• 제목/요약/키워드: Conferences

검색결과 293건 처리시간 0.02초

Ensuring Patient Safety in Pediatric Dental Care

  • Daewoo Lee
    • 대한소아치과학회지
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    • 제51권2호
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    • pp.109-131
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    • 2024
  • This review aims to examine safety concerns in pediatric dental care and underscore the need for comprehensive patient safety initiatives within the Korean Academy of Pediatric Dentistry. Drawing insights from the prevailing patient safety policies of the American Academy of Pediatric Dentistry, case reports, and systematic reviews, this review elucidates issues such as dental fires during sedation, ocular complications from local anesthesia, and surgical emphysema. This review highlights the significance of safety toolkits encompassing infection control, medical error reduction, dental unit waterline infection, and nitrous oxide safety in pediatric dental settings, underscoring the need to foster a safety culture. Furthermore, this study explores the curriculum for pediatric dentistry residency programs, emphasizing concepts such as high-reliability organizations and mortality and morbidity conferences. The study suggests the need for initiatives to enhance patient safety, including establishing safety committees, expanding reporting systems, policy development, and supporting research related to patient safety. In conclusion, this study underlines key messages, emphasizing the utmost priority of patient safety, acknowledging the inevitability of human error, promoting effective communication, and cultivating a patient safety culture. These principles are vital for advancing patient safety in pediatric dental care and improving outcomes among pediatric patients.

치위생 연구의 장애요인 (Barriers to research utilization among dental hygiene researchers)

  • 문소정;신선정;정원균;김남희
    • 한국치위생학회지
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    • 제10권4호
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    • pp.745-755
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    • 2010
  • Objectives : The research of dental hygiene has made considerable progress over the past 10 years toward developing a unique body of knowledge for guiding education, practice, and profession. The purpose of this study was to determine Barriers to Research Utilization among Dental Hygiene Researchers. Methods : This study used cross-sectional design, self-reported questionnaire. That was consisted of 31 items(5 categories), reliability was tested(Cronbach's Alpha=0.882). The subjects were 117, mean age was $36.1{\pm}9.3$. They were consisted of full-time faculty (35.9%) and the doctoral course(61.0%). Results : The greatest barriers in dental hygiene research were 'Dental hygienists are isolated from knowledgeable colleagues with whom to discuss with' in Dental Hygienist category and 'The facilities are inadequate for implementation' in setting. In Research category, 'the research has not been replicated' and 'the relevant literature is not complied in one place' in presentation were the greatest. The researchers who were the twenty's, received dental hygiene license after 2000 year and studying for the master's degree had more barriers in all categories significantly. Conclusions : This finding provided evidence that there are barriers in dental hygiene research and we found the junior researchers have more difficulties. To improve this barriers, dental hygiene related associations need to focus on the research utilization and encourage them to attend conferences. In addition, research related education should be provided to them. Further study is essential to investigate the barriers for the established researchers in dental hygiene and to find specific solutions.

Risk of Serious Neutropenic Events in Cancer Patients Treated with Bevacizumab: A Meta-analysis

