The genus Glyphodes Guenée, 1854 reported over 150 species in the world. They are widely distributed throughout tropical regions, with some species penetrating into subtropical and warm temperate areas. Five species of the genus Glyphodes Guenée are reported for the first time in Laos: Glyphodes actorionalis Walker, G. bivitralis Guenée, G. caesalis Walker, G. extorris Dognin, and G. stolalis Guenée. Photographs of adult, male and female genitalia, with short description

We present a summary of our spectroscopic redshift catalogue of 404 sources in the AKARI Deep Field South (ADF-S). We have used the AAOmega spectrograph to target mid-infrared and far-infrared sources selected primarily from AKARI observations in this field for which we were able to obtain optical counterparts. Our sources with identified redshifts include 316 with Hα detections at z  0:345 and 15 sources at z > 1 with MgII or Ly emission lines. About 13% of our z  0:345 sources are dominated by active galactic nuclei (AGN) emission, although many show emission from both star formation and AGNs. The median Balmer decrement is 5.9. Ultra-luminous infrared galaxies (ULIRGs) were found only in the higher-redshift sources. Optical and near infrared data will be available shortly, enabling calibration of the line luminosities and spectral energy distribution (SED) tting for these sources.

The extragalactic background suggests half the energy generated by stars was reprocessed into the infrared (IR) by dust. At z1.3, 90% of star formation is obscured by dust. To fully understand the cosmic star formation history, it is critical to investigate infrared emission. AKARI has made deep mid-IR observation using its continuous 9-band filters in the NEP field (5.4 deg2), using 10% of the entire pointed observations available throughout its lifetime. However, there remain 11,000 AKARI infrared sources undetected with the previous CFHT/Megacam imaging (r ~25.9ABmag). Redshift and IR luminosity of these sources are unknown. These sources may contribute signicantly to the cosmic star-formation rate density (CSFRD). For example, if they all lie at 1< z <2, the CSFRD will be twice as high at the epoch. We are carrying out deep imaging of the NEP eld in 5 broad bands (g; r; i; z; and y) using Hyper Suprime-Camera (HSC), which has 1.5 deg field of view in diameter on Subaru 8m telescope. This will provide photometric redshift information, and thereby IR luminosity for the previously-undetected 11,000 faint AKARI IR sources. Combined with AKARI's mid-IR AGN/SF diagnosis, and accurate mid- IR luminosity measurement, this will allow a complete census of cosmic star-formation/AGN accretion history obscured by dust.

고준위방사성폐기물 심층처분에서 처분안전성의 신뢰도를 향상시킬 수 있는 방안으로 그리고 처분 프로그램 개발 및 인허가를 위해 많은 나라들에서 자국에 적합한 safety case를 개발하고 있다. 본 연구에서는 방사성폐기물 처분을 위한 safety case 의 의의, 필요성, 개발과정들을 정리하고 소개하였다. 그리고 처분안전성을 safety case의 다양한 측면에서 논의하였다. 아울러 스위스, 일본, 미국, 스웨덴, 핀란드 등 해외의 safety case 개발 현황과 현재 KAERI에서 개발 중인 safety case의 개발 전략을 간략히 소개하였다. 고준위방사성폐기물 처분안전성의 신뢰도 향상을 위해 safety case 기반 하에서 어떤 노력들이 필요한지를 분석하였다. 그리고 국내 상황을 반영하여 신뢰할 수 있는 정보자료의 구축, 안전성 관련 과정들의 이해, 안전성 평가의 불확실성 저감, 이해당사자와의 의사소통, 공정성과 투명성 확보 등의 실행 방안을 제안하고 논의하였다. 본 논문에 제시된 내용들은 심층처분 safety case를 이해하고, 국내에서 개발하고 있는 고준위방사성폐기물 처분 safety case 개발을 통한 처분안전성 신뢰도 향상에 기여할 수 있을 것으로 기대한다.

