• Journal of Astronomy and Space Sciences
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• 제31권2호
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• pp.177-186
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• 2014

The Immersion Grating Infrared Spectrometer (IGRINS) is a near-infrared wide-band high-resolution spectrograph jointly developed by the Korea Astronomy and Space Science Institute and the University of Texas at Austin. IGRINS employs three HAWAII-2RG Focal Plane Array (H2RG FPA) detectors. We present the design and fabrication of the detector mount for the H2RG detector. The detector mount consists of a detector housing, an ASIC housing, a Field Flattener Lens (FFL) mount, and a support base frame. The detector and the ASIC housing should be kept at 65 K and the support base frame at 130 K. Therefore they are thermally isolated by the support made of GFRP material. The detector mount is designed so that it has features of fine adjusting the position of the detector surface in the optical axis and of fine adjusting yaw and pitch angles in order to utilize as an optical system alignment compensator. We optimized the structural stability and thermal characteristics of the mount design using computer-aided 3D modeling and finite element analysis. Based on the structural and thermal analysis, the designed detector mount meets an optical stability tolerance and system thermal requirements. Actual detector mount fabricated based on the design has been installed into the IGRINS cryostat and successfully passed a vacuum test and a cold test.

• 한국약용작물학회지
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• 제15권3호
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• pp.215-219
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• 2007

HPLC에 의한 미량 Ginsenoside의 분석법을 확립하고자 연구를 수행하였던 바, 그 결과를 요약하면 다음과 같다. 인삼 ginsenosid의 분석은 많이 시도되어 왔으나 주요 사포닌 및 미량 사포닌의 분석법이 정립되지 않고 있는 실정인바, 본 연구에서는 이동상 용매의 기울기 용리를 다양하게 변화를 주어 Rb$_1$, Rb$_2$, Rb$_3$, Rc, Rd, Re, Rf Rg$_1$, Rg$_2$, Rg$_3$, Rh$_1$, Rh$_2$의 총 12종의 사포닌을 양호하게 분리하는데 성공하였다. 이동상의 흐름 속도는 1.00ml/min이고 column온도는 35$^{\circ}$C, UV detector의 파장은 203nm로 모두 일정하게 한 결과였으며, 최적의 분석조건은 H$_2$O와 CH$_3$CN의 용매 조성이 82/18, 70/30, 55/45, 50/50으로 각각의 ginsenosides의 안정적인 Area 값을 얻을 수 있었고 재현성을 시도해본 결과, 반복간 편차가 적어 재현성이 매우 양호한 것으로 나타났다.

• 한국약용작물학회지
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• 제9권1호
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• pp.21-25
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• 2001

인삼의 주종 사포닌인 7종 사포닌($Rb_1,\;Rb_2,\;Rc,\;Rd,\;Re,\;Rf\;and\;Rg_1$)을 고속액체크로마토그라피로 분석하는 일반적인 방법인 순상 column에서 $Rg_1$, Re 및 Rf가 명확히 분리되지 않는 문제점을 개선하기위하여 본 연구를 수행하였다. 고속액체크로마토그라피를 이웅하여 역상 ${\mu}{\beta}ondapak$ ODS컬럼으로 인삼중 주종 사포닌인 7종 ginsenosides $Rg_{1},\;Re,\;Rf,\;Rb_{1},\;RC,\;Rb_{2}$ 및 Rd를 양호하게 분리하였다. 이때 분석 조건으로 이동상 용매 조성은 (A) $H_{2}O$, (B) methyl cyanaide을 (A) 90/(B) 10에서 (A) 0/(B) 100으로 기울기 용리를 이용하였으며, 기울기 용리 제어장치를 사용하여 용리시켰다. 용매 흐름속도는 1.5ml/min, 검출기는 UV detector(203nm)이었다. 이 방법은 분리능과 재현성 및 회수율이 양호하므로, 앞으로 인삼중 ginsenosides 분석에 응용될 수 있을 것으로 사료된다.

• 천문학회지
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• 제38권2호
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• pp.109-112
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• 2005

We present the design, expected performance, and current status of the wide field near-infrared camera (OAOWFC) now being developed at Okayama Astrophysical Observatory, NAOJ, NINS. OAOWFC is a near-infrared survey telescope whose effective aperture is 91cm. It works at Y, J, H, and $K_s$ bands and is dedicated to the survey of long period variable stars in the Galactic plane. The field of view is $0.95 {\times} 0.95 deg^2$ which is covered by one HAWAII-2 RG detector of 2048 ${\times}$ 2048 pixels with the pixel size of $18.5 {\mu}m\;{\times}\;18.5{\mu}m$, that results in the sampling pitch of 1.6 arcsec/pixel. OAOWFC can sweep the area of $840 deg^2$ every 3 weeks, attaining a limiting magnitude of 13 in $K_s$ band. It allows us to observe long period variables embedded in the Galactic plane where interstellar extinction is severe in optical.

