Early-type galaxies in the SDSS. I. The sample

A sample of nearly 9000 early-type galaxies, in the redshift range 0.01 < z < 0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. This paper describes how the sample was selected, presents examples of images and seeing corrected fits to the observed surface brightness profiles, describes our method for estimating K-corrections, and shows that the SDSS spectra are of sufficiently high quality to measure velocity dispersions accurately. It also provides catalogs of the measured photometric and spectroscopic parameters. In related papers, these data are used to study how early-type galaxy observables, including luminosity, effective radius, surface brightness, color, and velocity dispersion, are correlated with one another.Comment: 63 pages, 21 figures. Accepted by AJ (scheduled for April 2003). This paper is part I of a revised version of astro-ph/0110344. The full version of Tables 2 and 3, i.e. the tables listing the photometric and spectroscopic parameters of ~ 9000 galaxies, are available at http://astrophysics.phys.cmu.edu/~bernardi/SDSS/Etypes/TABLE

Early-type galaxies in the SDSS. III. The Fundamental Plane

A magnitude limited sample of nearly 9000 early-type galaxies, in the redshift range 0.01 < z < 0.3, was selected from the Sloan Digital Sky Survey using morphological and spectral criteria. The Fundamental Plane relation in this sample is R_o ~ sigma^{1.49\pm 0.05} I_o^{-0.75\pm 0.01} in the r* band. It is approximately the same in the g*, i* and z* bands. Relative to the population at the median redshift in the sample, galaxies at lower and higher redshifts have evolved only little. If the Fundamental Plane is used to quantify this evolution then the apparent magnitude limit can masquerade as evolution; once this selection effect has been accounted for, the evolution is consistent with that of a passively evolving population which formed the bulk of its stars about 9 Gyrs ago. One of the principal advangtages of the SDSS sample over previous samples is that the galaxies in it lie in environments ranging from isolation in the field to the dense cores of clusters. The Fundamental Plane shows that galaxies in dense regions are slightly different from galaxies in less dense regions.Comment: 27 pages, 10 figures. Accepted by AJ (scheduled for April 2003). This paper is part III of a revised version of astro-ph/011034

Early-type galaxies in the SDSS. IV. Colors and chemical evolution

The colors and chemical abundances of early-type galaxies at redshifts z<0.3 are studied using a sample of nearly 9000 galaxies, selected from the Sloan Digital Sky Survey using morphological and spectral criteria. In this sample, redder galaxies have larger velocity dispersions. Color also correlates with magnitude and size, but these correlations are entirely due to the L-sigma and R_o-sigma relations: the primary correlation is color-sigma. The red light in early-type galaxies is, on average, slightly more centrally concentrated than the blue. Because of these color gradients, the strength of the color--magnitude relation depends on whether or not the colors are defined using a fixed metric aperture. Chemical evolution and star formation histories of early-type galaxies are investigated using co-added spectra of similar objects. At fixed sigma, the population at z ~ 0.2 had weaker Mg_2 and stronger H_beta absorption compared to the population at z ~ 0. It was also bluer. Comparison of these colors and line-strengths, and their evolution, with single-burst stellar population models suggests a formation time of 9 Gyrs ago, consistent with a Fundamental Plane analysis of this sample.Comment: 38 pages, 16 figures. Accepted by AJ (scheduled for April 2003). This paper is part IV of a revised version of astro-ph/0110344. The full version of Table 3 and the 182 composite spectra can be downloaded from http://astrophysics.phys.cmu.edu/~bernardi/SDSS/Etypes/SPECFITS A README file (bernardi4.README) explains the content of the director

The Seventh Data Release of the Sloan Digital Sky Survey

This paper describes the Seventh Data Release of the Sloan Digital Sky Survey (SDSS), marking the completion of the original goals of the SDSS and the end of the phase known as SDSS-II. It includes 11663 deg^2 of imaging data, with most of the roughly 2000 deg^2 increment over the previous data release lying in regions of low Galactic latitude. The catalog contains five-band photometry for 357 million distinct objects. The survey also includes repeat photometry over 250 deg^2 along the Celestial Equator in the Southern Galactic Cap. A coaddition of these data goes roughly two magnitudes fainter than the main survey. The spectroscopy is now complete over a contiguous area of 7500 deg^2 in the Northern Galactic Cap, closing the gap that was present in previous data releases. There are over 1.6 million spectra in total, including 930,000 galaxies, 120,000 quasars, and 460,000 stars. The data release includes improved stellar photometry at low Galactic latitude. The astrometry has all been recalibrated with the second version of the USNO CCD Astrograph Catalog (UCAC-2), reducing the rms statistical errors at the bright end to 45 milli-arcseconds per coordinate. A systematic error in bright galaxy photometr is less severe than previously reported for the majority of galaxies. Finally, we describe a series of improvements to the spectroscopic reductions, including better flat-fielding and improved wavelength calibration at the blue end, better processing of objects with extremely strong narrow emission lines, and an improved determination of stellar metallicities. (Abridged)Comment: 20 pages, 10 embedded figures. Accepted to ApJS after minor correction

