The Rest-frame Optical Colors of 99,000 SDSS Galaxies

We synthesize the rest-frame Stroemgren colors using SDSS spectra for 99,088 galaxies selected from Data Release 1. This narrow-band ~200 AA photometric system (uz, vz, bz, yz), first designed for the determination of effective temperature, metallicity and gravity of stars, measures the continuum spectral slope of galaxies in the rest-frame 3200-5800 AA wavelength range. Galaxies form a remarkably narrow locus (~0.03 mag) in the resulting color-color diagram. The Bruzual & Charlot population synthesis models suggest that the position of a galaxy along this locus is controlled by a degenerate combination of metallicity and age of the dominant stellar population. Galaxy distribution along the locus is bimodal, with the local minimum corresponding to an ~1 Gyr old single stellar population. The position perpendicular to the locus is independent of metallicity and age, and reflects the galaxy's dust content, as implied by both the models and the statistics of IRAS detections. A comparison of this locus with the galaxy locus in the H_delta-D_n(4000) diagram, utilized by Kauffmann et al. (2003) to estimate stellar masses, reveals a tight correlation, although the two analyzed spectral ranges barely overlap. Overall, the galaxy spectral energy distribution in the entire UV to near-IR range can be described as a single-parameter family with an accuracy of 0.1 mag, or better. This nearly one-dimensional distribution of galaxies in the multi-dimensional space of measured parameters strongly supports the conclusion of Yip et al. (2004), based on a principal component analysis, that SDSS galaxy spectra can be described by a small number of eigenspectra. Apparently, the contributions of stellar populations that dominate the optical emission from galaxies are combined in a simple and well-defined way.Comment: Accepted for publication in MNRAS; 19 pages, 28 color figure

Abc method – guarantor of real costs in the mining extractive industry entities

The article aims to emphasize the importance of the ABC method in the provision of real production costs within mining extractive industry entities in Romania. Starting from the progress of investigations undertaken in the specialty literature regarding the adaptation and implementation of the ABC method to the specifics of the entities in the mining and quarrying industry to the achievements made so far by various specialists, the authors of this article demonstrate the successful implementation of the ABC method in mining entities in Romania and the determination of the real costs. The documentation which was the basis of the study and comparison between applicative traditional method used and the ABC method applied is likely to prove the viability of the organization of the managerial accounting of mining extractive industry entities in Romania in order to increase their performances. The article ends with the conclusions of the authors concerning the enlargement of the successful implementation of the ABC method in mining extractive industry entities in Romania

Abc method – guarantor of real costs in the mining extractive industry entities

The article aims to emphasize the importance of the ABC method in the provision of real production costs within mining extractive industry entities in Romania. Starting from the progress of investigations undertaken in the specialty literature regarding the adaptation and implementation of the ABC method to the specifics of the entities in the mining and quarrying industry to the achievements made so far by various specialists, the authors of this article demonstrate the successful implementation of the ABC method in mining entities in Romania and the determination of the real costs. The documentation which was the basis of the study and comparison between applicative traditional method used and the ABC method applied is likely to prove the viability of the organization of the managerial accounting of mining extractive industry entities in Romania in order to increase their performances. The article ends with the conclusions of the authors concerning the enlargement of the successful implementation of the ABC method in mining extractive industry entities in Romania

Dashboard, Tool for Monitoring and Measuring the Performances of Entities within Mining Extractive

This article aims to emphasis the importance of dashboard in monitoring and measuring the performances of entities within mining extractive industry of Romania. Having regard to the stage of the researches carried out in the specialty literature regarding the implementation of ABC method to the peculiarity of entities within mining extractive industry and up to the achievements made at present by various professionals, the authors of this article demonstrate the utility of dashboard in monitoring and measuring the performances of mining entities of Romania and of making decisions based on information provided by it. The main tool underlying the elaboration of dashboard was presented, namely the results account as accounting synthesis document of managerial accounting. The article ends with the conclusions of authors with a view to advantages and importance of using the dashboard of ABC method within the entities of mining extractive industry of Romania

Dashboard, Tool for Monitoring and Measuring the Performances of Entities within Mining Extractive