  • Zhou, Fan;Shao, Jiang-Hua;Wu, Lin-Quan;Yin, Xiang-Bao;Yu, Xin
    • Asian Pacific Journal of Cancer Prevention
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    • 제14권4호
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    • pp.2453-2459
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    • 2013
  • Bevacizumab has been approved for use in combination with chemotherapy to treat many types of cancer but associated neutropenic events, including febrile neutropenia, have been reported. To estimate the incidence and relative risk of neutropenic events in cancer patients treated with bevacizumab combination therapy, we searched PubMed, EMBASE, and Web of Science literature databases, as well as abstracts presented at the American Society of Clinical Oncology conferences, to identify relevant studies published from January 1966 to December 2011. Studies that compared bevacizumab plus chemotherapy or biological therapy with chemotherapy or biological therapy alone, and that had adequate safety data profiles, were selected for analysis. Statistical analyses were conducted to calculate the summary incidence rates, relative risks (RRs), and 95% confidence intervals (CIs) using fixed- or random-effects models. A total of 22 clinical trials involving 15,056 patients were included in the analysis. The summary incidences of high-grade neutropenia (HGN) and high-grade febrile neutropenia (HGFN) in patients receiving bevacizumab was 27.3% (95% CI: 26.4%-28.3%) and 3.91% (95% CI: 3.51%-4.37%), respectively. The risks of HGN (RR=1.10; 95% CI: 1.02-1.19; P=0.02) and HGFN (RR=1.31; 95% CI: 1.08-1.59; P=0.005) were significantly increased in bevacizumab-treated patients, compared to those who did not receive bevacizumab. The RR of bevacizumab-associated HGN, but not HGFN, varied significantly with tumor types (P=0.005). The increased risk of bevacizumab-associated neutropenic events was dose-dependent, as the RR was greater at a dose of 5 mg/kg/week than at 2.5 mg/kg/week. Our findings suggest that bevacizumab addition to cancer therapy significantly increases the risk of serious neutropenic events, and this risk may be dose-dependent.

변형된 Dijkstra 알고리즘을 활용한 오버레이 멀티캐스트 QoS 향상 기법 연구 (A Study on QoS Improvement for Overlay Multicast Using Modified Dijkstra Algorithm)

  • 이형옥;남지승;박준석
    • 한국산학기술학회논문지
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    • 제14권7호
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    • pp.3468-3473
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    • 2013
  • 본 화상 회의, 인터넷 방송 등의 실시간 응용 시스템을 위해 오버레이 멀티캐스트 트리가 충족 시켜야 하는 조건은 크게 두 가지이다. 첫 번째는 호스트, 즉 트리 상의 노드의 차수가 적절한 상한이어야 한다는 것이고 두 번째 조건은, 멀티캐스트 트리의 지름, 즉 트리 상의 경로 거리로 볼 때 가장 먼 두 사용자 간의 거리가 작아야 한다는 것이다. 각 노드의 차수가 상한을 가지고 있을 때 지름이 최소인 트리를 구성하는 문제는 NP-complete 문제로 알려져 있다. 본 논문에서는 Dijkstra 알고리즘의 Cost값을 트리를 구성하는 노드들의 가용대역폭, Delay를 체크한 후, 제안하는 Score Function을 적용하여 계산한다. 그리고 그 값을 Dijkstra 알고리즘에 적용하여 트리를 구성하고 시뮬레이션을 통해 성능평가를 하였다.

우리나라의 「이동성 야생동물종의 보전에 관한 협약」 가입 여부에 대한 타당성 분석 (Feasibility Study on the Ratification of 'Convention on the Conservation of Migratory Species of Wild Animals(CMS)' to Korea)

  • 박용하;최재용
    • 환경영향평가
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    • 제18권2호
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    • pp.111-122
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    • 2009
  • The impact of Korea's joining the Convention on the Conservation of Migratory Species of Wild Animals(CMS) was analyzed to examine its merits and faults as well as to discuss Korea's opportunities. Results of the analysis based on the agenda and decisions of the Conferences of the Parties, the parties performance, and other committees meetings over the last decades indicated that the affiliation of Korea into the CMS could provide various advantages and opportunities for Korea. First, Korea could upgrade its conservation activities regarding migratory species to the global aspects. Second, Korea could take initiatives for conservation of the migratory species in the Far East Asia. Third, Korea would have a better system in forecasting and problem-solving against the epidermic Avian Influenza through systematic cooperation with the CMS parties and other related international regimes. Finally, Korea will be in a better position to generate statistical data and to develop techniques to reduce the by-catches of the sharks and whales. Korea has already provided a fair and protective institutions for most of the migratory endangered species listed under Appendix I and II of the CMS. This implies that Korea may not require additional major changes to the basic acts and/or legislation. Joining the CMS may negatively impact on the fisheries and related businesses related to whales and sharks around the Ulsan and Pohang provinces. However, the obligation to protect whales and sharks demanded by the CMS is regarded as an acceptable article in Korea according to the analysis of the existing policies and scientific aspects. Nevertheless, if the joining the CMS should generate irreversible hardship for local people's livelihood and cultural aspects, Korea may ask for reservations on particular activities. Overall, we suggest that by joining the CMS, Korea could see various advantages and promotion in national policy.

