• 천문학회보
• /
• 제33권2호
• /
• pp.53.2-53.2
• /
• 2008

• 천문학논총
• /
• 제27권4호
• /
• pp.219-220
• /
• 2012

We present the results of far-infrared spectroscopic observations of the Large Magellanic Cloud (LMC) with FIS-FTS. We covered a large area across the LMC, including 30 Doradus (30 Dor) and N44 star-forming regions, by 191 pointings in total. As a result, we detect the [OIII] and [CII] line emission as well as far-infrared dust continuum emission throughout the LMC. We find that the [OIII] emission is widely distributed around 30 Dor. The observed size of the distribution is too large to be explained by massive stars in 30 Dor, which are assumed to be enshrouded by clouds with the constant gas density estimated from the [OIII] line intensities. Therefore the surrounding structure is likely to be highly clumpy. We also find a global correlation between the [OIII] and the far-infrared continuum emission, suggesting that the gas and dust are well mixed in the highly-ionized region where the dust survives in clumpy dense clouds shielded from energetic photons. Furthermore we find that the ratios of [CII]/CO are as high as 110,000 in 30 Dor, and 45,000 even on average, while they are typically 6,000 for star-forming regions in our Galaxy. The unusually high [CII]/CO is also consistent with the picture of clumpy small dense clouds.

• 디자인학연구
• /
• 제13권3호
• /
• pp.303-312
• /
• 2000

시장경제에 뿌리를 둔 아이덴티티 시스템 개발작업은 "분산으로부터 통합" 을 대원칙으로 삼아 지난 반세기동안 발전해 왔으며 , 그 필요성은 이미지 마케팅 측면에서 입증되어 왔다. 그러나 1995년을 기점으로 가속화된 정보통신분야의 발전에 의한 정보의 양과 속도는 과거와 비교할수 없으며, 따라서 정보의 수용자들은 자신들의 기준으로 정보를 평가, 선택할수 있는 기회를 가지게 되었다. 이러한 환경변화에 적절히 대응키 위해서는 새로운 방법을 모색해야 하며, 종래의 방법에 의존한 도입 효과는 불확실하다. 아미덴티티 시스템에서 허용되는 유연성의 정도는 경영과 마케팅전략에 의해 결정되어야 한다. 기업활동영역이 다양한 경우, 시대의 트랜드에 민감한 업종, 그리고 일반인과소비자들에 감성적 접근을 시도하는 기업들에게 FIS은 효과적으로 기능 한다. FIS은 성장 변화하는 운영체계를 가지므로 환경변화에 대한 적응력이 탁월하며, 기업의 이미지를 신선하게 유지시킬수 있는 것이 가장 큰 장점이다.

• 한국항행학회논문지
• /
• 제18권4호
• /
• pp.325-333
• /
• 2014

CNS/ATM을 구성하는 감시 시스템의 핵심 기술인 ADS-B는 항공기와 항공기 간의 정보 교환을 통해 기존의 레이더 감시 시스템을 보완 및 대체할 수 있다. ADS-B를 지상 항공 교통 관리 시스템에서 사용할 수 있도록 구축하는 지상 ADS-B 시스템은 항공기와 ADS-B 메시지를 송수신하는 지상장비, ADS-B/TIS-B/FIS-B 서버 등 다양한 장비가 필요하며 이들 장비는 네트워크 기반의 분산 시스템 형태로 구성된다. 따라서 지상 ADS-B 시스템의 분산된 장비들을 효율적으로 관리할 수 있도록 원격에서 지상 ADS-B 시스템을 구성하는 장비들의 상태를 감시하고 제어 할 수 있는 상태 감시 및 원격 제어 시스템이 반드시 필요하다. 본 논문에서는 네트워크 기반 상태 관리 프로토콜인 SNMP를 이용하여 지상 ADS-B 시스템을 구성하는 모든 장비의 상태를 감시하고 제어할 수 있는 ADS-B 시스템 상태 감시 및 원격 제어 시스템을 설계하고 구현하였다.

• Journal of Dental Anesthesia and Pain Medicine
• /
• 제19권1호
• /
• pp.29-36
• /
• 2019

Background: An inability to cope with threatening dental stimuli, i.e., sight, sound, and sensation of airotor, manifests as anxiety and behavioral management problems. Behavior modification techniques involving pre-exposure to dental equipment will give children a first-hand experience of their use, sounds, and clinical effects. The aim of this study was to compare the techniques of Tell-Show-Play-doh, a smartphone dentist game, and a conventional Tell-Show-Do method in the behavior modification of anxious children in the dental operatory. Methods: Sixty children in the age group of 4-8 years, with Frankl's behavior rating score of 2 or 3, requiring Class I and II cavity restorations were divided into three groups. The groups were Group 1: Tell-Show-Play-doh; Group 2: smartphone dentist game; and Group 3: Tell-Show-Do technique and each group comprised of 20 children. Pulse rate, Facial Image Scale (FIS), Frankl's behavior rating scale, and FLACC (Face, Leg, Activity, Cry, Consolability) behavior scales were used to quantify anxious behavior. Operator compliance was recorded through a validated questionnaire. Results: The results showed lower mean pulse rates, lower FIS and FLACC scores, higher percentage of children with Frankl's behavior rating score of 4, and better operator compliance in both the Tell-Show-Play-doh and smartphone dentist game groups than in the conventional Tell-Show-Do group. Conclusion: The Tell-Show-Play-doh and smartphone dentist game techniques are effective tools to reduce dental anxiety in pediatric patients.

