT THE EDGE: OPTICAL NEAR/IR RAPID-CADENCE MONITORING OF NEWLY OUTBURSTING FU ORIONIS OBJECT HBC 722 vol.764, pp.1, 2013, https://doi.org/10.1088/0004-637X/764/1/22
  4. COLOR VARIABILITY OF HBC 722 IN THE POST-OUTBURST PHASES vol.149, pp.2, 2015, https://doi.org/10.1088/0004-6256/149/2/73
  5. HOST GALAXY PROPERTIES AND BLACK HOLE MASS OF SWIFT J164449.3+573451 FROM MULTI-WAVELENGTH LONG-TERM MONITORING ANDHSTDATA vol.808, pp.1, 2015, https://doi.org/10.1088/0004-637X/808/1/96
  6. CORRELATION BETWEEN GALAXY MERGERS AND LUMINOUS ACTIVE GALACTIC NUCLEI vol.804, pp.1, 2015, https://doi.org/10.1088/0004-637X/804/1/34
  7. The Infrared Medium-deep Survey. III. Survey of Luminous Quasars at 4.7 ≤ z ≤ 5.4 vol.231, pp.2, 2017, https://doi.org/10.3847/1538-4365/aa7de5
  8. SYNCHROTRON SELF-INVERSE COMPTON RADIATION FROM REVERSE SHOCK ON GRB 120326A vol.789, pp.2, 2014, https://doi.org/10.1088/0004-637X/789/2/146
  9. Development of SED Camera for Quasars in Early Universe (SQUEAN) vol.128, pp.969, 2016, https://doi.org/10.1088/1538-3873/128/969/115004
  10. ∼ 5 with a Medium-band-based Approach vol.870, pp.2, 2019, https://doi.org/10.3847/1538-4357/aaf387