• 한국항공우주학회지
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• 제46권6호
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• pp.519-526
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• 2018

우주 자원을 분석하기 위해서는 지구로 가져와야 한다는 단점이 있었다. 하지만, 레이저 유도 분해 분광법(Laser-induced breakdown spectroscopy, LIBS)고 라만 분광법(Raman spectroscopy)을 활용한다면 우주 광물의 실시간 정성 정량적으로 분석이 가능하다. 레이저 유도 분해 분광법은 높은 에너지의 레이저를 물질 표면에 집중시켜 플라즈마를 생성한후, 방출되는 빛을 분광기를 통해 획득하여 원자 구성을 분석하는 분광법이다. 라만 분광법은 레이저를 물질 표면에 조사시켜 산란되는 빛을 측정하여 분자구조를 분석하는 분광법이다. 이 두 가지 분광법은 각각 미지의 광물의 원자 분자를 분석하는 상호보완적인 분광법으로 우주탑재체로서 효율적인 장점을 가지고 있다. 본 연구에서는 주성분 분석법(Principal Component Analysis, PCA)을 활용하여 광물을 정성적으로 분석했다. 또한, 두 가지 광물을 혼합한 시료를 제작하여 구성 성분 비율에 따른 신호 세기로부터 물질의 구성 비율을 예측하는 정량분석을 시행하였다.

• 천문학회보
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• 제43권1호
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• pp.44.1-44.1
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• 2018

We present a spectroscopic study of the Galactic supernova remnant (SNR) Cygnus Loop using the fifth Data Release (DR5) of LAMOST. The LAMOST (Large Sky Area Multi-Object Fiber Spectroscopic Telescope) features both a large field-of-view (about 20 deg2) and a large aperture (~4 m in diameter), which allow us to obtain 4000 spectra simultaneously. Its wavelength coverage ranges from ${\sim}3700{\AA}$ to $9000{\AA}$ with a spectral resolution of $R{\approx}1800$. The Cygnus Loop is a prototype of middle-aged SNRs, which has advantages of being bright, large in angular size (${\sim}3.8^{\circ}{\times}3^{\circ}$), and relatively unobscured by dust. Along the line of sight of the Cygnus Loop, 2747 LAMOST DR5 spectra are found in total, which are spatially distributed over the entire remnant. Among them, 778 spectra are selected based on the presence of emission lines (i.e., [O III]${\lambda}5007$, Ha, and [S II]${\lambda}{\lambda}$ 6717, 6731) for further visual inspection. About half of them (336 spectra) show clear spectral features to confirm their association with the remnant, 370 spectra show stellar features only, and 72 spectra are ambiguous and need further investigation. For those associated with the remnant, we identify emission lines and measure their intensities. Spectral properties considerably vary within the remnant, and we compare them with theoretical models to derive physical properties of the SNR such as electron density and temperature, and shock velocity. While some line ratios are in good agreement with model prediction, others cannot be explained by simple shock models with a range of shock velocities. We discuss these discrepancies between model predictions and the observations and finally highlight the powerfulness of the LAMOST data to investigate spatial variations of physical properties of the Cygnus Loop.

• Applied Biological Chemistry
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• 제32권1호
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• pp.1-7
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• 1989

Methyl linolenate를 자동산화반응(自動酸化反應)의 model 화합물(化合物)로 선정(選定)하여 실온(室溫)에서 90m1/min.의 air flow rate로 96시간(時間) 산화(酸化)시켰으며 여기서 얻어진 산화생성물(酸化生成物)을 TLC로 분리(分離)한 다음 각(各) 분획물(分劃物)을 ir, uv, nmr로 분석(分析)하였다. 분광기기분석(分光機器分析) 결과(結果)는 서로 일치(一致)하였으며 Rf. 0.28과 $0.15{\sim}0.10$의 화합물(化合物)들이 hydroperoxide와 cis, trans-substituted diene인 것으로 확인(確認)되었고 주(主)로 cis, transconjugated diene system과 약간(若干)의 trans, trans-configuration인 것으로 밝혀졌다. 특(特)히 $5.83{\sim}6.60ppm$에서 나타난 multiplet 부위(部位)는 산화생성물(酸化生成物)들의 화학구조(化學構造)를 결정(決定)함에 있어서 큰 도움을 줄 것으로 생각하기 때문에 앞으로 많은 연구(硏究)가 요망(要望)된다.

