• Title/Summary/Keyword: light curves

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Seasonal Prevalence of the Vector Mosquitoes of Japanese Encephalitis Virus in Kyungpook Province, Korea (경북지역에서의 일본뇌염 매개모기에 출현 소장)

  • 주종윤;화전의인
    • Parasites, Hosts and Diseases
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    • v.23 no.1
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    • pp.139-150
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    • 1985
  • In order to determine the seasonal prevalence and population density of vector mosquitoes in Kyungpook Province, a survey based on average numbers of female mosquito per trap-night, were carried out during the period from May to November in 1984. Among the 34, 571 mosquitoes collected in Kyungsan county in animal shelters and human dwellings by light traps, approximately 45.0 per cent were Culex tritaeniorhynchus, 34.0 per cent Culex pipiens pallens, and 19.0 per cent Anopheles sinensis. By comparison, distribution of mosquito species in Ankang town, in which Japanese encephalitis had been reported in the past, were quite different and A. sinensis was the most abundant species, being constituted in 75.8 per cent, followed by C. tritaeniorhynchus(23.2 per cent), and C. pipiens pallens(O.6 per cent). In the general pattern of seasonal prevalence, C. tritaeniorhynchus first appeared in mid-June, and trapped in large numbers during the periods from mid-August to early September, showing a simple sharply pointed one-peaked curve, while C. pipiens pallens was found to be active through almost the entire season showing irregular curves with several peaks. The trend of seasonal distribution of A. sinensis was similar to that of C. tritaeniorhynchus, but the earliest dates of appearance and disappearance differed from that of C. tritaeniorhynchus. The results of hourly catches of mosquitoes by human baited traps have clearly shown the differences in the biting rhythm among the vector mosquitoes of this Province, such as the facts that C. tritaeniorhynchus and A. sinensis are rather constantly active all through a night with more or less inconspicuous peaks twice a night, while C. pipiens pallens exhibits an irregular curve, and the numbers of A. vexans nipponii, C. vagans and Armigeres subalbatus are very small and are not sufficient for estimating the biting rhythm. Four genera and fourteen species of larval mosquitoes collected from eighteen kinds of habitats which classified according to the categories followed by Bates (1949). The main breeding sites contributing to peak C. tritaeniorhynchus adult densities in this surveyed areas were evidently ricefields, ground pools, puddles and swamps and marshes, etc. Summarizing the results, this study indicated that the highest population density of C. tritaeniorhynchus was encountered in late August and early September, showing a simple sharply pointed one-peaked curve.

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Toxicity Assessment of Silver Ions Compared to Silver Nanoparticles in Aqueous Solutions and Soils Using Microtox Bioassay (Microtox 생물검정법을 이용한 은 이온과 은 나노입자의 수용액과 토양에서의 독성 비교 평가)

