In a previous study, it was reported that enzymatic hydrolysis under pressurization could be a new method which could produce arginine dipeptide and free amino acid in anchovy hydrolysate as salty enhancer at optimal condition. Powder is more efficient than liquid in terms of transport and storage stability. For the purpose of producing spray dried powder of various salt contents was investigated the effect of different salt concentration of anchovy hydrolysate on spray dried powder properties. The anchovy hydrolysate of various salt contents(in the range of approximately 0.7- 19.8% w/w) prepared adding the fish sauce (Dae-Young fish market) at inlet drying air temperatures of 120°C and 140°C. The process yield and physicochemical properties such as moisture content, bulk density, hygroscopicity and the morphology (EDS, XPS, XRD) of the anchovy hydrolysate powder was measured. The glass transition temperatures (Tg) of the powders equilibrated under various water activities were determined using a differential scanning calorimeter (DSC). Different drying conditions and salt concentration could generate anchovy hydrolysate powders with different process yield, bulk density and moisture content. The spray-dried anchovy hydrolysate powder was confirmed by XRD to be a mixture of an amorphous substances and crystalline salts. The energy dispersive X-ray spectrometer (EDS) and X-Ray Photoelectron Spectroscopy (XPS) analysis demonstrated that the surface NaCl concentration of the powders increased with an increasing drying air temperature. Increasing moisture adsorption of the anchovy hydrolysate powders resulted in a Tg reduction. It is suggested that producing spray dried anchovy hydrolysate for the industrial use is the use of the feed salt concentration of not lower than % w/w and inlet air temperature at 120°C, 140°C

We demonstrated the sensitivity of optically active single-walled carbon nanotubes (SWCNTs) with a diameter below 1 nm that were homogeneously dispersed in cement composites under a mechanical load. Deoxyribonucleic acid (DNA) was selected as the dispersing agent to achieve a homogeneous dispersion of SWCNTs in an aqueous solution, and the dispersion state of the SWCNTs were characterized using various optical tools. It was found that the addition of a large amount of DNA prohibited the structural evolution of calcium hydroxide and calcium silicate hydrate. Based on the in-situ Raman and X-ray diffraction studies, it was evident that hydrophilic functional groups within the DNA strongly retarded the hydration reaction. The optimum amount of DNA with respect to the cement was found to be 0.05 wt%. The strong Raman signals coming from the SWCNTs entrapped in the cement composites enabled us to understand their dispersion state within the cement as well as their interfacial interaction. The G and G’ bands of the SWCNTs sensitively varied under mechanical compression. Our results indicate that an extremely small amount of SWCNTs can be used as an optical strain sensor if they are homogeneously dispersed within cement composites.

Bee venom contains a variety of peptide constituents, including low-molecular-weight protease inhibitors. While the putativelow-molecular-weight serine protease inhibitor Api m 6 containing a trypsin inhibitor-like cysteine-rich domain was identifiedfrom honeybee (Apis mellifera) venom, no anti-fibrinolytic or anti-microbial roles for this inhibitor have been elucidated.In this study, we identified an Asiatic honeybee (A. cerana) venom serine protease inhibitor (AcVSPI) that was shownto act as a microbial serine protease inhibitor and plasmin inhibitor. AcVSPI was found to consist of a trypsin inhibitor-likedomain that displays ten cysteine residues. Interestingly, the AcVSPI peptide sequence exhibited high similarity to the putativelow-molecular-weight serine protease inhibitor Api m 6, which suggests that AcVSPI is an allergen Api m 6-like peptide.Recombinant AcVSPI was expressed in baculovirus-infected insect cells, and it demonstrated inhibitory activity against trypsin,but not chymotrypsin. Additionally, AcVSPI has inhibitory effects against plasmin and microbial serine proteases; however,it does not have any detectable inhibitory effects on thrombin or elastase. Consistent with these inhibitory effects, AcVSPIinhibited the plasmin-mediated degradation of fibrin to fibrin degradation products. AcVSPI also bound to bacterial andfungal surfaces and exhibited anti-microbial activity against fungi as well as gram-positive and gram-negative bacteria. Thesefindings demonstrate the anti-fibrinolytic and anti-microbial roles of AcVSPI as a serine protease inhibitor.

