• Title/Summary/Keyword: Sed5

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Identification and spectral analysis of the CIBER/LRS detected stars

  • Kim, MinGyu;Matsumoto, T.;Lee, Hyung Mok;Arai, T.;Battle, J.;Bock, J.;Brown, S.;Cooray, A.;Hristov, V.;Keating, B.;Korngut, P.;Lee, Dae-Hee;Levenson, L.R.;Lykke, K.;Mason, P.;Matsuura, S.;Nam, U.W.;Renbarger, T.;Smith, A.;Sullivan, I.;Wada, T.;Jeong, Woong-Seob;Zemcov, M.
    • The Bulletin of The Korean Astronomical Society
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    • v.37 no.2
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    • pp.141.1-141.1
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    • 2012
  • CIBER (Cosmic Infrared Background ExpeRiment) is a sounding-rocket borne experiment which is designed to find the evidence of the First stars (Pop.III stars) in the universe. They are expected to be formed between the recombination era at z ~ 1100 and the most distant quasar (z ~ 8). They have never been directly detected due to its faintness so far, but can be observed as a background radiation at around $1{\mu}m$ which is called the Cosmic Near-Infrared Background (CNB). The CIBER is successfully launched on July 10, 2010 at White Sands Missile Range, New Mexico, USA. It consists of three kinds of instruments. One of them is a LRS (Low Resolution Spectrometer) which is a refractive telescope of 5.5 cm aperture with spectral resolution of 20 ~ 30 and wavelength coverage of 0.7 to $2.0{\mu}m$ to measure the spectrum of the CNB. Since LRS detects not only CNB but also stellar components, we can study their spectral features with the broad band advantage especially at around $1{\mu}m$ which is difficult at ground observations because of the atmospheric absorption by water vapor. I identified around 300 stars from observed six fields. If we can classify their spectral types with SED fitting, we can study their physical conditions of the stellar atmosphere as well as making a stellar catalogue of continuous stellar spectrum.

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Two-D fluid analysis at flow runoff in the dry stream, Jeju island (제주도 건천의 홍수유출시 2차원 흐름해석)

  • Yang, Won-Seok;Yang, Sung-Kee;Kim, Dong-Su
    • Proceedings of the Korea Water Resources Association Conference
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    • 2012.05a
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    • pp.587-587
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    • 2012
  • 현재 대부분 하천관리의 흐름해석에서 주가 되었던 1차원 분석은 하천 단면에 따른 횡적인 수면차, 유속분포를 분석할 수 없다는 단점을 가지고 있으며, 특히 유량 및 유속이 급속도로 늘어나는 홍수시에는 그 오차가 더욱 커질 수 있다. 반면에 2차원 모형의 흐름해석은 사행하천의 흐름 특성과 만곡부에서의 종 횡방향 수면경사 및 양안의 수면차와 합류지점의 횡방향 흐름 등의 영향을 고려할 수 있으며 1차원 해석과는 달리 전 단면에 걸쳐 유속 및 수위 분포를 나타낼 수 있어 실제흐름에 가까운 수리량을 얻을 수 있다. 본 연구를 위해 적용된 해석모형인 SMS는 미국 Brigham Young 대학의 환경모형연구실과 미공병단(USACE)의 수로실험국(WES) 등에서 개발한 프로그램으로서 RMA2, RMA4, SED2D 모형 등으로 구성되어 있다. 각각의 모형은 수리 동역학적 해석, 오염물 이송확산 해석, 유사의 이송 및 퇴적 해석이 가능하며 이 중 RMA2를 이용한 2차원 흐름해석을 통하여 보다 적합한 하천관리에 이용가능하도록 하고자 한다. 연구대상 지역은 제주도 한천 하류부로서 제주도 하천 특성상 평상시 건천의 상태를 이루고 있으나 태풍 및 집중호우시 홍수유출이 발생하여 수위가 급격하게 상승하는 양상을 보인다. 대표적인 예로 태풍 '나리'시 최대 일강우량 420mm로 인한 인근 지역에 0.5 ~ 1.5m의 침수흔적을 보이고 있다. 본 연구에서는 2011년 최고수위를 기록한 태풍 '무이파'를 대상으로 하였으며 대상지역의 Kalesto를 이용한 수위-유속 자료를 이용하여 산출된 유량을 경계조건으로 사용하였고 격자망 형성을 위한 지형 데이터는 지형도 및 측량자료를 이용하여 구축하였다. 사용된 대표적인 매개변수는 하상의 조도계수를 나타내는 Manning의 n값과 유체의 밀도, 속도구배, 구조 등 여러 가지의 유체조건에 따라 변하는 성질인 와점성계수(eddy viscosity)로 요약할 수 있으며 Manning의 n값은 하천설계기준에 따른 하천기본계획의 조도계수를 사용하였고 와점성계수는 적합한 흐름 분포를 결정하기 위해 흐름이 안정될 때까지 변화시켜 해석을 시행하였다. 해석결과 만곡부에서는 급한 흐름을 보이고 있으며 최대하폭 구간에서는 완만한 흐름이 나타나 사행하천의 흐름특성과 횡적인 하천단면에 따른 변화, 하상고 차이로 인한 유속분포를 확인할 수 있으며 이는 보다 유용한 하천관리에 이용가능할 것으로 사료된다.