  • Wie, Min-A;Oh, Se-Jin;Kim, Sung-Chul;Kim, Rog-Young;Lee, Sang-Phil;Kim, Won-Il;Yang, Jae E.
    • Korean Journal of Soil Science and Fertilizer
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    • v.45 no.6
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    • pp.1114-1119
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    • 2012
  • This study was conducted to assess the microbial toxicity of ionic silver solution ($Ag^+N$) and silver nanoparticle suspension ($Ag^0NP$) based on the Microtox bioassay. In this test, the light inhibition of luminescent bacteria was measured after 15 and 30 min exposure to aqueous solutions and soils spiked with a dilution series of $Ag^+N$ and $Ag^0NP$. The resulting dose-response curves were used to derive effective concentration (EC25, $EC_{50}$, EC75) and effective dose ($ED_{25}$, $ED_{50}$, $ED_{75}$) that caused a 25, 50 and 75% inhibition of luminescence. In aqueous solutions, $EC_{50}$ value of $Ag^+N$ after 15 min exposure was determined to be < $2mg\;L^{-1}$ and remarkably lower than $EC_{50}$ value of $Ag^0NP$ with $251mg\;L^{-1}$. This revealed that $Ag^+N$ was more toxic to luminescent bacteria than $Ag^0NP$. In soil extracts, however, $ED_{50}$ value of $Ag^+N$ with 196 mg kg-1 was higher than $ED_{50}$ value of $Ag^0NP$ with $104mg\;kg^{-1}$, indicating less toxicity of $Ag^+N$ in soils. The reduced toxicity of $Ag^+N$ in soils can be attributed to a partial adsorption of ionic $Ag^+$ on soil colloids and humic acid as well as a partial formation of insoluble AgCl with NaCl of Microtox diluent. This resulted in lower concentration of active Ag in soil extracts obtained after 1 hour shaking with $Ag^+N$ than that spiked with $Ag^0NP$. With longer exposure time, EC and ED values of both $Ag^+N$ and $Ag^0NP$ decreased, so their toxicity increased. The toxic characteristics of silver nanomaterials were different depending on existing form of Ag ($Ag^+$, $Ag^0$), reaction medium (aqueous solution, soil), and exposure time.

INTENSIVE MONITORING SURVEY OF NEARBY GALAXIES (IMSNG)

  • Im, Myungshin;Choi, Changsu;Hwang, Sungyong;Lim, Gu;Kim, Joonho;Kim, Sophia;Paek, Gregory S.H.;Lee, Sang-Yun;Yoon, Sung-Chul;Jung, Hyunjin;Sung, Hyun-Il;Jeon, Yeong-beom;Ehgamberdiev, Shuhrat;Burhonov, Otabek;Milzaqulov, Davron;Parmonov, Omon;Lee, Sang Gak;Kang, Wonseok;Kim, Taewoo;Kwon, Sun-gill;Pak, Soojong;Ji, Tae-Geun;Lee, Hye-In;Park, Woojin;Ahn, Hojae;Byeon, Seoyeon;Han, Jimin;Gibson, Coyne;Wheeler, J. Craig;Kuehne, John;Johns-Krull, Chris;Marshall, Jennifer;Hyun, Minhee;Lee, Seong-Kook J.;Kim, Yongjung;Yoon, Yongmin;Paek, Insu;Shin, Suhyun;Taak, Yoon Chan;Kang, Juhyung;Choi, Seoyeon;Jeong, Mankeun;Jung, Moo-Keon;Kim, Hwara;Kim, Jisu;Lee, Dayae;Park, Bomi;Park, Keunwoo;O, Seong A
    • Journal of The Korean Astronomical Society
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    • v.52 no.1
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    • pp.11-21
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    • 2019
  • Intensive Monitoring Survey of Nearby Galaxies (IMSNG) is a high cadence observation program monitoring nearby galaxies with high probabilities of hosting supernovae (SNe). IMSNG aims to constrain the SN explosion mechanism by inferring sizes of SN progenitor systems through the detection of the shock-heated emission that lasts less than a few days after the SN explosion. To catch the signal, IMSNG utilizes a network of 0.5-m to 1-m class telescopes around the world and monitors the images of 60 nearby galaxies at distances D < 50 Mpc to a cadence as short as a few hours. The target galaxies are bright in near-ultraviolet (NUV) with $M_{NUV}$ < -18.4 AB mag and have high probabilities of hosting SNe ($0.06SN\;yr^{-1}$ per galaxy). With this strategy, we expect to detect the early light curves of 3.4 SNe per year to a depth of R ~ 19.5 mag, enabling us to detect the shock-heated emission from a progenitor star with a radius as small as $0.1R_{\odot}$. The accumulated data will be also useful for studying faint features around the target galaxies and other science projects. So far, 18 SNe have occurred in our target fields (16 in IMSNG galaxies) over 5 years, confirming our SN rate estimate of $0.06SN\;yr^{-1}$ per galaxy.