The Resolved Outer Population of NGC6822 with WFPC2

We present F336W (U), F439W (B), F555W (V), and F675W (R) Wide Field Planetary Camera 2 (WFPC2) photometry of two outer regions of the Local Group dwarf irregular galaxy NGC6822. The NE region is ~13 arcmin from the galaxy centre, while the W region lies 10 arcmin out, and within the wispy low surface brightness outer regions of the galaxy. The fields are not crowded and contain few NGC 6822 stars. We discuss errors and uncertainties and find that the W region contains a main sequence that extends to stars of about 2 solar masses, with an age of about 200 Myr. The NE region has no main sequence or stars younger than 1 Gyr, but does contain some luminous red stars that are not matched in the W field. These stars are not clumped in the field. The results suggest that the W region may be a trace of a tidal event that triggered the current star-formation in this isolated galaxy.Comment: 12 pages including 2 tables, plus 4 figures (#1 omitted) To appear in PAS

Heavy and Complex X-ray Absorption Towards the Nucleus of Markarian 6

We have used the ASCA satellite to make the first X-ray spectra of Markarian 6, a bright Seyfert 1.5 galaxy with complex and variable permitted lines, an ionization cone, and remarkable radio structures. Our 0.6--9.5 keV spectra penetrate to the black hole core of this Seyfert and reveal heavy and complex intrinsic X-ray absorption. Both total covering and single partial covering models fail to acceptably fit the observed absorption, and double partial covering or partial covering plus warm absorption appears to be required. The double partial covering model provides the best statistical fit to the data, and we measure large column densities of ~ (3-20) * 10^{22} cm^{-2} irrespective of the particular spectral model under consideration. These X-ray columns are over an order of magnitude larger than expected based on observations at longer wavelengths. Our data suggest that most of the X-ray absorption occurs either in gas that has a relatively small amount of dust or in gas that is located within the Broad Line Region. The X-ray absorber may well be the putative `atmosphere' above the torus that collimates the ionization cone. We also detect an apparently broad 6.4 keV iron K-alpha line, and we present optical spectra demonstrating that the optical emission lines were in a representative state during our ASCA observation.Comment: 30 pages, 7 figures, Astrophysical Journal. Paper is also available at: http://www.astro.psu.edu/users/johnf/Text/research.htm

Young and Intermediate-age Distance Indicators

Distance measurements beyond geometrical and semi-geometrical methods, rely mainly on standard candles. As the name suggests, these objects have known luminosities by virtue of their intrinsic proprieties and play a major role in our understanding of modern cosmology. The main caveats associated with standard candles are their absolute calibration, contamination of the sample from other sources and systematic uncertainties. The absolute calibration mainly depends on their chemical composition and age. To understand the impact of these effects on the distance scale, it is essential to develop methods based on different sample of standard candles. Here we review the fundamental properties of young and intermediate-age distance indicators such as Cepheids, Mira variables and Red Clump stars and the recent developments in their application as distance indicators.Comment: Review article, 63 pages (28 figures), Accepted for publication in Space Science Reviews (Chapter 3 of a special collection resulting from the May 2016 ISSI-BJ workshop on Astronomical Distance Determination in the Space Age

Is there an association between hospital accreditation and patient satisfaction with hospital care? A survey of 37 000 patients treated by 73 hospitals

Objective: In many countries hospitals are undergoing accreditation as mandatory or voluntary measures. It is believed that accreditation positively influence quality of care and patient satisfaction. This survey aims at assessing the relationship between patient satisfaction and accreditation status. Design: Between January and May 2007, 4 weeks after their discharge, 78 508 patients from 328 departments in 73 hospitals received a validated questionnaire. Data from 36 777 patients (response rate 55%) were available for analyses. Main: Outcome Measures Recommendation rate was used as primary endpoint, which was available from 35 945 patients. To address the clustering of patients within hospitals, we applied univariate and multivariable generalized estimating equations. As covariates we used ‘gender’ and ‘age’ at the patient level and the ‘number of beds’ and ‘hospital teaching status’ at the hospital level. Results: Overall and not addressing the clustering, 66.3% of all the patients recommend their hospital to others. This recommendation, however, was not related to the accreditation status in the univariate analyses (odds ratio (OR) for accreditation (‘yes’) and recommendation (‘yes’) 0.99, 95% confidence interval (CI) 0.85–1.16, P= 0.92). This result was similar in the multivariable regression model adjusted for clustering (OR = 0.98, 95% CI 0.84–1.13, P= 0.74). Conclusions: Our results support the notion that accreditation is not linked to measurable better quality of care as perceived by the patient. Hospital accreditation may represent a step towards total quality management, but may not be a key factor to quality of care measured by the patient's willingness to recommend.C. Sack, A. Scherag, P. Lütkes, W. Günther, K.-H. Jöckel and G. Holtman

Rare data on a rocky shore fish reproductive biology: sex ratio, length of first maturation and spawning period of Abudefduf saxatilis (Linnaeus, 1758) with notes on Stegastes variabilis spawning period (Perciformes: Pomacentridae) in São Paulo, Brazil

This study presents data on the reproduction of Abudefduf saxatilis, a rocky shore inhabitant at the northern coast of São Paulo State. A total of 73 individuals were collected using hooks and baits. They were measured, weighed and dissected, sex and maturation stage were analysed, first macroscopically, then part of the material was taken for microscopical confirmation. Visual censuses were also done for underwater observation of egg's presence. Results showed equivalence of males and females in the population, first maturation occurring between 101 and 115mm of total length, spawning period occurs from November to February for Abudefduf saxatilis and October to January for Stegastes variabilis. Reproductive period for A. saxatilis was positively related to air temperature and thermic amplitude, but the environmental clue most likely to influence this rhythm is photoperiod. Transects with visual census of males guarding eggs were also a reliable tool for finding reproductive period in these demersal, egg-guarder species.<br>Esse estudo apresenta dados sobre a reprodução de Abudefduf saxatilis, uma espécie habitante de costões rochosos no litoral norte do estado de São Paulo. Os peixes foram coletados com anzol e isca num total de 73 indivíduos, foram medidos, pesados, dissecados, seu sexo e maturidade gonadal foram analisados, primeiro macroscopicamente, depois parte desse material foi levado para confirmação microscópica. Censos visuais também foram feitos para observar a presença de ovos. Os resultados apontam para uma equivalência entre o número de machos e fêmeas na população, a primeira maturação ocorre entre 101 e 115 mm de comprimento total, a desova ocorre entre os meses de novembro a fevereiro em Abudefduf saxatilis e outubro a janeiro em Stegastes variabilis. O período reprodutivo de A. saxatilis está positivamente relacionado à temperatura do ar e amplitude térmica, mas o indicador ambiental mais provável de influenciar o ritmo reprodutivo é o fotoperíodo. Os censos visuais feitos com a transecção mostraram-se uma ferramenta confiável para encontrar o período de desova nessas espécies demersais que guardam seus ovos

Correlated multiwavelength emission from the X-ray-bright Seyfert galaxy III Zw 2

‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1046/j.1365-8711.2002.05603.x [Full text of this article is not available in the UHRA]Peer reviewe