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Preparation of Microporous Silica Membrane from TEOS-$H_2O$ System and Separation Of $H_2$-$N_2$ Gas Mixture (TEOS-$H_2O$계로부터 다공성 실리카 막의 제조 및 수소-질소 혼합기체의 분리)

  • 강태범;이현경;이용택
    • Membrane Journal
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    • v.10 no.2
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    • pp.55-65
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    • 2000
  • The porous silica membrane was prepared from Si(${OC}_2H_5)_4-H_2O$ system by sol-gel method. To investigate the characteristics of gels and porous silica membrane, we examined gels and porous silica membrane using TG-DTA, X-ray diffractometer, IR spectrophotometer, BET, SEM and TEM. The optimum mole ratio of Si(OC$_2$H$_{5}$)$_4$ : $H_2O$ $C_2$H$_{5}$OH for porous silica membrane was 1 : 4.5 : 4. The porous silica membrane was obtained by heat treatment of the gel above 700 $^{\circ}C$. The specific surface area of sintered gel was 3.8 $m^2$/g to 902.3 $m^2$/g at 100 $^{\circ}C$ to 1100 $^{\circ}C$ The pore size of sintered gel was in the range 20 $\AA$~ 50$\AA$. The particle size of sintered gel was 15 nm to 30 nm at 30$0^{\circ}C$ to 700$^{\circ}C$. The performance of the porous silica membrane was investigated for the separation of $H_2$/$N_2$ gas mixture. Gas separation through porous silica membrane depends upon Knudsen flow and surface flow. The veal separation factor($\alpha$) of $H_2$/$N_2$ was 5.17 at 155.15 cmHg and $25^{\circ}C$. The real separation factor($\alpha$), head separation factor($\beta$), and tail separation factor( $\bar{B}$) increased as the pressure of permeation cell Increased.sed.

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Prevalence and Characterization of Staphylococcus aureus Pathogenic Factors Isolated from Various Foods in Korea (국내 다양한 식품에서 분리한 황색포도상구균의 오염도 및 병원성 인자의 특징)

  • Cho, Yong-Sun;Lee, Joo-Young;Lee, Myung-Ki;Shin, Dong-Bin;Kim, Dong-Ho;Park, Ki-Moon
    • Korean Journal of Food Science and Technology
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    • v.43 no.5
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    • pp.648-654
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    • 2011
  • Staphylococcus aureus, a major human pathogen, produces a wide array of toxins, which causes various types of disease symptoms. Prevalence of S. aureus in various foods collected during 2006-2008 in Korea was investigated. S. aureus was isolated from 275 of 5,186 (5.3%) food samples collected from hyper-markets in Korea. Seasonal temperature affected the prevalence of S. aureus in various foods with high isolation rate during the summer. Most of the enterotoxigenic strains produced enterotoxin A only or enterotoxin A in combination with another toxin. A total of 54.5% of the tested strains contained either one or more enterotoxin genes and 3.6% possessed a tst gene. This study offers basic information for securing the stability of food during storage and circulation, and provides an epidemiological tool to study the cause, origin and temporal spread of S. aureus food poisoning.