The ability of plants to endure environmental stress factors, which are going to be more severe due to global warming, is important especially for forest plants. Because obtain trait of resistance to temperature using conventional breeding for woody plants is a time consuming way. In this study, chloroplast-localized OsHSP26 gene was overexpressed in Populus alba L. to breed tolerant transgenic poplar to temperature stress. The plantlets of OsHSP26-overexpressed transgenic poplar showed more heathy phenotypic response than wild-type plants under both prolonged low- and high-temperature stress. While the SPAD value, which refers chlorophyll content, in wild-type plants decreased depending on the exposure time to the temperature stress, higher SPAD value were shown in the transgenic plants. The contents of total phenolic compounds in the transgenic plants were lower than those of the wild-type plants, and not significantly changed except in the treatment of prolonged low-temperature. However, the total flavonoids contents of the transgenic plants were dramatically increased under prolonged temperature stress. The DPPH scavenging activities of the transgenic plants were higher than those of the wild-type plants under temperature stress. Consequently, it was revealed that overexpressing OsHSP26 allow for P. alba to be tolerant to temperature stress.

in vitro studies on salt torerance was carried out with Salix gracilistyla. Shoot growth of plants treated with NaCl showed statistically significances among different levels of concentration(0~200 mM) on 1/2MS medium. Plant growth was not grown at in higher concentration than 75 mM and plants were dead over 150 mM Nacl Browned leaf was observed from 14 days at higher concentration than then 75 mM NaCl, and chlorophyll content was dramatically decreased. Main roots and rootlet in same concentrates(75 mM) or high NaCl treatment were changed the color to black. The proline and sugar contents were dramatically increased in the higher than 75 mM NaCl treatments after 14 - 15 days. To determine NaCl and minerals in salt stressed plants, leaf, stem and root of in vitro plant were subjected to ICP analysis. Na content was increased with culture days in all three parts. These results suggest that S. gracilistyla can be used vegetative restoration in coastal wetlands reclaimed.

The aim of this study was to use an in vitro method and estimate glycaemic index (GI) from porridges to determine the digestibility of porridges. Glycaemic index’s concept is to classify foods on the basis of their postprandial blood glucose response. The GI of a foodstuff is generally measured by determining the increment in blood glucose concentration after the consumption of a test meal over a set period of time and comparing it with an isoglucosidic control meal (normally white bread or glucose) and expressed as a percentage. In this study, the 5 porridges were studied for their starch digestibility. The available starch contents of the samples varied from 65~85 g/100 g dry solids. From in vitro digestion, the porridge samples were Medium glycaemic index foods with calculated GIs ranging from 56 to 67.

The present paper proposes an categorization of commercial fluid products. A total of 21 commercial fluid products were analyzed(porridges, universal design foods, foods for special medical purposes) corresponding to 11 different commercial brands. Joint consideration has been made of viscous behavior (flow and thixotropy) and viscoelastic behavior (oscillatory testing). Rheological measurements were fitted to different rheological mathematical models, and a total of 4 parameters were generated. Our results correspond to three different classes. The three defined classes have been named in a way similar those most commonly used in the literature. Each class has been defined from the parameters allows us to know the common rheological characteristics of any of the products belonging to a given class.

Agrobacterium tumefaciens-mediated transformation (AtMT) has been widely used for generation of fungal transformants and recently applied to Beauveria bassiana. In this study to comprehend how the AtMT promoter influences on the expression of selection marker (hygromycin B resistance gene; hph), two different Ti-Plasmids were constructed: pCeg (gpdA promoter-based) and pCambia-egfp (CaMV 35S promoter-based). Putative transformants were subjected to the PCR, RT-PCR and qRT-PCR to inspect the T-DNA insertion rate and gene expression level. In conclusion, more than 80% of the colonies succeeded in AtMT transformation and the hph expression level of AtMT/pCeg colonies was higher than that of AtMT/pCambia-egfp colonies. This result can provide useful information on the AtMT of B. bassiana, especially antibiotics susceptibility and promoter-dependant expression level.

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.

There exists strong evidence supporting the co-evolution of central supermassive black holes and their host galaxies; however it is still under debate how such a relation comes about and whether it is relevant for all or only a subset of galaxies. An important mechanism connecting AGN to their host galaxies is AGN feedback, potentially heating up or even expelling gas from galaxies. AGN feedback may hence be responsible for the eventual quenching of star formation and halting of galaxy growth. A rich multi- wavelength dataset ranging from the X-ray regime (Chandra), to far-IR (Herschel), and radio (WSRT) is available for the North Ecliptic Pole field, most notably surveyed by the AKARI infrared space telescope, covering a total area on the sky of 5.4 sq. degrees. We investigate the star formation properties and possible signatures of radio feedback mechanisms in the host galaxies of 237 radio sources below redshift z = 2 and at a radio 1.4 GHz ux density limit of 0.1 mJy. Using broadband SED modelling, the nuclear and host galaxy components of these sources are studied simultaneously as a function of their radio luminosity. Here we present results concerning the AGN content of the radio sources in this eld, while also offering evidence showcasing a link between AGN activity and host galaxy star formation. In particular, we show results supporting a maintenance type of feedback from powerful radio-jets.

