112 research outputs found

    A crosscultural analysis of elderly people’s morality in interactive media

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    This study examines elderly people’s innate moral foundations in influencing decisions, and their subsequent enjoyment in an interactive media environment. The Moral Foundation Questionnaire was used to distinguish between the moral intuitions of elderly US and German respondents, who were believed to have divergent yet stable moral codes that would be salient in a novel virtual world. In an experimental design, participants (N=116) were confronted with a computer simulation in which they could decide to violate or uphold each of five moral intuitions. Germans and Americans differed in their moral foundations, yet for both groups higher moral salience led to a decrease in decisions to commit moral violations in a virtual world. Results for enjoyment were mixed

    Times of Minima of Some Eclipsing Binaries

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    We present new times of minima in the light curves of some eclipsing binarie

    Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

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    In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra, and, in combination with earlier surveys, results in 330 542 redshifts across five sky regions covering similar to 250 deg(2). The redshift density, is the highest available over such a sustained area, has exceptionally high completeness (95 per cent to r(KiDS) = 19.65 mag), and is well-suited for the study of galaxy mergers, galaxy groups, and the low redshift (z < 0.25) galaxy population. DR4 includes 32 value-added tables or Data Management Units (DMUs) that provide a number of measured and derived data products including GALEX, ESO KiDS, ESO VIKING, WISE, and HerschelSpace Observatory imaging. Within this release, we provide visual morphologies for 15 330 galaxies to z < 0.08, photometric redshift estimates for all 18 million objects to r(KiDS) similar to 25 mag, and stellar velocity dispersions for 111 830 galaxies. We conclude by deriving the total galaxy stellar mass function (GSMF) and its sub-division by morphological class (elliptical, compact-bulge and disc, diffuse-bulge and disc, and disc only). This extends our previous measurement of the total GSMF down to 10(6.75) M-circle dot h(70)(-2) and we find a total stellar mass density of rho(*) = (2.97 +/- 0.04) x 10(8) M-circle dot h(70) Mpc(-3) or Omega(*)=(2.17 +/- 0.03) x 10(-3) h(70)(-1). We conclude that at z < 0.1, the Universe has converted 4.9 +/- 0.1 per cent of the baryonic mass implied by big bang Nucleosynthesis into stars that are gravitationally bound within the galaxy population

    Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions

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    In Galaxy And Mass Assembly Data Release 4 (GAMA DR4), we make available our full spectroscopic redshift sample. This includes 248 682 galaxy spectra, and, in combination with earlier surveys, results in 330 542 redshifts across five sky regions covering ∼250 deg2. The redshift density, is the highest available over such a sustained area, has exceptionally high completeness (95 per cent to rKiDS = 19.65 mag), and is well-suited for the study of galaxy mergers, galaxy groups, and the low redshift (z < 0.25) galaxy population. DR4 includes 32 value-added tables or Data Management Units (DMUs) that provide a number of measured and derived data products including GALEX, ESO KiDS, ESO VIKING, WISE, and HerschelSpace Observatory imaging. Within this release, we provide visual morphologies for 15 330 galaxies to z < 0.08, photometric redshift estimates for all 18 million objects to rKiDS ∼ 25 mag, and stellar velocity dispersions for 111 830 galaxies. We conclude by deriving the total galaxy stellar mass function (GSMF) and its sub-division by morphological class (elliptical, compact-bulge and disc, diffuse-bulge and disc, and disc only). This extends our previous measurement of the total GSMF down to 106.75 M⊙h−270 and we find a total stellar mass density of ρ* = (2.97 ± 0.04) × 108 M⊙h70 Mpc−3 or Ω∗=(2.17±0.03)×10−3h−170⁠. We conclude that at z < 0.1, the Universe has converted 4.9 ± 0.1 per cent of the baryonic mass implied by big bang Nucleosynthesis into stars that are gravitationally bound within the galaxy population

    A birth cohort study in the southeast part of Turkey evaluating wheezing phenotypes

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    World Allergy and Asthma Congress of the European-Academy-of-Allergy-and-Clinical-Immunology and World-Allergy-Organization -- JUN 22-26, 2013 -- Milan, ITALYWOS: 000325142905111…European Acad Allergy & Clin Immunol, World Allergy Or

    Adverse Drug Reactions In Children; Clinical And Laboratory Characteristics

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    American-Academy-of-Allergy-Asthma-and-Immunology Annual Meeting -- MAR 18-22, 2011 -- San Francisco, CAWOS: 000295846400738…Amer Acad Allergy Asthma & Immuno

    A case of diffuse alveolar hemorrhage after orthognathic surgery: Case report with the literature review'

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    Diffuse alveolar hemorrhage (DAH) disease is a rare but acutely developing condition that may occur after general anesthesia, if not diagnosed and treated on time, could be life-threatening. Orthognathic surgeries, frequently performed for functional and esthetic correction, are generally composed of a young population in their twenties with no other disease. The aim of presenting this case report was to describe the etiology, diagnosis, and treatment of DAH to emphasize the importance of timely diagnosis
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