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 AKARI North Ecliptic Pole Deep Field is a natural location to accomplish deep extragalactic surveys. It is supported by comprehensive ancillary data extending from radio to X-ray wavelengths, which have been used to classify radio sources as radio-loud and radio-quiet objects and to create a catalogue of Active Galactic Nuclei (AGN). This has been achieved by using a radio-optical classification and colour- colour diagrams rather than the more usual way based on spectroscopy Furthermore, we explore whether this technique can be extended by using a far-Infrared (FIR) colour-colour diagram which has been used to identify 268 high redshift candidates.

We report the results of a multi-wavelength study in the North Ecliptic Pole (NEP) deep field and examine the far infrared-radio correlation (FIRC) for high and low redshift objects. We have found a correlation between the GMRT data at 610 MHz and the Herschel data at 250μm that has been used to define a spectral index. This spectral index shows no evolution against redshift. As a result of the study, we show a radio colour-infrared diagram that can be used as a redshift indicator.

We have imaged the AKARI Deep Field with the GMRT radio telescope at 610 MHz, detecting 1224 radio components, which are optically identified with 455 optical galaxies having a mean r0 magnitude brighter of 22.5 (to a completeness limit of 25.4 mag), and an average redshift ~ 0.8.

The preliminary data reduction, analysis and first results from the Herschel survey of the AKARI NEP field are presented. Herschel SPIRE observations of the NEP-Wide region and PACS observations of the NEP-Deep region have yielded galaxy catalogues of 4000 and 900 sources respectively down to ux density levels of approximately 15 mJy at 100-250 microns. Source counts produced from these catalogues reach cosmologically significant depths tracing the evolutionary upturn and turnover in the source counts. The source counts are in agreement with other large area surveys carried out with Herschel bridging the gap between the shallow and deep Herschel surveys.

The thermoelectric Seebeck and Peltier effects of a single walled carbon nanotube (SWCNT) quantum dot nanodevice are investigated, taking into consideration a certain value of applied tensile strain and induced ac-field with frequency in the terahertz (THz) range. This device is modeled as a SWCNT quantum dot connected to metallic leads. These two metallic leads operate as a source and a drain. In this three-terminal device, the conducting substance is the gate electrode. Another metallic gate is used to govern the electrostatics and the switching of the carbon nanotube channel. The substances at the carbon nanotube quantum dot/ metal contact are controlled by the back gate. Results show that both the Seebeck and Peltier coefficients have random oscillation as a function of gate voltage in the Coulomb blockade regime for all types of SWCNT quantum dots. Also, the values of both the Seebeck and Peltier coefficients are enhanced, mainly due to the induced tensile strain. Results show that the three types of SWCNT quantum dot are good thermoelectric nanodevices for energy harvesting (Seebeck effect) and good coolers for nanoelectronic devices (Peltier effect).

Lycorine, a natural alkaloid extracted from the Amaryllidaceae plant family, was reported to various physiological and pharmacological effects including anti-cancer activity. Nevertheless, there is no report of the anticancer effect of lycorine in oral cancer cells. The effects of lycorine on cell proliferation and apoptosis were examined through trypan blue exclusion assay, 4’-6-diamidino-2-phenylindole (DAPI) stain, Live/Dead assay, Western blot analysis and RT-PCR. Lycorine suppressed cell viability and induced apoptosis in MC3 and HSC-3 cell lines. Lycorine decreased survivin protein but did not affect its mRNA. It regulated survivin through accelerating protein degradation in a time-dependent manner although neither proteasome nor lysosome was not associated with lycorine-mediated protein degradation. Collectively, our results suggest that lycorine may be a potential therapeutic anti-cancer drug candidate for the treatment of human oral cancer.

Moral licensing is a non-conscious effect that provides a moral boost in the self-concept, which increases the preference for a relative immoral action by dampening the negative self-attributions associated with such behavior. Applied to a marketing context, moral licensing explains why a purchase of a green product (a positive moral act) is likely to increase the likelihood of subsequently purchasing a luxury good (a negative moral act). This study addresses the question how big this effect typically is and which factors influence its size by conducting a Meta-Analysis and a Meta-Regression. Based on a random effects model, the point estimate for the generalized effect size Cohen’s d is 0.365 (SE=0.047; p=0.000). Results of a Meta-Regression indicate, for the first time, that the three moderators cultural background, type of decision and type of comparison explain a substantial amount of the total variation of moral licensing effect’s size.

Coastal areas across the globe and people who live in them are vulnerable to a host of natural disasters including hurricanes, typhoons, and tsunamis. During the past several decades, coastal communities of the world have also been seriously affected by man-made disasters resulting in severe social, economic, and environmental damages. The 2010 Deepwater Horizon oil spill (DWH) was the worst man-made disaster for the Gulf coast communities of the US. Community residents and resource organizations in the Florida Gulf coast responded quickly to address social, economic, and environmental needs after this disaster. The purpose of this single case study is to determine these community responses. The research uses documents from community organizations and in-depth interviews with community leaders. Constant comparative analysis method was used to determine major and sub categories of community efforts. Results show that community efforts centered on collaboration, outreach, and grassroots mobilization for resiliency after the disaster.

