• 원예과학기술지
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• 제31권2호
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• pp.173-178
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• 2013

국내에서 육성되어 수출딸기의 주역인 '매향' 딸기의 수경재배에서 적절한 배양액 농도를 구명하고자 하였다. 2010년 9월 20일에 코코피트를 충진한 수경재배 벤치에 정식하고, 야마자키 조성 딸기배양액을 이용하여 처리별로 EC를 0.6, 0.8, 1.2, $1.8dS{\cdot}m^{-1}$로 급액하였다. 지상부 생육은 배양액 농도 차이에 따라 일부 차이를 나타내긴 하였지만 그 차이는 미미하여 큰 영향을 받지는 않는 것으로 생각되었다. 과장은 정화방에서는 EC 0.8과 $1.2dS{\cdot}m^{-1}$처리에서 가장 길었고 $1.8dS{\cdot}m^{-1}$에서 가장 짧았다. 제 2화방에서는 EC $1.8dS{\cdot}m^{-1}$처리에서 가장 짧았고 나머지 처리 간에는 유의한 차이가 없었다. 제 3화방은 정화방과 동일한 경향을 나타내었으며, 제 4화방은 처리 간에 통계적으로 유의한 차이가 없었다. 과경은 정화방과 제 1화방에서는 처리 간에 유의한 차이가 없었으며, 제 3화방에서는 EC 1.8의 높은 농도보다는 0.6의 가장 낮은 농도에서 과경이 더 길었다. 제 4화방에서는 EC $1.8dS{\cdot}m^{-1}$처리에서 가장 과경이 짧았으며 다른 처리 간에는 유의한 차이가 없었다. 과중은 정화방에서는 EC 1.2와 $0.8dS{\cdot}m^{-1}$에서 가장 컸고 높은 농도의 EC $1.8dS{\cdot}m^{-1}$에서 낮았다. 제 2화방에서는 EC $1.8dS{\cdot}m^{-1}$에서 가장 낮았으며 다른 농도 간에는 유의한 차이가 없었다. 제 3화방에서는 처리 간에 유의한 차이가 없었으며, 제 4화방에서는 0.8에서 $1.8dS{\cdot}m^{-1}$까지는 차이가 없었지만 낮은 농도의 $0.6dS{\cdot}m^{-1}$보다는 높은 농도의 $1.8dS{\cdot}m^{-1}$의 과중이 월등하게 낮았다. 과실 내의 가용성 고형물은 각 화방에 따라서 처리 간에 약간의 변화는 있었지만 전반적으로 EC $0.6dS{\cdot}m^{-1}$ 처리에서 가장 높은 경향을 나타내었다. 특히 제 3화방에서는 EC 0.6에서 $1.8dS{\cdot}m^{-1}$까지 배양액의 농도가 높아짐에 따라 가용성 고형물의 함량이 순차적으로 낮아지는 것을 볼 수 있었다. 딸기 '매향'의 수경재배에서 배양액의 EC 관리는 온도가 낮은 저온기에는 EC $0.8-1.2dS{\cdot}m^{-1}$ 농도로 관리하는 것이 좋을 것으로 생각되었다. 이러한 결과는 딸기 수경재배에서 유용하게 활용될 것으로 기대된다.

• 천문학회보
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• 제40권2호
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• pp.41.2-41.2
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• 2015

We have performed deep wide-field CCD photometry of the young open cluster IC 1805 in the famous star forming region W4, and obtained photometric data for more than 91,000 stars in the field of IC 1805 based on observations with the 3.6m CFHT and the AZT-22 1.5m telescope at Maidanak Astronomical Observatory in Uzbekistan. The photometric data cover an area $43^{\prime}{\times}45^{\prime}$ which is far larger and far deeper than any other optical observations made for the cluster. In order to select the young stellar objects with mid-IR excess emission, we have performed mid-IR photometry of the cluster using the archival images obtained with the Spitzer Space Telescope IRAC and MIPS instruments. From a preliminary analysis of the data, we determined the reddening law ($R_V=3.02{\pm}0.05$), distance modulus ($V_0-M_V=11.9{\pm}0.2$), and the spatial distribution of members.