• 한국동물위생학회지
• /
• 제45권3호
• /
• pp.191-199
• /
• 2022

We investigated the virulence genes, O-serotypes, antimicrobial resistance of pathogenic E. coli isolated from carcasses (n=455) and environmental (n=372) samples of 11 cattle and 12 pig slaughterhouses from December 2020 to December 2021. E. coli were isolated from nine carcasses (2.0%), three slaughter facilities (1.4%), two utensils (2.7%) and three abattoir workers (3.5%) from four cattle and four pig slaughterhouses. Among all isolates, 13 STEC (76.5%) were identified, followed by four EPEC (23.5%). As a result of the antibiotic susceptibility test, all isolates were resistant to at least one antimicrobial, of which 70.6% isolates showed multidrug resistance patterns. The serotypes were diverse in pigs compared to cattle, with serotypes O18, O66, O109 in cattle and O9, O76, O85, O100, O153, and O159 in pigs. In a single cattle slaughterhouse, eight STEC O66 were isolated from various types of sample (4 slaughter animal surfaces, 3 gloves, and 1 knife) with two antimicrobial resistance patterns (CHL-FIS-STR and CHL-FIS). Those two types of strain were suspected cross-contamination from utensils to slaughter animal surfaces. These results showed that pathogenic E. coli were detected in carcasses and various environmental samples in cattle and pig slaughterhouses. Nationwide monitoring and hygiene management are required to prevent cross-contamination of STEC isolate slaughterhouses.

• 천문학논총
• /
• 제27권4호
• /
• pp.293-294
• /
• 2012

We established a separation scheme to distinguish galaxies from stars with the aid of AKARI/FIS color-color (CC) diagrams. In all the combinations of CC diagrams we can distinguish two separate clouds. It was shown that in all cases one of them contains more than 95% of galaxies and the other one, in most cases, consists in more than 80% of stars (Pollo et al., 2010). Currently we are looking into more detailed classifications. We are especially interested in separating different morphological types of galaxies, mainly within spiral galaxies. Moreover, we study the properties of infrared galaxies.

• 천문학논총
• /
• 제27권4호
• /
• pp.339-341
• /
• 2012

It is a long known fact that there exists a tight correlation between far-infrared and radio emission both for galaxies hosting active galactic nuclei and for star forming galaxies. We probe the radio - infrared correlation for a sample of extragalactic sources constructed by the cross-correlation of the AKARI/IRC All-Sky Survey Point Source Catalogue, the AKARI/FIS All-Sky Survey Bright Source Catalogue, and the NRAO VLA Sky Survey. Additionally, all objects of our sample were identified as galaxies in NED and SIMBAD databases, and a part of them is known to host active galactic nuclei (AGNs). After remeasuring all the fluxes, in order to avoid small aperture effects, we compare the ratio of radio to infrared emission from different types of extragalactic sources, and discuss the FIR/radio correlation as seen by AKARI and make a comparison to the previous results obtained thanks to IRAS.

• International Journal of Internet, Broadcasting and Communication
• /
• 제12권3호
• /
• pp.149-155
• /
• 2020

Air pollution is a problem of environmental health risk in big cities. Recently, researchers have proposed using various artificial intelligence technologies to predict air pollution. The proposed model is Cooperative of Artificial Neural Network (ANN) and Fuzzy Inference System (FIS), to predict air pollution of Korean cities using Python. Data air pollutant variables were collected and the Air Korean Web site air quality index was downloaded. This paper's aim was to predict on the health risks and the very unhealthy values of air pollution. We have predicted the air pollution of the environment based on the air quality index. According to the results of the experiment, our model was able to predict a very unhealthy value.

• 천문학논총
• /
• 제32권1호
• /
• pp.113-116
• /
• 2017

A significant number of the parameters of a gamma-ray burst (GRB) and its host galaxy are calculated from the afterglow. There are various methods obtaining extinction values for the necessary correction for galactic foreground. These are: galaxy counts, from HI 21 cm surveys, from spectroscopic measurements and colors of nearby Galactic stars, or using extinction maps calculated from infrared surveys towards the GRB. We demonstrate that AKARI Far-Infrared Surveyor sky surface brightness maps are useful uncovering the fine structure of the galactic foreground of GRBs. Galactic cirrus structures of a number of GRBs are calculated with a 2 arcminute resolution, and the results are compared to that of other methods.