공급망 형성을 위한 협업기업 발굴방법의 최신 동향 분석 (The State-of-the-art of Discovering New Suppliers to Build a Supply Chain)

  • 김경덕;조보람;신문수;류광열;조현보
    • 산업공학
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    • 제25권1호
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    • pp.21-30
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    • 2012
  • In the past, buyers and suppliers met each other to find common interests off-line in exhibitions and conferences, or through personal connection. These activities were time consuming and costly. With the advent of information era, these activities moved to online market places, where buyers search for suppliers with a set of keywords that are believed to be representative of their requirements. Its fundamental assumption is that all the potential candidates are registered in a certain database. However, recently buyers want to diversify suppliers due to needs of cost competitiveness or frequent new product development. To this end, instead of choosing suppliers from the supplier pool, discovering suppliers from all over the world should be emphasized. In order to enable buyers to describe their requirements and suppliers to capture their manufacturing capabilities via online market places, the semantic differences of terms between buyers and suppliers should be resolved. The paper summarizes various supplier discovery frameworks and prototype systems, which can be employed to expose domestic small-medium enterprises into global buyers in the near future.

GALAXY SED FITTING FROM AKARI TO HERSCHEL: 0.7 < z < 4 SUB-MILLIMETER LYMAN BREAK GALAXIES IN INFRARED

  • Burgarella, D.;The PEP-HerMES-COSMOS team, The PEP-HerMES-COSMOS team
    • 천문학논총
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    • 제27권4호
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    • pp.311-316
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    • 2012
  • Lyman break Galaxies are galaxies selected in the rest-frame ultraviolet. But, one important and missing information for these Lyman break galaxies is the amount of dust attenuation. This is crucial to estimate the total star formation rate of this class of objects and, ultimately, the cosmic star formation density. AKARI, Spitzer and Herschel are therefore the major facilities that could provide us with this information. As part of the Herschel Multi-tiered Extragalactic Survey, we have began investigating the rest-frame far-infrared properties of a sample of more than 4,800 Lyman Break Galaxies in the GOODS-North fiels. Most LBGs are not detected individually, but we do detect a sub-sample of 12 objects at 0.7 < z <1.6 and one object at z = 2.0. The ones detected by Herschel SPIRE have redder observed NUV-U and U-R colors than the others, while the undetected ones have colors consistent with average LBGs at z > 2.5. We have analysed their UV-to-FIR spectral energy distributions using the code cigale to estimate their physical parameters. We find that LBGs detected by SPIRE are high mass, luminous infrared galaxies. They also appear to be located in a triangle-shaped region in the $A_{FUV}$ vs. $logL_{FUV}$ diagram limited by $A_{FUV}$ = 0 at the bottom and by a diagonal following the temporal evolution of the most massive galaxies from the bottom-right to the top-left of the diagram. In a second step, we move to the larger COSMOS field where we have been able to detect 80 Lyman break galaxies (out of ~ 15,600) in the far infrared. They form the largest sample of Lyman break galaxies at z > 2.5 detected in the far-infrared. We tentatively name them Submillimeter Lyman break galaxies (S-LBGs).