This article aims to emphasis the importance of dashboard in monitoring and measuring the performances of entities within mining extractive industry of Romania. Having regard to the stage of the researches carried out in the specialty literature regarding the implementation of ABC method to the peculiarity of entities within mining extractive industry and up to the achievements made at present by various professionals, the authors of this article demonstrate the utility of dashboard in monitoring and measuring the performances of mining entities of Romania and of making decisions based on information provided by it. The main tool underlying the elaboration of dashboard was presented, namely the results account as accounting synthesis document of managerial accounting. The article ends with the conclusions of authors with a view to advantages and importance of using the dashboard of ABC method within the entities of mining extractive industry of Romania

Hubble Space Telescope Spectroscopy of the Balmer lines in Sirius B

Sirius B is the nearest and brightest of all white dwarfs, but it is very difficult to observe at visible wavelengths due to the overwhelming scattered light contribution from Sirius A. However, from space we can take advantage of the superb spatial resolution of the Hubble Space Telescope to resolve the A and B components. Since the closest approach in 1993, the separation between the two stars has become increasingly favourable and we have recently been able to obtain a spectrum of the complete Balmer line series for Sirius B using HST?s Space Telescope Imaging Spectrograph (STIS). The quality of the STIS spectra greatly exceed that of previous ground-based spectra, and can be used to provide an important determination of the stellar temperature (Teff = 25193K) and gravity (log g = 8.556). In addition we have obtained a new, more accurate, gravitational red-shift of 80.42 +/- 4.83 km s-1 for Sirius B. Combining these results with the photometric data and the Hipparcos parallax we obtain new determinations of the stellar mass for comparison with the theoretical mass-radius relation. However, there are some disparities between the results obtained independently from log g and the gravitational redshift which may arise from flux losses in the narrow 50x0.2arcsec slit. Combining our measurements of Teff and log g with the Wood (1995) evolutionary mass-radius relation we get a best estimate for the white dwarf mass of 0.978 M. Within the overall uncertainties, this is in agreement with a mass of 1.02 M obtained by matching our new gravitational red-shift to the theoretical M/R relation.Comment: 11 pages, 6 figures, accepted for publication in the Monthly Notices of the Royal Astronomical Societ

The early-type dwarf galaxy population of the Hydra I cluster

We analyse the properties of the early-type dwarf galaxy population in the Hydra I cluster. We investigate the galaxy luminosity function (LF), the colour-magnitude relation (CMR), and the magnitude-surface brightness relation down to M_V~-10 mag. Another goal of this study is to find candidates for ultra-compact dwarf galaxies (UCDs). Two spectroscopic surveys performed with Magellan I/LDSS2 and VLT/VIMOS, as well as deep VLT/FORS1 images in V and I bands were examined. We identify cluster members by radial velocity measurements and select other cluster galaxy candidates by their morphology. One possible UCD candidate with M_V=-13.26 mag is found. Our sample of 100 morphologically selected dwarf galaxies defines a CMR that extends the CMR of the giant cluster galaxies to the magnitude limit of our survey (M_V~-10 mag). It matches the relations found for the Local Group and the Fornax cluster dwarfs almost perfectly. The Hydra I dwarfs also follow a magnitude-surface brightness relation similar to that of the LG dwarfs. Moreover, we observe a continuous relation for dwarf galaxies and giant early-type galaxies when plotting the central surface brightness \mu_0 of a S\'ersic model vs. the galaxy magnitude. The effective radius is found to be largely independent of the luminosity for M_V>-18 mag, being R_e~0.8 kpc. We derive a very flat faint-end slope of the LF (\alpha = -1.13 \pm 0.04) from fitting a Schechter function, whereas fitting a power law for M_V>-14 mag gives \alpha = -1.40 \pm 0.18. Our findings suggest that early-type dwarf and giant galaxies are the same class of objects. The similarity of the dwarf galaxy scaling relations to other environments implies that internal processes could be more important for their global photometric properties than external influences. (abridged)Comment: 17 pages, 16 figures, accepted for publication in A&A, 4 references added to the replaced versio

Relating basic properties of bright early-type dwarf galaxies to their location in Abell 901/902

