In the region of the intermediate open cluster M35 (NGC 2168), the time-series of V CCD images was taken for 12 nights from December 18, 2007 to September 25, 2010. From this observation, we detected 22 variable stars including 15 new ones. They are 6 δ Scuti, a Cepheid, an RR Lyrae, 9 eclipsing binaries and 5 semi-long periodic and/or slow irregular type variable stars. For the V photometry of the δ2 Scuti stars, the multi-frequency analysis was performed using the Discrete Fourier Transform and the linear least-square fitting.

본 연구는 하이부쉬 블루베리(Vaccinium corymbosum) 'Jersey' 품종을 이용하여 적방 1/3, 적방 1/3 +적화 1/2, 적방 2/3 및 적방 2/3 + 적화 1/2처리 후 무처리 과실의 수확량과 과실 품질을 조사하여 적방 적화 정도에 따른 수량과 과실 크기, 가용성당함량, 산함량, 과실 경도를 분석하였다. 적방 적화 처리는 과립중, 종경 및 횡경에 유의한 과립 비대효과를 가져왔다. 과실 수확량은 무처리와 적방 1/3 처리구에서 가장 높았으며, 그 이외의 처리에서는 과립비대는 이루어졌으나 수확량의 감소가 발생하였다. 무처리와 적방 1/3 처리의 경우 전체 수확량은 비슷하였으나, 적방 1/3 처리구에서는 상품성이 큰 대립의 과실이 차지하는 비율이 무처리에 비해서 큰 것으로 조사되었다. 가용성당함량은 적방과 적화 처리에 따라 수량이 감소한 적방 2/3, 적방 2/3 + 적화 1/2 처리구에서 유의하게 증가하였으나, 산함량과 경도에는 영향을 미치지 않았다. 적방 적화에 따른 영향은 과립 비대와 수량에 유의한 차이를 주었으나 과실품질에는 크게 영향을 미치지 않는 것으로 조사되었다.

Taking the great advantage of Subaru's wide field coverage both in the optical and in the near infrared, we have been providing panoramic views of distant clusters and their surrounding environments over the wide redshift range of 0:4 < z < 3. From our unique data sets, a consistent picture has been emerging that the star forming activity is once enhanced and then truncated in galaxy groups in the outskirts of clusters during the course of cluster assembly at z < 1. Such activity is shifted into cluster cores as we go further back in time to z ~ 1.5. At z = 2 - 2.5, we begin to enter the epoch when massive galaxies are actually forming in the cluster core. And by z ~ 3, we eventually go beyond the major epoch of massive galaxy formation. It is likely that the environmental dependence of star forming activity is at least partly due to the external environmental effects such as galaxy-galaxy interaction in medium density regions at z < 1, while the intrinsic effect of galaxy formation bias overtakes the external effect at higher redshifts, resulting in a large star formation activity in the cluster center.

The core and global properties of the early-type ("red sequence") galaxies in the Virgo and Fornax clusters are examined using high-quality HST/ACS imaging for 143 galaxies. Rather than dividing neatly into disparate populations having distinct formation and/or evolution histories, many of the core and global properties of these galaxies show smooth and systematic variations along the galaxy luminosity function. The few examples of the rare class of compact elliptical galaxies in our sample all show properties that are strongly suggestive of tidal stripping by massive galaxies; if so, then these systems should not be viewed as populating the low-luminosity extension of so-called "normal" elliptical sequences. These results demonstrate that complete and/or unbiased samples are a pre-requisite for identifying the physical mechanisms that gave rise to the early-type galaxies we observe locally, and how these mechanisms varied with mass and environment.

Recently, to improve operating efficiency with the higher in-line rate in automated production lines, a lot of cases of grouping machines and material handling system together to form a cluster has shown frequently. This article addresses the job allocati

UBVI CCD photometry is obtained for the Ruprecht 93 (Ru 93)region. We are unable to confirm the existence of an intermediate-age open cluster in Ru 93 from the spatial distribution of blue stars. On the other hand, we find two young star groups in the observed field: the nearer one (Ru 93 group) comprises the field young stars in the Sgr-Car arm at d ≈ 2.1 kpc, while the farther one (WR 37 group) is the young stars around WR 37 at d ≈ 4.8 kpc. We derive an abnormal extinction law (RV = 3.5) in the Ruprecht 93 region.