Five species of the genus Glyphodes Guenée (Lepidoptera, Crambidae) are reported for the first time in Laos: Glyphodes actorionalis Walker, G. bivitralis Guenée, G. caesalis Walker, G. extorris Dognin, and G. stolalis Guenée. Illustrations of adults and genitalia, distribution are provided.

Every day, large amounts of personal information are collected by private companies from consumers through multiple sources. Loyalty programs are one of the most popular tools, used to gather such information. Information that is used to offer more personalised options and to target more effectively their promotions. However, many consumers are still attracted to such programs because of the rewards and other benefits offered. Privacy concerns over loyalty programs seem to take their toll. According to a Colloquy (2015) report the numbers of active members is dropping and one of the main reasons cited in the report is privacy concerns. Declining numbers and increased privacy concerns raise the question of how concerned consumers appreciate the benefits offered by loyalty programs and how their satisfaction and loyalty are affected. Apparently, loyalty programs cannot always guarantee loyalty (Nielsen, 2013) as a large portion of consumers demand better protection of their privacy (Madden, 2014) and decline to subscribe to such programs over privacy concerns (Maritz, 2013). The objectives of this study are firstly to examine the underlying reasons behind consumers’ privacy perceptions and secondly to investigate how such perceptions alter consumers’ appraisal of the benefits offered by the loyalty program as well as satisfaction with the program and consumer loyalty. Based on a review of the relevant literature a set of testable hypotheses was developed.

The main objective of this paper is to elucidate the present status of Plant Genetic Resources (PGRs), their research, and management system in the genebank of Nepal. PGRs for food and agriculture are the biological basis of world food and nutrition security. The remarkable elevation ranging from 60 meter above sea level (masl) to highest summit Mount Everest (8,848 masl) has created huge geographical and climatic variation which harbor enormous plant species in the country. National Agriculture Genetic Resource Center (NAGRC) or ‘Genebank’ currently conserved 11,051 accessions of more than 110 crops species belonging to cereals (5,850), pseudo cereals (1,150), pulses (1,800), oilseeds (185), and vegetables (565) including other crops (1,501) at ex-situ. Diversity mapping, characterization and evaluation of PGRs, duplicates identification, diversity study, pre-breeding and landrace enhancement are the major research works of NAGRC, and its management strategies include conservation method, types, and groupings of PGRs. Characterization, evaluation and tagging of economically important traits in PGRs are now more important for strengthening their pre-breeding and proper utilization. Additionally, strong communication and collaborative network among public, private, community based organizations and international organizations are important for the effective management of PGRs.

Arctiinae are one of the most species-rich subfamily in the family Erebidae (or classified as family Arctiidae). Around 11.155 species of 750 genera have been described from all over the world (Heppner, 2005) of which 5.931 inhabit the Neotropics (Watson & Goodger, 1986; Heppner, 1991; Scoble, 1995). Taxonomic study of the Arctiinae in Cambodia has been done by a few foreign entomologists. As the results of this study, 182 species of 68 genera are reported on, of which described in recent pages 135 species of 44 genera are reported from Cambodia for the first time, five species are new to science (Bayarsaikhan & Bae, 2015; Bayarsaikhan et al., 2015; Bayarsaikhan & Bae, 2016): Danielithosia wooshini; Stictane cambodiensis; S. khmerensis; S. bokorensis; Cyana angkorensis. The materials for identification are based on the collection of Incheon National University, which were collected from 2009-2015 in Cambodia by Cambodian and Korean researchers.

The marine microalgae Isochrysis galbana was cultured under various light–emitting diode (LED) light conditions with different wavelengths to examine changes in growth and in amino acid and fatty acid profiles. The culture conditions for the microalgae were Conway medium, salinity of 33 psu, temperature of 24°C, and a 16/8 h light/dark photoperiod. Six light sources, including 5 units of 180W LED lamps (peak wavelength: blue [LB] 470 nm; green [LG] 525 nm; yellow [LY] 595 nm; red [LR] 636 nm; white [LW] 442 nm) and 1 unit of a 175W metal halide (MH) lamp, were used for the experiment. The dry cell weights (gL–1) of I. galbana under different light conditions were in the order of LW>LB≥MH>LR>LG>LY. Levels of essential amino acids were revealed to be significantly higher under LW, LG, and MH than under the other wavelengths (P<0.05). The fatty acid, unsaturated fatty acid, and DHA contents of I. galbana were higher under MH, LW, and LG. In addition, the carotenoid content was higher under MH, LW, and LG than under the other wavelengths (P<0.05). The fucoxanthin content was highest under MH (0.28%) and lowest under LY (0.2%), and it was 0.26% under LW and LG. The results indicate that the combined use of LW and LG is effective when using LED lamps for I. galbana cultivation.