• 천문학논총
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• 제32권1호
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• pp.287-291
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• 2017

We present the results of our mid-infrared (MIR) observations of distant clusters of galaxies with AKARI. The wide-field of view of IRC/AKARI ($10^{\prime}{\times}10^{\prime}$) is ideally suited for studying dust-obscured star-formation (SF) activity of galaxies along the cosmic web in the distant universe. We performed a deep and wide-field $15{\mu}m$ (rest-frame ${\approx}8{\mu}m$) imaging observation of the RXJ1716+6708 cluster (z = 0.81) with IRC. We find that $15{\mu}m$-detected cluster member galaxies (with total infrared luminosities of $L_{IR}{\geq}10^{11}L_{\odot}$) are most preferentially located in the cluster outskirt regions, whilst such IR-luminous galaxies avoid the cluster centre. Our $H{\alpha}$ follow-up study of this field confirmed that a significant fraction of $15{\mu}m$-detected cluster galaxies are heavily obscured by dust (with $AH{\alpha}$>3 mag in extreme cases). The environment of such dusty star-burst galaxies coincides with the place where we see a sharp "break" of the colour-density relation, suggesting an important link between dust-obscured SF activity and environmental quenching. We also report the discovery of a new cluster candidate around a radio galaxy at z = 1.52 (4C 65.22), where we obtained one of the deepest IRC imaging datasets with all the nine filters at $2-24{\mu}m$. This field will provide us with the final, excellent laboratory for studying the dust-enshrouded SF activity in galaxies along the cosmic web at the critical epoch of cluster galaxy evolution with AKARI.

• KSII Transactions on Internet and Information Systems (TIIS)
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• 제9권2호
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• pp.680-699
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• 2015

The use of web service has been increased rapidly, with an increase in the number of available services, finding the exact service is the challenging task. Service discovery is the most significant job to complete the service discoverers needs. In order to achieve the efficient service discovery, we focus on designing a cluster based service discovery model for service registering and service provisioning among all mobile nodes in a mobile ad hoc network (MANETs). A dynamic backbone of nodes (i.e. cluster heads) that forms a service repository to which MANET nodes can publish their services and/or send their service queries. The designed model is based on storing services with their service description on cluster head nodes that are found in accordance with the proposed cluster head election model. In addition to identifying and analyzing the system parameters for finding the effectiveness of our model, this paper studies the stability analysis of the network, overhead of the cluster, and bandwidth utilization and network traffic is evaluated using analytic derivations and experimental evaluation has been done.

• 천문학회지
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• 제35권2호
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• pp.87-95
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• 2002

We have conducted VI CCD photometry of the open cluster NGC 6819 in order to understand the effects of dynamical evolution in old open clusters. Our photometry covers 18' $\times$ 18' on the sky, centered on the cluster, which seems to cover the whole cluster field. Our photometry reaches down to V $\approx$ 20.5, which allows us to analyze the luminosity function and spatial distribution of stars brighter than Mv $\approx$ 8.5. There is a clear evidence for mass segregation in NGC 6819, i.e., the giants and upper main-sequence stars are concentrated in the inner regions, whereas the lower main-sequence stars distribute almost uniformly throughout the cluster. The luminosity function of the main-sequence stars of NGC 6819 is almost flat. The flat luminosity function indicates that a large number of low mass stars has escaped from the cluster unless its initial mass function is much different from the Salpeter type (${\phi}(m){\propto} m^{-(1+x)},x = 1.35$).

• 한국진공학회지
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• 제12권2호
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• pp.105-111
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• 2003

Gas cluster 실험에서 reflectron을 mass selector로서 사용 가능한지를 알아보기 위하여 ‘SIMION’ program을 이용하여 computer simulation하였다. Reflectron 내에서 입자의 비행경로는 질량과는 무관하고 에너지에 따라 변한다. 그러나 $(CO_2)n $ gas cluster의 경우, reflecron을 통과한 직후 cluster의 위치는 cluster의 질량에 따라 공간적으로 분포한다는 것을 알았다. 이것은 cluster의 E/m이 일정하기 때문에 나타난 것으로, 이러한 질량의 공간 분해능이 있기 때문에 reflectron을 mass selector로서 이용할 수 있다는 것을 확인하였다 질량 분해능은 cluster size와 입사각에는 무관하고, 입사위치에 비례한다는 것을 알았다. 이것은 reflectron의 크기를 조정함으로서 질량 분해능을 향상시킬 수 있다는 것을 의미한다. 그러므로 gas cluster 실험에서 reflectron은 질량 분해능이 대단히 우수한 mass selector로서 응용할 수 있다는 것을 확인하였다.

• Journal of Astronomy and Space Sciences
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• 제13권1호
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• pp.55-62
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• 1996

We present UBV CCD photomety of the metal-poor globular cluster M30. The data were obtained using the 40 inch telescope at Mt. Stromlo and Siding Spring Observatory (MSSSO). We used DAOPHOT CCD reduction package in order to obtain Color-Magnitude Diagram (CMD). We have derived some fundametal parameters of the globular cluster such as metal abundance ([Fe/H]), helium abundance (Y), and distance modulus (m-M) from the CMD. The derived parameters were [Fe/H]=-2.50, Y=0.28, and (m-M)=14.64. From the latter, the distance of 8.3kpc is obtained. Despite the photometric uncertainty near the main-sequence turnoff, we estimate the age of M30 to be 1.6${\pm}$3 Gyrs from the Revised Yale Isocyrones. If [O/Fe]=+0.4, this age will be reduced to 14.2${\pm}$3 Gyrs.