We present a study of the population of bright early-type dwarf galaxies in the multiple-cluster system Abell 901/902. We use data from the STAGES survey and COMBO-17 to investigate the relation between the color and structural properties of the dwarfs and their location in the cluster. The definition of the dwarf sample is based on the central surface brightness and includes galaxies in the luminosity range -16 >= M_B >~-19 mag. Using a fit to the color magnitude relation of the dwarfs, our sample is divided into a red and blue subsample. We find a color-density relation in the projected radial distribution of the dwarf sample: at the same luminosity dwarfs with redder colors are located closer to the cluster centers than their bluer counterparts. Furthermore, the redder dwarfs are on average more compact and rounder than the bluer dwarfs. These findings are consistent with theoretical expectations assuming that bright early-type dwarfs are the remnants of transformed late-type disk galaxies involving processes such as ram pressure stripping and galaxy harassment. This indicates that a considerable fraction of dwarf elliptical galaxies in clusters are the results of transformation processes related to interactions with their host cluster.Comment: 12 pages, 8 figures, accepted for publication in A&A, typo corrected in abstrac

The Ks-band Tully-Fisher Relation - A Determination of the Hubble Parameter from 218 ScI Galaxies and 16 Galaxy Clusters

The value of the Hubble Parameter (H0) is determined using the morphologically type dependent Ks-band Tully-Fisher Relation (K-TFR). The slope and zero point are determined using 36 calibrator galaxies with ScI morphology. Calibration distances are adopted from direct Cepheid distances, and group or companion distances derived with the Surface Brightness Fluctuation Method or Type Ia Supernova. Distances are determined to 16 galaxy clusters and 218 ScI galaxies with minimum distances of 40.0 Mpc. From the 16 galaxy clusters a weighted mean Hubble Parameter of H0=84.2 +/-6 km s-1 Mpc-1 is found. From the 218 ScI galaxies a Hubble Parameter of H0=83.4 +/-8 km s-1 Mpc-1 is found. When the zero point of the K-TFR is corrected to account for recent results that find a Large Magellanic Cloud distance modulus of 18.39 +/-0.05 a Hubble Parameter of 88.0 +/-6 km s-1 Mpc-1 is found. A comparison with the results of the Hubble Key Project (Freedman et al 2001) is made and discrepancies between the K-TFR distances and the HKP I-TFR distances are discussed. Implications for Lamda-CDM cosmology are considered with H0=84 km s-1 Mpc-1. (Abridged)Comment: 37 pages including 12 tables and 7 figures. Final version accepted for publication in the Journal of Astrophysics & Astronom

To which countries do European psychiatric trainees want to move to and why?

publisher: Elsevier articletitle: To which countries do European psychiatric trainees want to move to and why? journaltitle: European Psychiatry articlelink: http://dx.doi.org/10.1016/j.eurpsy.2017.06.010 content_type: article copyright: © 2017 Elsevier Masson SAS. All rights reserved.publisher: Elsevier articletitle: To which countries do European psychiatric trainees want to move to and why? journaltitle: European Psychiatry articlelink: http://dx.doi.org/10.1016/j.eurpsy.2017.06.010 content_type: article copyright: © 2017 Elsevier Masson SAS. All rights reserved.BACKGROUND: There is a shortage of psychiatrists worldwide. Within Europe, psychiatric trainees can move between countries, which increases the problem in some countries and alleviates it in others. However, little is known about the reasons psychiatric trainees move to another country. METHODS: Survey of psychiatric trainees in 33 European countries, exploring how frequently psychiatric trainees have migrated or want to migrate, their reasons to stay and leave the country, and the countries where they come from and where they move to. A 61-item self-report questionnaire was developed, covering questions about their demographics, experiences of short-term mobility (from 3 months up to 1 year), experiences of long-term migration (of more than 1 year) and their attitudes towards migration. RESULTS: A total of 2281 psychiatric trainees in Europe participated in the survey, of which 72.0% have 'ever' considered to move to a different country in their future, 53.5% were considering it 'now', at the time of the survey, and 13.3% had already moved country. For these immigrant trainees, academic was the main reason they gave to move from their country of origin. For all trainees, the overall main reason for which they would leave was financial (34.4%), especially in those with lower (2500€) incomes, personal reasons were paramount (44.5%). CONCLUSIONS: A high number of psychiatric trainees considered moving to another country, and their motivation largely reflects the substantial salary differences. These findings suggest tackling financial conditions and academic opportunities