We carry out the study of 850 μm sources in a part of the XMM-LSS field. The 850 μm imaging data were obtained by the SCUBA-2 on the James Clerk Maxwell Telescope (JCMT) for three days in July 2015 with an integration time of 6.1 hours, covering a circular area with a radius of 15′. We choose the central area up to a radius of 9.′15 for the study, where the noise distribution is relatively uniform. The root mean square (rms) noise at the center is 2.7 mJy. We identify 17 sources with S/N > 3.5. Differential number count is estimated in flux range between 3.5 and 9.0 mJy after applying various corrections derived by imaging simulations, which is consistent with previous studies. For detailed study on the individual sources, we select three sources with more reliable measurements (S/N > 4.5), and construct their spectral energy distributions (SEDs) from optical to far-infrared band. Redshift distribution of the sources ranges from 0.36 to 3.28, and their physical parameters are extracted using MAGPHYS model, which yield infrared luminosity LIR = 1011.3−1013.4 L⊙, star formation rate SFR = 101.3−103.2 M⊙yr−1 and dust temperature TD = 30−53 K. We investigate the correlation between LIR and TD, which appears to be consistent with previous studies.

In this study, cellulose nanoplates (CNPs) were fabricated using cellulose nanocrystals obtained from commercial microcrystalline cellulose (MCC). Their pyrolysis behavior and the characteristics of the product carbonaceous materials were investigated. CNPs showed a relatively high char yield when compared with MCC due to sulfate functional groups introduced during the manufacturing process. In addition, pyrolyzed CNPs (CCNPs) showed more effective chemical activation behavior compared with MCC-induced carbonaceous materials. The activated CCNPs exhibited a microporous carbon structure with a high surface area of 1310.6 m2/g and numerous oxygen heteroatoms. The results of this study show the effects of morphology and the surface properties of cellulose-based nanomaterials on pyrolysis and the activation process.

The Korea Mushroom Resource Bank (KMRB) was launched as a national research resource bank in 2015 by the Ministry of Science, ICT and Future Planning. The main goal of the KMRB is to secure important biological resources, mushroom-forming basidiomycota, significant sources of fundamental and novel substances and materials, as dried specimen, cultures, and genomic DNA. For wider application of fungal resources in education, medicinal and industrial uses, the KMRB will undertake following tasks: 1) Survey natural environments across Korea to catalogue mushroom diversity, 2) Establish resource management system based on accurate identification of mushroom, 3) Evaluate the usefulness of the discovered mushroom, 4) Create a secure preservation and loan system. With a global focus on utilizing natural resources, mushroom resources provide excellent opportunities for academic research, and discovering novel substances for use as medicine and energy.

We present an optical imaging survey of AKARI Deep Field South (ADF-S) using the Korea Microlensing Telescope Network (KMTNet), to find optical counterparts of dusty star-forming galaxies. The ADF-S is a deep far-infrared imaging survey region with AKARI covering around 12 deg2, where the deep optical imaging data are not yet available. By utilizing the wide-field capability of the KMTNet telescopes (∼4 deg2), we obtain optical images in B, R and I bands for three regions. The target depth of images in B, R and I bands is 24 mag (AB) at 5, which enables us to detect most dusty star-forming galaxies discovered by AKARI in the ADF-S. Those optical datasets will be helpful to constrain optical spectral energy distributions as well as to identify rare types of dusty star-forming galaxies such as dustobscured galaxy, sub-millimeter galaxy at high redshift.

Using current-voltage (I-V) and capacitance-voltage (C-V) measurements, the electrical properties of Au and Cu Schottky contacts to n-Ge were comparatively investigated. Lower values of barrier height, ideality factor and series resistance were obtained for the Au contact as compared to the Cu contact. The values of capacitance showed strong dependence on the bias voltage and the frequency. The presence of an inversion layer at the interface might reduce the intercept voltage at the voltage axis, lowering the barrier height for C-V measurements, especially at lower frequencies. In addition, a higher interface state density was observed for the Au contact. The generation of sputter deposition-induced defects might occur more severely for the Au contact; these defects affected both the I-V and C-V characteristics.