• 천문학논총
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• 제15권spc1호
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• pp.119-126
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• 2000

The BOES (BOAO Echelle Spectrograph), a fiber-fed echelle spectrograph of the BOAO 1.8 m telescope, has been designed and now is being manufactured. The BOES follows a white pupil design collimated with two off-axis parabolic mirrors. The 136mm collimating beam leaving the 41.59 grooves/mm R4 echelle grating is refocused near the narrow folding mirror. Through the two cross-disperser prisms and $\phi250 mm(f/1.5)$ transmission camera, the beam images on EEV $2k\times4k$ CCD. The BOES can take the wavelength range of 3700 to $10100{\AA}$ at a single spot with spectral resolution R = 20000 to 40000 depending on the fiber set employed. We describe the key sciences and performance, current status of construction, and future plan of the BOES.

• 천문학회지
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• 제35권4호
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• pp.221-227
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• 2002

Cassegrain interface module (CIM) of the fiber-fed high resolution echelle spectrograph has been designed and manufactured for the 1.8 m reflector at the Bohynsan Optical Astronomy Observatory. We also constructed a long slit spectrograph attached to this CIM, which would replace the earlier rather inefficient medium dispersion spectrometer. We present detailed description for design and manufacturing concepts of the CIM which consists of a slit assembly, slit monitoring system, calibration lamp system and a long slit spectrograph, in order to provide how the overall system and each part. are constructed. The preliminary performance test carried out so far seems to indicate a successful result.

• 천문학회보
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• 제43권1호
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• pp.50.1-50.1
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• 2018

We present the development of tools for Echelle spectrograph of NYSC 1-m telescope. The eShel spectrograph(Shelyak) has operated at Deokheung Optical Astronomy Observatory since 2016. We carried out test observation in 2016 and completed the preprocessing and wavelength calibration of the spectroscopic data using IRAF. Based on the reduction process in IRAF, PySpecW, a set of tools for spectroscopic data was developed in 2017. PySpecW was optimized for NYSC 1m telescope, and written in Python for youth to use easily on any OS. PySpecW consists of preprocessing, aperture tracing, aperture extraction, wavelength calibration, and dispersion correction for extracted spectra.

• 천문학회보
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• 제27권2호
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• pp.25-25
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• 2002

• 한국지구과학회지
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• 제33권7호
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• pp.608-617
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• 2012

분해능이 ${\Delta}{\lambda}{\sim}-0.1{\AA}$인 고분산 분광기를 사용하여 공생별 Z Andromedae (And)의 분광자료를 연구하였다. 분광 관측은 (1) 2001년 8월 30일(위상 ${\Phi}$=0.77)과 2002년 8월 12일(위상 ${\Phi}$ =0.22)에 Lick 천문대의 Hamilton Echelle Spectrograph (HES)를 사용하여, 1800초와 3600초 노출의 고분산 자료를 얻었으며, (2) 2009년 10월 21일(위상 ${\Phi}$=0.70)에는 보현산 천문대의 Bohyunsan Echelle Spectrograph (BOES)를 사용하여 1200초 노출 시간의 고분산 자료를 얻었다. 약 $3600{\AA}-9500{\AA}$파장대의 HES와 BOES 관측 자료로 부터 HI, HeI, HeII에 대한 방출선을 선택하여 분석하였다. 이 선들의 선 윤곽 분석 작업을 통해 2개 또는 3개로 분리시키고, 위상별로 각 성분이 어떤 지역에서 형성되고, 백색왜성과 적색거성의 궤도 운동과 어떠한 관련이 있는지를 조사하였다. 라만 산란(Raman scattering)된 $H{\alpha}$선 선폭 및 HI, HeI, HeII의 위상별 변화를 보이는 방출선의 특성으로부터, 방출선들은 백색왜성 주위를 감싸는 강착원반과 이 원반 안의 두 라그랑지안(Lagrangian) 포인트 $L_1$과 $L_2$지역에서 주로 생성된 것으로 결론지었다. Z And는 활동성이 2009년과 2001년에 가장 활발했고, 2002년의 선 윤곽은 매우 복잡한 양상을 보임에도 불구하고, 활동성은 비교적 조용하였음을 암시하고 있다.

• 한국광학회:학술대회논문집
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• 한국광학회 2004년도 제15회 정기총회 및 동계학술발표회
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• pp.16-17
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• 2004

• 천문학회보
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• 제31권1호
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• pp.23.2-23.2
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• 2006

• 천문학회지
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• 제38권2호
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• pp.117-120
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• 2005

Current instrumentation activities and the open user status of Okayama Astrophysical Observatory (OAO) are reviewed. There are two telescopes in operation and one telescope under reforming at OAO. The 188cm telescope is provided for open use for more than 200 nights in a year. The typical over-subscription rate of observation proposals for the 188cm telescope is ${\~}$ 1.5 - 2. The 50cm telescope is dedicated to $\gamma$-ray burst optical follow-up observation and is operated in collaboration with Tokyo Institute of Technology. The 91cm telescope will become a new very wide field near-infrared camera in two years. The high-dispersion echelle spectrograph (HIDES) is the current primary instrument for the open use of the 188cm telescope. Two new instruments, an infrared multi-purpose camera (ISLE) and an optical low-dispersion spectrograph (KOOLS), are now under development. They will be open as common use instruments in 2006.

• 천문학회보
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• 제41권2호
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• pp.50.1-50.1
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• 2016

We have found cool homopause temperatures (Kim et al. 2016) of 180 - 250 K for the 8-micron North Polar Hot Spot (8NPHS) of Jupiter, which has been observed to be stationary at 180 deg (SysIII) longitude since the early 1980s. The 3-micron spectro-images of Jupiter that we analyzed were obtained with GNIRS, Gemini Near-Infrared Spectrograph at Gemini North on January 13, 2013(UT), and at $8{\mu}m$ on Feburary 6, 2013(UT) with TEXES, the Texas Echelon Cross Echelle Spectrograph at the NASA IRTF. The cool homopause was unexpected, and a possible implication of the relatively cool 8NPHS homopause compared with those of other auroral regions will be presented.

• 천문학논총
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• 제18권1호
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• pp.69-74
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• 2003

A CCD camera for the BOES (Bohyunsan Observatory Echelle Spectrograph) has been developed. The camera consists of a 2048 ${\times}$ 4096 format CCD, a SDSU Gen-I CCD controller, and a continuous flow cryostat (CFC) designed by the ESO. In order to control the CCD under SDSU Gen-I controller, the voltage level of all the biases and clocks were lowered by -6V. The CFC showed cooling time of about 10 hour, after which the chip temperature settled down with variation less than ${\pm}1^{\circ}C$. The final chip temperature is around -105$^{\circ}C$ with the setting value for the CFC as -170$^{\circ}C$.