• 한국식품과학회지
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• 제33권3호
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• pp.282-287
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• 2001

인삼 조사포닌을 기존의 고온 MeOH 추출/n-BuOH 분획법 및 고온 MeOH 추출/Diaion HP-20 흡착/MeOH 용출법과 새로이 시도된 고온 MeOH 추출/cation AG 50W흡착/$H_2O$ 용출/n-BuOH 추출법(AG 50W법), 상온 MeOH 추출/Diaion HP-20 흡착/MeOH 용출법(상온추출법)과 EtOAc/n-BuOH 직접 추출법으로 분리한 다음 기존의 HPLC/RI 방법으로 ginsenoside조성을 비교한 결과 EtOAc/n-BuOH 직접 추출법을 제외하고는 큰 차이가 없었으나 분리능과 감도가 우수한 HPLC/ELSD방법을 사용한 결과, ginsenoside $Rb_2$, Rf, $Rg_1$ 및 $Rh_1$ 등을 뚜렷이 식별할 수 있었고 추출 및 분획방법에 따라 조사포닌간 ginsenoside의 현저한 조성차이를 볼 수 있었다. 특히 AG 50W법에 의해 분리된 조사포닌에서 뚜렷한 prosapogenin 피크를 볼 수 있었으며 LC/MS의 결과, ginsenoside $Rb_1$, $Rb_2$ 등의 7종의 주종 사포닌 이외에도 5종의 prosapogenin과 1종의 chikusetsusaponin을 포함한 총 13종의 ginsenoside를 동정하였다. 새로이 정립한 HPLC 분석조건, 즉 $NH_2$ 대신에 $C_{18}$ column을 사용하고 $KH_2PO_4/CH_3CN$ gradient로 상온추출법으로 분리한 조사포닌을 분석한 결과, malonyl ginsenoside 피크를 용이하게 확인할 수 있었다.

• 분석과학
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• 제11권6호
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• pp.436-439
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• 1998

인삼 사포닌을 역상 고속 액체크로마토그래피 방법을 이용하여 여러 종류의 컬럼으로 분석하였다. 최적 조건은 Novapak $C_{18}$ ODS 역상 칼럼($3.9mm{\times}150mm$, $5{\mu}m$), $CH_3CN/H_2O$ 이성분 이동상 용액과 기울기 제어장치, 그리고 1.5 mL/min의 용매 흐름속도였으며, UV 검출기(203 nm)를 사용하였다. 인삼의 주성분인 ginsenoside $Rb_1$, $Rb_2$, Rc, Rd, Re, Rf 그리고 $Rg_1$ 7종을 50분 안에 양호하게 분리하였다. 각 성분에 대한 검량선은 직선성이 좋았으며, 회귀계수는 0.98~0.99이었다.

• 천문학회보
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• 제39권2호
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• pp.91.1-91.1
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• 2014

IGRINS (the Immersion GRating INfrared Spectrometer) is a high resolution wide-band infrared spectrograph developed by the Korea Astronomy and Space Science Institute (KASI) and the University of Texas at Austin (UT). This spectrograph has H-band and K-band science cameras, both of which use Teledyne's $2.5{\mu}m$ cutoff $2k{\times}2k$ HgCdTe HAWAII-2RG CMOS science grade detectors. Teledyne's cryogenic SIDECAR ASIC boards and JADE2 USB interface cards were installed to control these detectors. We performed lab experiments and test observations to optimize and evaluate the detector systems of science cameras. In this presentation, we describe a process to optimize bias voltages and way to reduce pattern noise with reference pixel subtraction schemes. We also present measurements of the following properties under optimized settings of bias voltages at cryogenic temperature (70K): read noise, Fowler noise, dark current, and reference-level stability, full well depth, linearity and conversion gain.

