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이창무,김병욱,이현 한국부동산분석학회 2002 不動産學硏究 Vol.8 No.2
Stock price index type of housing price indices were commonly used in Korea. However, this type of indices are not suitable for Korean housing market experiencing rapid changes in stock including both new constructions and demolitions. Especially, the recent Korean housing market has experienced substantial changes in housing characteristics. Basically, the stock price index type of housing price index requires a constant survey stock over time in order to maintain the comparability in total housing values. However, the constant stock concept is hard to accept in the Korean housing market accompanying with rapid increase and qualitative changes in housing stock. An alternative is a hedonic price index. However, the basic data requirements for the application of the hedonic model cannot be fulfilled in the Korean housing market where actual sale information is mostly unknown. In order to overcome this structural deficiency, the price indices in Korea are based o periodical price survey with the help of real estate brokers. If we accept the assumption that the whole condominium units belonging to a basic survey unit (an area type in an condominium complex) share the same housing characteristics and the surveyed price, we can use the repeat sale index concept with some modifications. The persistent price survey generates a perfect form of repeat sales data. This paper proposes a practical method for the application of repeat sale index to condominium sales price indexing.
Layer-by-Layer Assembly for Graphene-Based Multilayer Nanocomposites: Synthesis and Applications
Lee, Taemin,Min, Sa Hoon,Gu, Minsu,Jung, Yun Kyung,Lee, Wonoh,Lee, Jea Uk,Seong, Dong Gi,Kim, Byeong-Su American Chemical Society 2015 Chemistry of materials Vol.27 No.11
<P>Two-dimensional (2D) graphene sheets have become a versatile platform for the fabrication of innovative hybrid materials with various functions due to their unique electrical, optical, thermal, and mechanical properties. The preparation of graphene-based composites with nanoscale precision is highly important for reproducible and controllable performance through the analysis of interplay between each component. In particular, the layer-by-layer (LbL) assembly technique is known as a simple, inexpensive, and versatile process for the fabrication of highly ordered multilayer film structures from various types of materials. The LbL structures capable of controlling nanoscale composition and architectures are achieved through the sequential adsorption of oppositely charged components by attractive forces such as electrostatic interactions. In this review, we will focus on the recent progress in graphene-based nanocomposites hybridized with various nanomaterials such as carbon nanomaterials, polymers, and inorganic nanoparticles by the LbL assembly. Multilayered graphene nanocomposites exhibit improved physical/chemical properties and superior performance compared with the individual components due to the synergistic effects in various applications including electric devices, energy storage and conversion, and biological usages.</P><P><B>Graphic Abstract</B> <IMG SRC='http://pubs.acs.org/appl/literatum/publisher/achs/journals/content/cmatex/2015/cmatex.2015.27.issue-11/acs.chemmater.5b00491/production/images/medium/cm-2015-00491c_0013.gif'></P>
THE TRIPLY ECLIPSING HIERARCHICAL TRIPLE STAR KIC002856960
Lee, Jae Woo,Kim, Seung-Lee,Lee, Chung-Uk,Lee, Byeong-Cheol,Park, Byeong-Gon,Hinse, Tobias Cornelius IOP Publishing 2013 The Astrophysical journal Vol.763 No.2
<P>In a recent study, Armstrong et al. presented an eclipsing binary star of about 6.2 hr period with transit-like tertiary signals occurring every 204.2 days in the Kepler public data of KIC002856960 and proposed three possible hierarchical structures: (AB) b, (AB) C, and A(BC). We analyzed the Kepler light curve by including a third light source and one starspot on each binary component. The results represent that the close eclipsing pair is in a low-mass eccentric-orbit, detached configuration. Based on 123 eclipse timings calculated from the Wilson-Devinney binary model, a period study of the close binary reveals that the orbital period has experienced a sinusoidal variation with a period and a semi-amplitude of 205 +/- 2 days and 0.0021 +/- 0.0002 days, respectively. The period variation would be produced by the light-travel-time effect due to a gravitationally bound third body with a minimum mass of M-3 sin i(3) = 0.76 M-circle dot in an eccentric orbit of e(3) = 0.61. This is consistent with the presence of third light found in our light curve solution and the tertiary signal of 204.2 day period most likely arises from the K-type star crossed by the close eclipsing binary. Then, KIC002856960 is a triply eclipsing hierarchical system, A(BC), consisting of a close binary with two M-type dwarfs and a more massive K-type component. The presence of the third star may have played an important role in the formation and evolution of the close pair, which may ultimately evolve into a contact system by angular momentum loss.</P>