Sustainable community development has become a cornerstone for the overall sustainability movement in the recent years. Island provinces, due to the unique make up of their communities can and should adopt sound community development process for sustaining their futures growth. Civic engagement and citizen input are crucial for planning sustainable growth of island communities. This is primarily due to the fact that most island communities are inundated with rapidly growing tourism industry that threatens to affect the future of their environmental assets, island cultures and living standards. The purpose of this article is to highlight the importance of environmental governance and citizen participation for sustainable growth of island communities. In addition to discussing the importance of citizen participation in sustainable development of island communities, this article also provides a brief case study of Jeju island and its recent attempts to promote sustainability in the wake of rapidly growing tourist industry. Two emerging and important planning processes that can enhance sustainable community development of island provinces are also discussed with specific applications to Jeju

The Kepler mission has shown that small planets are extremely common. It is likely that nearly every star in the sky hosts at least one rocky planet. We just need to look hard enough - but this requires vast amounts of telescope time. MINERVA (MINiature Exoplanet Radial Velocity Array) is a dedicated exoplanet observatory with the primary goal of discovering rocky, Earth-like planets orbiting in the habitable zone of bright, nearby stars. The MINERVA team is a collaboration among UNSW Australia, Harvard-Smithsonian Center for Astrophysics, Penn State University, University of Montana, and the California Institute of Technology. The four-telescope MINERVA array will be sited at the F.L. Whipple Observatory on Mt Hopkins in Arizona, USA. Full science operations will begin in mid-2015 with all four telescopes and a stabilised spectrograph capable of high-precision Doppler velocity measurements. We will observe ~100 of the nearest, brightest, Sun-like stars every night for at least five years. Detailed simulations of the target list and survey strategy lead us to expect 154 new low-mass planets.

Weak gravitational lensing is an ecient technique for detecting galaxy clusters and probing their mass distribution. We present a weak gravitational lensing analysis of a large sample of galaxy clusters. We have built a nearly complete sample of 50 optically rich clusters, located in the redshift range 0:1 < z < 0:6 and observed in the Canada France Hawaii Telescope Legacy Survey (CFHT-LS). We used weak gravitational lensing to measure, for each galaxy cluster, the density radial prole, the total mass and the mass-to-light ratio (by comparing with the total luminosity of the member galaxies). This project is a preliminary step towards the next analysis of the weak lensing galaxy clusters in the surveys KiDS and VOICE, which are currently collecting data with the VLT Survey Telescope, in Chile.

We present [Fe ii] ⋋ 1.257 μm spectra toward the interacting binary UY Aur with 0:0014 angular resolution, obtained with the Near infrared Integral Field Spectrograph (NIFS) combined with the adaptive optics system Altair of the GEMINI observatory. In the [Fe ii] emission, UY Aur A (primary) is brighter than UY Aur B (secondary). The blueshifted and redshifted emission between the primary and secondary show a complicated structure. The radial velocities of the [Fe ii] emission features are similar for UY Aur A and B: ~ —100 km s-1 and ~ +130 km s-1 for the blueshifted and redshifted components, respectively. Considering the morphologies of the [Fe ii] emissions and bipolar out ow context, we concluded that UY Aur A drives fast and widely opening out ows with an opening angle of ~90° while UY Aur B has micro collimated jets.

Purpose: Non-invasive tear break up time (NITBUT) is a test commonly used by clinicians to measure the stability of the tear film. This study aims to compare the NITBUT of the Bausch and Lomb Biotrue Oneday (BT) Daily Disposable contact lenses against 3 other commercially available daily disposable lenses to see if BT can provide a more stable pre-lens tear film over the other 3 types of lenses at 12 hours of lens wear. Methods: Twelve existing contact lens wearers were recruited to wear 4 types of contact lenses each for a day of at least 12 hours. Other than BT, the other 3 test lenses were the daily disposable lenses made of etafilcon A (AV), narafilcon A (TE) and delefilcon A (DT1) materials. Each subject was assigned the lenses without knowing the brand of the lenses. Baseline NITBUT was first measured with no lens in the eye and pre-lens NITBUT was measured again at 12 hours after the lenses were worn. The NITBUT was measured using Oculus Keratograph 5M. This instrument measures the NITBUT objectively using infrared illumination which is invisible to the human eye and can prevent glare or bright light irritation during examination. Results: NITBUT was provided by the instrument as “first break” and “average break” values. In this study, the first break value was analyzed because that was the time when the break-up of tears was first detected by the instrument, and that matches with what the clinicians normally do in measuring NITBUT. The NITBUT for the nesofilcon A lens (BT) was longer than that for all the other 3 lens types in 10 out of the 12 subjects (83%). The mean TBUT for BT, AV, TE, DT1 was respectively 17.9 ± 4.3 sec, 9.5 ± 3.3 sec, 8.3 ± 5.9 sec and 8.8 ± 3.6 sec. Not only is the difference in NITBUT statistically significant (p<0.05, paired t-test – nesofilcon A (BT) Vs each of the 3 lens types), but also the NITBUT for BT is about double than that for all the other 3 types of lenses. Conclusion: The NITBUT for the nesofilcon A lens (BT) measured at 12 hours was about double than that for the other 3 lens types and the difference was statistically significant. The results suggested that the Biotrue Oneday provides a more stable pre-lens tear film than the other 3 types of daily disposable lenses at 12 hours of lens wear.

This fourth article in a six-part series correlating Kant’s philosophy with the Yijing begins by summarizing the foregoing articles: both Kant and the Yijing’s 64 hexagrams (gua) employ “architectonic” reasoning to form a fourlevel system with 0+4+12+(4x12) elements, the fourth level’s four sets of 12 correlating to Kant’s model of four university “faculties”. This article explores the second twelvefold set, the law faculty. The “idea of reason” guiding this wing of the comparative analysis is immortality. Three of Kant’s “quaternities” correspond to three sets of four gua in the Yijing: the fourfold nature of the soul in rational psychology (as substantial, simple, unified, spatially related) corresponds to gua 47, 6, 58, 10, respectively; the three “Definitive Articles” and fourth, “Secret Article”, in Perpetual Peace correspond to gua 16, 35,51, 21; and the four objective relations of law to duty in Metaphysics of Morals correspond to gua 45, 12, 17, 25.