The synthetic psychology of the self

Synthetic psychology describes the approach of “understanding through building” applied to the human condition. In this chapter, we consider the specific challenge of synthesizing a robot “sense of self”. Our starting hypothesis is that the human self is brought into being by the activity of a set of transient self-processes instantiated by the brain and body. We propose that we can synthesize a robot self by developing equivalent sub-systems within an integrated biomimetic cognitive architecture for a humanoid robot. We begin the chapter by motivating this work in the context of the criteria for recognizing other minds, and the challenge of benchmarking artificial intelligence against human, and conclude by describing efforts to create a sense of self for the iCub humanoid robot that has ecological, temporally-extended, interpersonal and narrative components set within a multi-layered model of mind

The National Early Warning Score and its subcomponents recorded within ±24 hours of emergency medical admission are poor predictors of hospital-acquired acute kidney injury

YesBackground: Hospital-acquired Acute Kidney Injury (H-AKI) is a common cause of avoidable morbidity and mortality. Aim: To determine if the patients’ vital signs data as defined by a National Early Warning Score (NEWS), can predict H-AKI following emergency admission to hospital. Methods: Analyses of emergency admissions to York hospital over 24-months with NEWS data. We report the area under the curve (AUC) for logistic regression models that used the index NEWS (model A0), plus age and sex (A1), plus subcomponents of NEWS (A2) and two-way interactions (A3). Likewise for maximum NEWS (models B0,B1,B2,B3). Results: 4.05% (1361/33608) of emergency admissions had H-AKI. Models using the index NEWS had the lower AUCs (0.59 to 0.68) than models using the maximum NEWS AUCs (0.75 to 0.77). The maximum NEWS model (B3) was more sensitivity than the index NEWS model (A0) (67.60% vs 19.84%) but identified twice as many cases as being at risk of H-AKI (9581 vs 4099) at a NEWS of 5. Conclusions: The index NEWS is a poor predictor of H-AKI. The maximum NEWS is a better predictor but seems unfeasible because it is only knowable in retrospect and is associated with a substantial increase in workload albeit with improved sensitivity.The Health Foundatio

A BIBLIOGRAPHY OF THE ABORIGINAL ARCHEOLOGY OF NEBRASKA

I have tried to make this Bibliography as complete as possible, including material from surrounding states pertinent to the archeological problems of Nebraska and references which pertain more to the history of Nebraska archeology than to its content. In compiling this list, I have used previous bibliographies by Robert W. Neuman (1962b, 1968) and Jerome E. Petsche (1968) which deal in part with Nebraska archeology

Evaluating Residence Patterns among Prehistoric Populations: Clues from Dental Enamel Composition

We determined enamel composition (Ca, P, Mg, Cu, Mn, Se, Zn, Al, Sr, Pb) for the mandibular canines of 94 individuals from 4 prehistoric Arikara cemetery populations, collecting the compositional data using scanning electron microscopy energy dispersive x-ray analysis. We examined each of the four samples independently and then pooled them for a group comparison using correspondence analysis. The results indicate significant intrapopulational dispersal, particularly when viewed by age and sex subgroups. When all sites are included for correspondence analysis, a distinctive pattern of adult male dispersal compared to the more tightly clustered adult female and subadult subsample is apparent. We hypothesize that the observed pattern of dispersal indicates local geographic and possible dietary differences among the groups. Furthermore, we hypothesize that the observed differences between males, and females and subadults for each site are the result of a residence pattern of out-migration for males

Sexual dimorphism in Cunninghamella

1.The terms heterothallic and homothallic are distinguished as applied to gametophytic sexual differentiation in the mucors. 2. Types of the evidence in support of sex intergrades in heterothallic mucors are given and criticized. 3. Burger's paper on Cunninghamella, in which he concludes that sexual dimorphism does not exist in this genus, is discussed (1) from the standpoint of his own data, (2) from the standpoint of our experience, and the decision is reached that his conclusion is not warranted. 4. Data on Cunninghamella elegans, Cunninghamella A (an undetermined species), C. echinulata, and C. bertholletiae give a total of 2250 contrasts between a total of 202 races. 5. In C. bertholletiae certain contrast combinations lead to imperfect sexual reactions when zygospores might be expected. 6. In none of the species were races found which reacted as sex intergrades 7. It is concluded that so far as the material investigated is concerned Cunninghamella is sexually dimorphic