Effect of Dietary Selenium on $\delta$-Aminolevulinic Acid Dehydratase Activity in Lead Poisoned Rats (식품 Selenium이 납중독된 흰쥐에 있어서 $\delta$-Aminolevulinic Acid Dehydratase 활성에 미치는 영향)

  • 방진숙
    • Journal of Nutrition and Health
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    • v.24 no.6
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    • pp.526-533
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    • 1991
  • The effect of dietary selenium on the activity of $\delta$-aminolevulinic acid dehydratase (ALAD) inhibited by the administration of lead were investigated in rats. The levels of dietary lead in the acetate form were 0(contro)200, 1, 000, 2, 000 and 5, 000ppm. Except control group four-level of lead diet groups were again subdivided into two depending on with and without 0.5ppm selenium supplementation. Sixty-three 40-day-old male Sprague-Dawley rats weighing 141$\pm$5g were distributed into total of nine diet groups according to RCB design and fed ad libidum for 4 weeks. Lead dietary groups did not show any significnat difference in food intake from the control group. Food efficiency and weight gain were lower in 2.000ppm and 5, 000ppm lead groups but not found in selenium supplemented ones. Hemoglobin contents hematocrit values ALAD activities in blood were significantly decreased and urinary aminolevulinic acid(ALA) excretion increa-sed with increasing dietary lead levels but partly restored by selenium supplementation. however only in 200, 1, 000 and 2, 000ppm dietary lead groups. On the other hand the hepatic ALAD activites of all four lead groups were recovered 19-30% from suppression by selenium supplementation. It was concluded that selenium administration alleviated lead toxicity in rats.

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Probiotic Properties of Enterococcus durans LP44 Isolated from Pigs Feces (돼지의 분변에서 분리한 Enterococcus durans LP44의 생균제로서의 특성)

  • 홍종욱;김인호;이상환;권오석;한영근;김지훈;강국희
    • Journal of the Korean Society of Food Science and Nutrition
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    • v.31 no.5
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    • pp.939-944
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    • 2002
  • We have screened the microorganisms from pigs feces for the development of probiotics which have acid-and bile-tolerance. Among them, a strain which was identified as Enterococcu durans LP44 was selected. Sixty Duroc$\times$Yorkshire$\times$Landrace pigs (6.30$\pm$0.04 kg average initial body weight) were used in a 14 days growth assay to determine the effects of Enterococco duran Lf44 culture on growth performance of weaned pigs. Dietary treatments included 1) DF (dry feeding),2) W (wet feeding),3) WF+5ED (wet feeding+5% Enterocucu duran LP44 culture),4) WF+ 10ED (wet feeding +10% Enterococcus durans LP44 culture). For overall periods, average daily gain in pigs fed % diet tended to increase compared to pigs fed DF diet without significant difference. Also, there was no significant difference in gain/feed. At 5 days after the onset of the experiment, pigs fed WF+5ED and WF+10ED diets were significantly increased in dry matter and nitrogen digestibilities compared to pigs fed DF and W diets (p<0.05). At 14 days after the onset of the experiment, pigs fed WF+ 10ED diet were significantly increased in dry matter digestibility compared to pigs fed DF diet (p<0.05). Also, pigs fed WF + 10ED diet were significantly increased in nitrogen digestibility compared to other treatments (p<0.05). In conclusion, supplemental Enterococcus durans LP44 was an effective means of improving ADG and nutrient digestibility.

Mycelial Growth of Ganoderma lucidum and Grifola frondosa in Milk Whey (유청을 이용한 영지버섯과 잎새버섯의 균사체 배양)

  • Chung, Kun-Sub;Koo, Young-Jo;Yoo, Jin-Young;Choi, Shin-Yang;Shin, Dong-Hwa
    • The Korean Journal of Mycology
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    • v.19 no.1
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    • pp.61-65
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    • 1991
  • For the production of mycelia of mushroom by submerged culture, the experiment was carried out. mushroom. The optimum culture broth for Ganoderma lucidum NG-L were compo­sed of CMC 0.8%(w/v) and $(NH_4)_2SO_4$ 0.2%, with 10%(v/v) of inoculum size and pH 5.5 when the milk whey was used as basal medium. In case of Grifola frondosa ATCC48688, the optimum broth were composed of soluble starch 2%(w/v) and $KNO_3$ 0.l%(w/v), with 8%(v/v) of inoculum size and pH 5.2. Among several plant growth hormones,indole-3-acetic acid and gibberellin $A_3-3-acetate$ stimulated the mycelial growth of Ganoderma lucidum NG-L and Grifola frondosa ATCC 48688 respectively. The culture broth of these mushrooms inhibited the growth of B. subtilis and P. aeruginosa.