• 천문학회지
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• 제55권2호
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• pp.23-36
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• 2022

We present a method to determine nitrogen abundance ratios with respect to iron ([N/Fe]) from molecular CN-band features observed in low-resolution (R ~ 2000) stellar spectra obtained by the Sloan Digital Sky Survey (SDSS) and the Large Sky Area Multi-Object Fiber Spectroscopic Telescope (LAMOST). Various tests are carried out to check the systematic and random errors of our technique, and the impact of signal-to-noise (S/N) ratios of stellar spectra on the determined [N/Fe]. We find that the uncertainty of our derived [N/Fe] is less than 0.3 dex for S/N ratios larger than 10 in the ranges T_eff = [4000, 6000] K, log g = [0.0, 3.5], [Fe/H] = [-3.0, 0.0], [C/Fe] = [-1.0, +4.5], and [N/Fe] = [-1.0, +4.5], the parameter space that we are interested in to identify N-enhanced stars in the Galactic halo. A star-by-star comparison with a sample of stars with [N/Fe] estimates available from the Apache Point Observatory Galactic Evolution Experiment (APOGEE) also suggests a similar level of uncertainty in our measured [N/Fe], after removing its systematic error. Based on these results, we conclude that our method is able to reproduce [N/Fe] from low-resolution spectroscopic data, with an uncertainty sufficiently small to discover N-rich stars that presumably originated from disrupted Galactic globular clusters.

• 천문학회지
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• 제20권2호
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• pp.63-94
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• 1987

Using many homogeneous data of DDO and UBV colors for all luminosity classes and physical quantities known from spectroscopic observations, new calibration schemes with DDO photometric parameters are presented for metal abundance, effective temperature and surface gravity of stars. And an intrinsic color relation is derived for the reddening estimate.

• 한국인쇄학회지
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• 제13권1호
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• pp.73-91
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• 1995

Spectroscopic and Photoelectric Characteristics in the Cyanine and Merocyanine Dye according to systematically change of their structures were experimentally discussed. As result, in solution, Hetero atoms(X) of Cyanine and Merocyanine dye were participated in resonance X of d obital rather than X of pobital,effected in resonance and contributed in extension of conjugated system. in solid film,new spectra,called eximer-fluorenscence,were appeared in 3-dimensional fluorenscence of high density of Cyanine dye but not of Merocyanine. The activational energy of conductivity in Merocyanine dye was lower than in cyanine, an the contrary,the drift mobility was higher and the former in photoelectric characteristics was more effec-tive than the latter. In this paper,authors invertigated the changes of dye structure by molecular obital method to confirm the results of spectroscopic and photoelectric characteristics in the Cyanine and Merocyanine Dye acco-rding to systematically cally change of their structure, and counted total energy on dihedral angle and dipol miments if dyes in S0 and S1.

• 천문학회보
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• 제35권2호
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• pp.84.2-84.2
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• 2010

Radial changes of stellar population within the Galactic globular clusters have been reported in many spectroscopic and photometric studies. We present new integrated spectroscopic data for 24 Galactic globular clusters and have measured line indices within various aperture sizes. Radial gradients have been investigated for the Balmer lines and metal lines (Mgb). Our results show an increase in the strength of the Balmer lines toward the centres in some clusters including NGC7078, NGC7089, and NGC6934, in which colour gradients also have been detected previously. However, some other clusters show little trend or even an increase toward the outskirt in the Balmer lines. Metal sensitive lines generally have an anti-correlation with the Balmer lines. We discuss possible stellar populations being responsible for the radial change in line indices.

• 천문학회보
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• 제43권1호
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• pp.58.1-58.1
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• 2018

The redshift range $1.4{\lesssim}z{\lesssim}2.5$ is often called the 'redshift desert' because of the difficulties in measuring spectroscopic redshifts due to the shifting of the major spectroscopic features into near-infrared wavelength (Steidel et al. 2004). One of the most efficient and fast way to select galaxies at this redshift range is the BzK technique designed by Daddi et al. (2004). Combining deep BVRz data from Deep Lens Survey with the wide-field (~4.08 deg2) K-band image, we select 1200 star-forming BzKs (sBzKs) and 120 passive BzKs (pBzKs) at K < 21.25. We discuss about the photometric redshifts, star formation rates, and stellar mass of the selected BzKs. Possible large scale structure at $1.4{\lesssim}z$ < 1.6 based on the spatial distribution of the BzKs is also introduced.

• Natural Product Sciences
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• 제21권4호
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• pp.273-277
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• 2015

Comprehensive chemical analysis of extracts and fractions of marine actinomycete strains led to the discovery of a new minor secondary metabolite, salternamide E (1), from a saltern-derived halophilic Streptomyces strain. The planar structure of salternamide E (1) was elucidated by a combinational analysis of spectroscopic data including NMR, MS, UV, and IR. The absolute configuration of salternamide E (1) was determined by circular dichroism spectroscopic analysis. Salternamide E displayed weak cytotoxicity against various human carcinoma cell lines.

• 한국광학회지
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• 제3권2호
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• pp.92-100
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• 1992

회전검광자형의 분광타원해석기를 제작하였다. 각 부품의 미소결함에 의한 오차를 고려하여 이들이 타원해석상수들에 미치는 영향을 최소로 하는 배치를 결정하였다. Straight through operation의 성능평가 결과 300nm~850nm의 파장대역에 걸쳐 tan$\psi$와 cos$\Delta$의 편차는 0.2%내외로 만족할 만한 것으로 판단되었다. SE를 사용하여 불화박막의 굴절율및 void분포상태를 측정하였고 응용성에 관하여 논의하였다.