A new facility, known as Pyrel III, has been installed at ENEA laboratories for pyrochemical process studies under inactive conditions. It is a pilot plant which allows electrorefining and electroreduction experiments to be conducted on simulated fuel. The main component of the plant is a zirconia crucible. The crucible is heated by a furnace which is supported in an externally water-cooled well under the floor of a steel glove-box, where an argon atmosphere is maintained by a continual purge of about 10 L·min-1. The vessel is loaded with LiCl-KCl eutectic salt (59-41 mol%) and is currently operated at 460 °C. Several improvements on Pyrel II (the previous operating plant) have been introduced into Pyrel III. They are described in detail, together with the results from the first experimental campaign which used lanthanum metal.Moreover, studies about the treatment of chloride salt wastes from pyroprocesses have been conducted in parallel. They follow two main routes: on one hand, a matrix termed sodalite, a naturally occurring mineral containing chlorine, has been synthesized from a mix of nepheline, simulated exhausted salts and glass frit; on the other hand, a novel method proposed by Korea Atomic Energy Research Institute (KAERI) is under assessment. The final waste forms have been fully characterized with the support of the Politechnique of Milan, by means of density measurements, thermal analysis, and stereomicroscopy observations, FTIR, XRD, and RAMAN spectra, as well as leach tests under static conditions.

We have investigated the long term variability of the intensities of the broad-line region emission lines in the UV spectra of Seyfert I galaxy NGC 5548 from 1973-1996. We have obtained the following results: 1) a high level correlation between the intensities of emission lines as well as between intensities of emission lines and continuum uxes was discovered. With increasing wavelength the correlation in both cases becomes weaker, 2) the relationship between the intensity of emission lines and the ux radiation in the continuum can be expressed by a power law function with coefficients of α ≈ 0:8 - 1:1 for different lines. When the difference between the wavelengths of spectral lines and the continuum is increased, the value of the power function decreases, and 3) it was found that the magnitude of the variability of the line intensities are weaker than the range of variability of the continuum uxes. The magnitude of the variability of the line intensities and the continuum uxes increase at longer wavelengths.

Hydroxyapatite (HA), which is an important calcium phosphate mineral, has been applied in orthopedics, dentistry, and many other fields depending upon its morphology. HA can be synthesized with different morphologies through controlling the synthesis method and several parameters. Here, we synthesize various morphologies of HA using two simple methods: hydrothermal combustion and solution combustion. The phase purity of the synthesized HA is confirmed using X-ray diffractometry. It demonstrates that pure phased hydroxyapatite can be synthesized using both methods. The morphology of the synthesized powder is examined using scanning electron microscopy. The effects of pH and temperature on the final powder are also investigated. At 140 oC, using the hydrothermal method, nano-micro HA rods with a hexagonal crystal structure can be synthesized, whereas using solution combustion method at 600 oC, a dense cubic morphology can be synthesized, which exhibits monoclinic crystal structures.

We studied a cluster family in the northern part of the Carina Nebula (NGC 3372) a group of clusters near NGC 3324 (Tr 15, NGC 3293, Loden 165, Loden 153 and IC 2581). We used data from UCAC4 to determine the cluster's membership and the near infrared CMDs of each cluster. We analyzed the spatial density and elongation as a function of radius for each cluster and found a possible interaction between NGC 3293 and Loden153. However, the shape distortion of NGC 3324 cannot be evaluated because of the inhomogenity in the coverage of UCAC4 in the east part of NGC 3324.