We study the dynamical evolution of the M87 globular cluster (GC) system using the most advanced and realistic Fokker-Planck (FP) model.By comparing our FP models with both mass function (MF) and radial distribution (RD) of the observed GC system, we find the best-fit initial (at M87's age of 2-3 Gyr) MF and RD for three GC groups: all GCs, blue GCs, and red GCs. We estimate the initial total mass in GCs to be 1.8+0.3-0.2 X 1010⊙, which is about 100 times larger than that of the Milky Way GC system. We also find that the fraction of the total mass currently in GCs is 34%. When blue and red GCs are fitted separately, blue GCs initially have a larger total mass and a shallower radial distribution than red GCs. If one assumes that most of the significant major merger events of M87 have ended by the age of 2-3 Gyr, our finding that blue (metal-poor) GCs initially had a shallower radial distribution supports the major merger scenario for the origin of metallicity bimodality.

Recently, to improve operating efficiency with the higher in-line rate in automated production lines, a lot of cases of grouping machines and material handling system together to form a cluster has shown frequently. This article addresses the job allocation and operation method of automated material handling for cluster-type production systems. First of all, the control problems of the automated material handling systems are classified into the control problem of inter-cluster material handling system and that of intra-cluster material handling system. Then, a distributed agent-based control scheme is proposed for the former, and an operational control procedure for the latter. Simulation experiment shows that the proposed method is efficient in reducing cycle times and improving utilization of material handling vehicles.

게임분야에서 몰입감을 높이고 게이머의 만족도를 높일 수 있는, 프로젝터 기반 고해상도 대형 디스플레이를 사용 한 게임이 지속적으로 연구되고 있다. PC 클러스터를 사용한 프로젝터 기반 대형 고해상도 타일드 디스플레이 시스템 은 대형 고해상도 타일드 디스플레이 시스템 분야에서 주요한 연구가 되었다. 많은 연구자들은 이 대형 고해상도 타 일드 디스플레이 시스템에 영향을 미치는 주요한 요인 중 클러스터 알고리즘, 고성능 그래픽 렌더링 기술, 고속 네트웍 등을 지속적으로 연구되어왔다. 그럼에도 불구하고 고해상도 타일드 디스플레이 시스템의 각 요소들을 전체적으로 조망하여 실제적인 고해상도 타일드 디스플레이 구축 과정을 보여주는 연구는 이루어지지 않았다. 본 논문에서는 고 해상도를 가지는 대형 디스플레이를 사용한 게임 시스템, PC 클러스터를 이용한 프로젝터 기반 대형 고해상도 디스플레이 시스템을 구축하는 데 필요한 각 요소 기술들을 서베이하여 보여주고, 이와 더불어 PC 클러스터를 이용한 프로젝터 기반 대형 고해상도 디스플레이 시스템의 구축에 실제 사용된 기술을 소개한다. 결과적으로 PC 클러스터를 이용 한 프로젝터 기반 대형 고해상도 디스플레이 시스템을 구축하고자 고려하는 연구자 및 업체가 시스템 구축을 쉽고 효율적으로 할 수 있도록 해 줄 수 있을 것이다.

Next to Paper I (Jeon 2009a), time-series BV CCD images of the open cluster M38 were taken for 4 nights on December, 2009. The observations have been carried out for total 27 nights. In addition to the 20 variable stars in the Paper I, the discovery of 44 new variable stars has been presented in this paper: 6δ Scuti stars, 2γ Doradus stars, 18 eclipsing binaries and 18 semi-long periodic and/or slow irregular type variable stars. For the V photometry of the δ Scuti and γ Doradus stars, multi-frequency analysis was performed using the Discrete Fourier Transform and linear least-square fitting. The period search for the eclipsing binaries and the semi-long periodic and/or slow irregular type variable stars was performed by phase fitting method. As a result, the periods for 23 variable stars among the 44 ones were defined.

In 450mm wafers production environment for next generation Fab, one of the most significant features is the adoption of full automation to the whole manufacturing processes involved. The full automation system will prevent the workers from intervening the manufacturing processes as much as possible and increase the importance of each individual wafer noticeably, and thus require a more robust scheduling system for entire semiconductor manufacturing processes. The scheduling system for 450mm wafers production also should be capable of monitoring the status of each individual wafer and collecting useful Fab data in real time. In this study, we first analysis of cluster tool in 450mm wafers production environment, and then propose a real-time scheduling algorithm based on timetabling algorithm.