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AKARI DEEP FIELD SOUTH: SPECTROSCOPIC OBSERVATIONS OF INFRARED SOURCES

  • Sedgwick, Chris;Serjeant, Stephen;Pearson, Chris;Matsuura, Shuji;Shirahata, Mai;Matsuhara, Hideo;Marchetti, Lucia;White, Glenn J.;Vaccari, Mattia;Baronchelli, Ivano;Rodighiero, Giulia;Hadsukade, Bunyo;Clements, David L.;Amber, Simon
    • Publications of The Korean Astronomical Society
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    • v.32 no.1
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    • pp.281-285
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    • 2017
  • We present a summary of our spectroscopic redshift catalogue of 404 sources in the AKARI Deep Field South (ADF-S). We have used the AAOmega spectrograph to target mid-infrared and far-infrared sources selected primarily from AKARI observations in this field for which we were able to obtain optical counterparts. Our sources with identified redshifts include 316 with $H{\alpha}$ detections at $z{\leq}0.345$ and 15 sources at z > 1 with MgII or $Ly{\alpha}$ emission lines. About 13% of our $z{\leq}0.345$ sources are dominated by active galactic nuclei (AGN) emission, although many show emission from both star formation and AGNs. The median Balmer decrement is 5.9. Ultra-luminous infrared galaxies (ULIRGs) were found only in the higher-redshift sources. Optical and near infrared data will be available shortly, enabling calibration of the line luminosities and spectral energy distribution (SED) fitting for these sources.

PROPERTIES OF DUST OBSCURED GALAXIES IN THE NEP-DEEP FIELD

  • Oi, Nagisa;Matsuhara, Hideo;Pearson, Chris;Buat, Veronique;Burgarella, Denis;Malkan, Matt;Miyaji, Takamitsu;AKARI-NEP team
    • Publications of The Korean Astronomical Society
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    • v.32 no.1
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    • pp.245-249
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    • 2017
  • We selected 47 DOGs at z ~ 1.5 using optical R (or r'), AKARI $18{\mu}m$, and $24{\mu}m$ color in the AKARI North Ecliptic Pole (NEP) Deep survey field. Using the colors among 3, 4, 7, and 9µm, we classified them into 3 groups; bump DOGs (23 sources), power-law DOGs (16 sources), and unknown DOGs (8 sources). We built spectral energy distributions (SEDs) with optical to far-infrared photometric data and investigated their properties using SED fitting method. We found that AGN activity such as a AGN contribution to the infrared luminosity and a Chandra detection rate for bump and power-law DOGs are significantly different, while stellar component properties like a stellar mass and a star-formation rate are similar to each other. A specific star-formation rate range of power-law DOGs is slightly higher than that of bump DOGs with wide overlap. Herschel/PACS detection rates are almost the same between bump and power-law DOGs. On the other hand SPIRE detection rates show large differences between bump and power-law DOGs. These results might be explained by differences in dust temperatures. Both groups of DOGs host hot and/or warm dust (~ 50 Kelvin), and many bump DOGs contain cooler dust (${\leq}30$ Kelvin).

Features and Properties of $YBa_2$$Cu_3$$O_{7-x}$ Films Grown on SrTi$O_3$ by High Frequency PLD

  • Shi, D.Q.;Ko, R.K.;Song, K.J.;Chung, J.K.;Choi, S.J.;Park, Y.M.;Shin, K.C.;Yoo, S.I.;Park, C.
    • Progress in Superconductivity
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    • v.5 no.1
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    • pp.75-79
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    • 2003
  • YBCO films were deposited with various thicknesses from 100nm to 1.6$\mu\textrm{m}$ on single crystal $SrTiO_3$ substrates by pulsed laser deposition (PLD). The effects of different deposition conditions, especially different deposition rates by means of changing the pulsed laser frequency up to 200Hz, on the J$_{c}$ value were studied. For YBCO film with the thickness of 200nm, the $J_{c}$ value of $2.1MA/\textrm{cm}^2$ has been achieved under the high deposition rate of 3.2nm/s (190nm/min). The $J_{c}$ can be maintained greater than $1M/\textrm{cm}^2$ with the thickness less than 1$\mu\textrm{m}$. The X-ray analysis was used to examine the texture, crystallization and surface quality. The SEM was employed to analyze the surface of YBCO, and it was shown the surface of YBCO film became rougher with increasing the thickness. There were many large singular outgrowths and networks of outgrowths on the surface of YBCO films which lowered the density of thick YBCO film. The outgrowth network was probably the a-axis YBCO corresponding to XRD $\theta$-2$\theta$scan and $\chi$-scan which were used to characterize a-axis orientation of YBCO film. The reason for J$_{c}$ declining with increasing the thickness was studied and discussed.sed.

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