THE 18 ㎛ LUMINOSITY FUNCTION OF GALAXIES WITH AKARI

  • Toba, Yoshiki;Oyabu, Shinki;Matsuhara, Hideo;Ishihara, Daisuke;Malkan, Matt;Wada, Takehiko;Ohyama, Youichi;Kataza, Hirokazu;Takita, Satoshi
    • 천문학논총
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    • 제27권4호
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    • pp.335-338
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    • 2012
  • We present the $18{\mu}m$ luminosity function (LF) of galaxies at 0.006 < z < 0.8 (the average redshift is ~ 0.04) using the AKARI mid-infrared All-Sky Survey catalogue. We have selected 243 galaxies at $18{\mu}m$ from the Sloan Digital Sky Survey (SDSS) spectroscopic region. These galaxies then have been classified into five types; Seyfert 1 galaxies (Sy1, including quasars), Seyfert 2 galaxies (Sy2), low ionization narrow emission line galaxies (LINER), galaxies that are likely to contain both star formation and Active Galactic Nuclei (AGN) activities (composites), and star forming galaxies (SF) using optical emission lines such as the line width of $H{\alpha}$ or the emission line ratios of [OIII]/$H{\beta}$ and [NII]/$H{\alpha}$. As a result of constructing the LF of Sy1 and Sy2, we found the following results; (i) the number density ratio of Sy2 to Sy1 is $1.64{\pm}0.37$, larger than the results obtained from optical LF and (ii) the fraction of Sy2 in the entire AGN population may decrease with $18{\mu}m$ luminosity. These results suggest that most of the AGNs in the local universe are obscured by dust and the torus structure probably depends on the mid-infrared luminosity.

THE FILAMENTARY WEB OF STAR FORMATION

  • White, Glenn J.;Doi, Yasuo;Komugi, Shinya;Kawada, Mitsunobu;Takita, Satoshi;Arimatsu, Ko;Ikeda, Norio;Kato, Daisuke;Kitamura, Yoshimi;Nakagawa, Takao;Ootsubo, Takafumi;Morishima, Takahiro;Hattori, Makoto;Tanaka, Masahiro;Etxaluze, Mireya;Shibai, Hiroshi
    • 천문학논총
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    • 제27권4호
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    • pp.201-207
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    • 2012
  • Following the first Public Release of the AKARI Point Source catalogues, we have worked on the production of a new far-infrared All-Sky Diffuse mapping product. In this paper we report first results from the All Sky diffuse maps that will shortly be released to the community, based on analysis of data from the Far Infrared Surveyor ($65{\mu}m-160{\mu}m$) instrument. These data are likely to have a strong impact on studies of extended structures, and the diffuse ISM.

COSMIC STAR FORMATION HISTORY AND AGN EVOLUTION NEAR AND FAR: AKARI REVEALS BOTH

  • Goto, Tomotsugu;AKARI NEP team, AKARI NEP team;AKARI all sky survey team, AKARI all sky survey team
    • 천문학논총
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    • 제27권4호
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    • pp.347-352
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    • 2012
  • Understanding infrared (IR) luminosity is fundamental to understanding the cosmic star formation history and AGN evolution, since their most intense stages are often obscured by dust. Japanese infrared satellite, AKARI, provided unique data sets to probe this both at low and high redshifts. The AKARI performed an all sky survey in 6 IR bands (9, 18, 65, 90, 140, and $160{\mu}m$) with 3-10 times better sensitivity than IRAS, covering the crucial far-IR wavelengths across the peak of the dust emission. Combined with a better spatial resolution, AKARI can measure the total infrared luminosity ($L_{TIR}$) of individual galaxies much more precisely, and thus, the total infrared luminosity density of the local Universe. In the AKARI NEP deep field, we construct restframe $8{\mu}m$, $12{\mu}m$, and total infrared (TIR) luminosity functions (LFs) at 0.15 < z < 2.2 using 4,128 infrared sources. A continuous filter coverage in the mid-IR wavelength (2.4, 3.2, 4.1, 7, 9, 11, 15, 18, and $24{\mu}m$) by the AKARI satellite allows us to estimate restframe $8{\mu}m$ and $12{\mu}m$ luminosities without using a large extrapolation based on a SED fit, which was the largest uncertainty in previous work. By combining these two results, we reveal dust-hidden cosmic star formation history and AGN evolution from z = 0 to z = 2.2, all probed by the AKARI satellite.