994 research outputs found

    Narratives as a Fundamental Component of Consciousness

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    In this paper, we propose a conceptual architecture that models human (spatially-temporally-modally) cohesive narrative development using a computer representation of quale properties. Qualia are proposed to be the fundamental "cognitive" components humans use to generate cohesive narratives. The engineering approach is based on cognitively inspired technologies and incorporates the novel concept of quale representation for computation of primitive cognitive components of narrative. The ultimate objective of this research is to develop an architecture that emulates the human ability to generate cohesive narratives with incomplete or perturbated information

    Explorations, Vol. 3, No. 1

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    Cover: Debouche, a thermo-formed acrylic sculpture, by Deborah de Moulpied, Associate Professor of Art at the University of Maine, (from the collection of Barbara Heldt and Gerald Smith, Oxford, England); photograph by Dale and Nedra Van Volkinburg. Articles include: Biotechnology, by Michael R. Gross The Search for Tom Swift or Some Reflections on One of America\u27s Best-Known Cultural Heroes, by David K. Vaughan ENDO-EXO 1 Sculpture in Motion Communication is Not Just Saying Words; It is Creating True Understanding, by Marisue Pickering Maine Outreach: Teaching Success, by Richard A. Hale and James F. Philp Through Cloud and Fog, Hunting the Elusive pH, by Richard Jagels Ocean Basin with a Past A Cryptic History: Breaking the Code Discerning a Future, by Detmar Schnitker We Stand Corrected in Volume II, Number 2, of EXPLORATIONS Dialogue: Letters [to the Editor] Updates from the Dispatch Cas

    The Milky Way in Context: Building an integral-field spectrograph data cube of the Galaxy

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    The Milky Way (MW) is by far the best-studied galaxy and has been regarded as an ideal laboratory for understanding galaxy evolution. However, direct comparisons of Galactic and extra-galactic observations are marred by many challenges, including selection effects and differences in observations and methodology. In this study, we present a novel code GalCraft to address these challenges by generating mock integral-field spectrograph data cubes of the MW using simple stellar population models and a mock stellar catalog of the Galaxy derived from E-Galaxia. The data products are in the same format as external galaxies, allowing for direct comparisons. We investigate the ability of pPXF to recover kinematics and stellar population properties for an edge-on mock observation of the MW. We confirm that pPXF can distinguish kinematic and stellar population differences between thin and thick disks. However, pPXF struggles to recover star formation history, where the SFR is overestimated in the ranges between 2-4 and 12-14 Gyr compared to the expected values. This is likely due to the template age spacing, pPXF regularization algorithm, and spectral similarities in old population templates. Furthermore, we find systematic offsets in the recovered kinematics, potentially due to insufficient spectral resolution and the variation of line-of-sight velocity with [M/H] and age through a line-of-sight. With future higher resolution and multi-[α\alpha/Fe] SSP templates, GalCraft will be useful to identify key signatures such as [α\alpha/Fe]-[M/H] distribution at different RR and z|z| and potentially measure radial migration and kinematic heating efficiency to study detailed chemodynamical evolution of MW-like galaxies.Comment: 27 pages, 27 figures (8 figs in appendix), submitted to MNRAS. Comments are welcom

    Bounds on the k-domination number of a graph

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    Abstract The k-domination number of a graph is the cardinality of a smallest set of vertices such that every vertex not in the set is adjacent to at least k vertices of the set. We prove two bounds on the k-domination number of a graph, inspired by two conjectures of the computer program Graffiti.pc. In particular, we show that for any graph with minimum degree at least 2k − 1, the k-domination number is at most the matching number

    Maternal super-obesity and perinatal outcomes in Australia: A national population-based cohort study

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    Background: Super-obesity is associated with significantly elevated rates of obstetric complications, adverse perinatal outcomes and interventions. The purpose of this study was to determine the prevalence, risk factors, management and perinatal outcomes of super-obese women giving birth in Australia. Methods: A national population-based cohort study. Super-obese pregnant women (body mass index (BMI) >50 kg/m2 or weight >140 kg) who gave birth between January 1 and October 31, 2010 and a comparison cohort were identified using the Australasian Maternity Outcomes Surveillance System (AMOSS). Outcomes included maternal and perinatal morbidity and mortality. Prevalence estimates calculated with 95 % confidence intervals (CIs). Adjusted odds ratios (ORs) were calculated using multivariable logistic regression. Results: 370 super-obese women with a median BMI of 52.8 kg/m2 (range 40.9–79.9 kg/m2) and prevalence of 2.1 per 1 000 women giving birth (95 % CI: 1.96–2.40). Super-obese women were significantly more likely to be public patients (96.2 %), smoke (23.8 %) and be socio-economically disadvantaged (36.2 %). Compared with other women, super-obese women had a significantly higher risk for obstetric (adjusted odds ratio (AOR) 2.42, 95 % CI: 1.77–3.29) and medical (AOR: 2.89, 95 % CI: 2.64–4.11) complications during pregnancy, birth by caesarean section (51.6 %) and admission to special care (HDU/ICU) (6.2 %). The 372 babies born to 365 super-obese women with outcomes known had significantly higher rates of birthweight ≥4500 g (AOR 19.94, 95 % CI: 6.81–58.36), hospital transfer (AOR 3.81, 95 % CI: 1.93–7.55) and admission to Neonatal Intensive Care Unit (NICU) (AOR 1.83, 95 % CI: 1.27–2.65) compared to babies of the comparison group, but not prematurity (10.5 % versus 9.2 %) or perinatal mortality (11.0 (95 % CI: 4.3–28.0) versus 6.6 (95 % CI: 2.6- 16.8) per 1 000 singleton births). Conclusions: Super-obesity in pregnancy in Australia is associated with increased rates of pregnancy and birth complications, and with social disadvantage. There is an urgent need to further address risk factors leading to super-obesity among pregnant women and for maternity services to better address pre-pregnancy and pregnancy care to reduce associated inequalities in perinatal outcomes. Keywords: Super-obesity, Obesity, Perinatal outcomes, Pregnancy, Maternal socio-economic disadvantage, Obstetric complication
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