• 고려인삼학회:학술대회논문집
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• 고려인삼학회 2002년도 학술대회지
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• pp.491-501
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• 2002

A cross-examination between KT&G Central Research Institute and Guangzhou Institute for Drug Control was carried out in order to select optimum conditions for extraction, separation and determination of ginsenosides in red ginseng and to propose a better method for the quantitative analysis of ginsenosides. The optimum extraction conditions of ginsenosides from red ginseng were as follows: the extraction solvent, $70\%$ methanol; the extraction temperature, $100^{\circ}C;$ the extraction time, 1 hour for once; and the repetition of extraction, twice. The optimum separation conditions of ginsenosides on the SepPak $C_{18}$ cartridge were as follows: the loaded amount, 0.4 g of methanol extract; the washing solvents, distilled water of 25 ml at first and then $30\%$ methanol of 25 ml; the elution solvent, $90\%$ methanol of 5 ml. The optimum HPLC conditions for the determination of ginsenosides were as follows: column, Lichrosorb $NH_2(25{\times}0.4cm,$ 5${\mu}m$, Merck Co.); mobile phase, a mixture of acetonitrile/water/isopropanol (80/5/15) and acetonitrile/water/isopropanol (80/20/15) with gradient system; and the detector, ELSD. On the basis of the optimum conditions a method for the quantitative analysis of ginsenosides were proposed and another cross-examination was carried out for the validation of the selected analytical method conditions. The coefficient of variances (CVs) on the contents of ginsenoside-$Rg_{1}$, -Re and $-Rb_1$ were lower than $3\%$ and the recovery rates of ginsenosides were $89.4\~95.7\%,$ which suggests that the above extraction and separation conditions may be reproducible and reasonable. For the selected HPLC/ELSD conditions, the CVs on the detector responses of ginsenoside-Rg, -Re and $-Rb_1$) were also lower than $3\%$, the regression coefficients for the calibration curves of ginsenosides were higher than 0.99 and two adjacent ginsenoside peaks were well separated, which suggests that the above HPLC/ELSD conditions may be good enough for the determination of ginsenosides.

• 천문학회보
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• 제39권1호
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• pp.52.2-52.2
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• 2014

The Immersion Grating Infrared Spectrometer (IGRINS) is an unprecedentedly minimized infrared cross-dispersed echelle spectrograph with a high-resolution and high-sensitivity optical performance. A silicon immersion grating features the instrument for the first time in this field. IGRINS will cover the entire portion of the wavelength range between 1.45 and $2.45{\mu}m$ accessible from the ground in a single exposure with spectral resolution of 40,000. Individual volume phase holographic (VPH) gratings serve as cross-dispersing elements for separate spectrograph arms covering the H and K bands. On the 2.7m Harlan J. Smith telescope at the McDonald Observatory, the slit size is $1^{\prime\prime}{\times}15^{\prime\prime}$. IGRINS has a $0.27^{\prime\prime}$ pixel-1 plate scale on a $2048{\times}2048$ pixel Teledyne Scientific & Imaging HAWAII-2RG detector with SIDECAR ASIC cryogenic controller. The instrument includes four subsystems; a calibration unit, an input relay optics module, a slit-viewing camera, and nearly identical H and K spectrograph modules. The use of a silicon immersion grating and a compact white pupil design allows the spectrograph collimated beam size to be 25mm, which permits the entire cryogenic system to be contained in a moderately sized rectangular vacuum chamber. The fabrication and assembly of the optical and mechanical hardware components were completed in 2013. In this presentation, we describe the major design characteristics of the instrument and the early performance estimated from the first light commissioning at the McDonald Observatory.

• 천문학회보
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• 제39권2호
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• pp.90-90
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• 2014

The Immersion Grating Infrared Spectrometer (IGRINS) is the first astronomical spectrograph that uses a silicon immersion grating as its dispersive element. IGRINS fully covers the H and K band atmospheric transmission windows in a single exposure. It is a compact high-resolution cross-dispersion spectrometer whose resolving power R is 40,000. An individual volume phase holographic grating serves as a secondary dispersing element for each of the H and K spectrograph arms. On the 2.7m Harlan J. Smith telescope at the McDonald Observatory, the slit size is $1^{{\prime}{\prime}}{\times}15^{{\prime}{\prime}}$. IGRINS has a plate scale of 0.27" pixel-1 on a $2048{\times}2048$ pixel Teledyne Scientific & Imaging HAWAII-2RG detector with a SIDECAR ASIC cryogenic controller. The instrument includes four subsystems; a calibration unit, an input relay optics module, a slit-viewing camera, and nearly identical H and K spectrograph modules. The use of a silicon immersion grating and a compact white pupil design allows the spectrograph collimated beam size to be 25mm, which permits the entire cryogenic system to be contained in a moderately sized ($0.96m{\times}0.6m{\times}0.38m$) rectangular Dewar. The fabrication and assembly of the optical and mechanical components were completed in 2013. From January to July of this year, we completed the system optical alignment and carried out commissioning observations on three runs to improve the efficiency of the instrument software and hardware. We describe the major design characteristics of the instrument including the system requirements and the technical strategy to meet them. We also present the instrumental performance test results derived from the commissioning runs at the McDonald Observatory.