• 천문학회보
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• 제38권2호
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• pp.72.2-72.2
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• 2013

We present a UBVI and $H{\alpha}$ photometric study of the young open cluster NGC 1893 in the outer Galaxy as part of "Sejong Open cluster Survey (SOS)" project. Using the properties of early-type stars in the photometric diagrams 65 early-type members were selected. More than 120 $H{\alpha}$ emission stars and candidates were found by $H{\alpha}$ photometry. Together with the published young stellar object catalogue and X-ray source list for this cluster, a total of 837 pre-main sequence (PMS) stars were identified in our photometric data. We obtained the mean reddening of < E(B-V) > = $0.56{\pm}0.08$ mag from the (U-B, B-V) diagram and confirmed the normal reddening law ($R_V=3.1$) toward NGC 1893 based on color excess ratios from optical to mid-infrared wavelengths. The zero-age main sequence fitting to the reddening-corrected color-magnitude diagrams gives a distance modulus of $V_0-M_V=12.8{\pm}0.1$. The age of the cluster inferred from stellar evolution models is about 1-2 Myr. We also found the Salpeter/Kroupa type initial mass function for this cluster. Finally, the mass accretion rate of 80 PMS stars with UV excess emission was estimated for the stars with masses from $0.6M_{\odot}$ to $5M_{\odot}$.

• 천문학회지
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• 제13권1호
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• pp.15-26
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• 1980

The BV-photographic photometry was made for 1714 stars (V<19.5) in NGC 6752. The C-M diagram of this cluster shows an unusually extended blue horizontal branch $(V=13.5{\sim}17.8)$ with a wide gap $(V=16{\sim}16.7)$ and the well defined giant branch with gaps at V=13.85 and 16.2. The turnoff point is defined at $V=17.25{\pm}0.15$ and (B-V) = $0.46{\pm}0.02$. If we take $V_{HB}=13.85$ for NGC 6752, then ${\Delta}V=2.80,\;(B-V)_{0,g}=0.76\;and\;{\Delta}V_{TO}=3.40$ and the chemical abundance is estimated to be [Fe/H]=-1.67 or $Z=4.3{\times}10^{-4}\;and\;Y=0.26$. Some other physical parameters of this cluster are derived and compared with those for the well observed clusters M 3, M 13, M 15 and M 92.

• Nutrition Research and Practice
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• 제13권2호
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• pp.169-177
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• 2019

BACKGROUND/OBJECTIVES: Excessive sugar intake is one of the causes associated with obesity and several chronic diseases prevalent in the modern society. This study was undertaken to investigate the effect of parenting variables based on the theory of planned behavior, on the sweetness preferences and sweets intake of children. SUBJECTS/METHODS: Parents and their children (n = 103, aged 5-7 years) were enrolled to participate in a survey for this study, after providing the required informed consent. Parents were asked to fill out a self-administered questionnaire at their residence. The sweetness preference test for children was conducted at a kindergarten (or daycare center) by applying the one-on-one interview method. RESULTS: The children were divided into two clusters categorized by the K-mean cluster analysis: Cluster 1 had higher sweetness preference (0.42 M sugar, 35%; 0.61 M sugar, 65%); Cluster 2 exhibited lower sweetness preference (0.14 M sugar, 9.5%; 0.20 M sugar, 9.5%; 0.29 M sugar, 81%). Cluster 1 had a higher frequency of sweets intake (P < 0.01), and lower sweets restriction (P < 0.05) and nutrition quotient score (P < 0.05). Sweets intake was negatively correlated with the nutritional quotient (r = -0.204, P < 0.05). The behavioral intention of parents was higher in cluster 2 (P < 0.05), while affective attitude, feeding practice, and reward were higher in cluster 1 (P < 0.001, P < 0.05, and P < 0.01, respectively). Furthermore, behavioral intention of parents showed a negative correlation with affective attitude (r = -0.282, P < 0.01) and feeding practice (r = -0.380, P < 0.01), and a positive correlation with subjective norm (r = 0.203, P < 0.05) and parenting attitude (r = 0.433, P < 0.01). CONCLUSIONS: This study indicates that the sweetness preferences and sweets intake of children is related to the parent's affective attitude, feeding practice and reward. We suggest that to reduce the sugar consumption of children, guidelines for access to sweets and pertinent parenting practices are required.