The Eleventh and Twelfth Data Releases of the Sloan Digital Sky Survey: Final Data from SDSS-III

The third generation of the Sloan Digital Sky Survey (SDSS-III) took data from 2008 to 2014 using the original SDSS wide-field imager, the original and an upgraded multi-object fiber-fed optical spectrograph, a new near-infrared high-resolution spectrograph, and a novel optical interferometer. All of the data from SDSS-III are now made public. In particular, this paper describes Data Release 11 (DR11) including all data acquired through 2013 July, and Data Release 12 (DR12) adding data acquired through 2014 July (including all data included in previous data releases), marking the end of SDSS-III observing. Relative to our previous public release (DR10), DR12 adds one million new spectra of galaxies and quasars from the Baryon Oscillation Spectroscopic Survey (BOSS) over an additional 3000 deg2 of sky, more than triples the number of H-band spectra of stars as part of the Apache Point Observatory (APO) Galactic Evolution Experiment (APOGEE), and includes repeated accurate radial velocity measurements of 5500 stars from the Multi-object APO Radial Velocity Exoplanet Large-area Survey (MARVELS). The APOGEE outputs now include the measured abundances of 15 different elements for each star. In total, SDSS-III added 5200 deg2 of ugriz imaging; 155,520 spectra of 138,099 stars as part of the Sloan Exploration of Galactic Understanding and Evolution 2 (SEGUE-2) survey; 2,497,484 BOSS spectra of 1,372,737 galaxies, 294,512 quasars, and 247,216 stars over 9376 deg2; 618,080 APOGEE spectra of 156,593 stars; and 197,040 MARVELS spectra of 5513 stars. Since its first light in 1998, SDSS has imaged over 1/3 of the Celestial sphere in five bands and obtained over five million astronomical spectra. \ua9 2015. The American Astronomical Society

New genetic loci link adipose and insulin biology to body fat distribution.

Body fat distribution is a heritable trait and a well-established predictor of adverse metabolic outcomes, independent of overall adiposity. To increase our understanding of the genetic basis of body fat distribution and its molecular links to cardiometabolic traits, here we conduct genome-wide association meta-analyses of traits related to waist and hip circumferences in up to 224,459 individuals. We identify 49 loci (33 new) associated with waist-to-hip ratio adjusted for body mass index (BMI), and an additional 19 loci newly associated with related waist and hip circumference measures (P < 5 × 10(-8)). In total, 20 of the 49 waist-to-hip ratio adjusted for BMI loci show significant sexual dimorphism, 19 of which display a stronger effect in women. The identified loci were enriched for genes expressed in adipose tissue and for putative regulatory elements in adipocytes. Pathway analyses implicated adipogenesis, angiogenesis, transcriptional regulation and insulin resistance as processes affecting fat distribution, providing insight into potential pathophysiological mechanisms

Correction to: Cluster identification, selection, and description in Cluster randomized crossover trials: the PREP-IT trials

An amendment to this paper has been published and can be accessed via the original article

Externalizing Behaviors among Children of HIV Seropositive Former and Current Drug Users: Parent Support Network Factors as Social Ecological Risks

Children affected by their parents’ dual drug use and HIV/AIDS face considerable challenges to their psychosocial development, including parent dysfunction and foster care placement. While HIV/AIDS may increase parents’ mobilization of social support, their drug use may restrict who is available to help them, with potential implications to the adjustment of their children with whom they remain in contact. This study sought to identify dually affected children’s living situations, and parent and parent’s support network factors as correlates of children’s externalizing problem behaviors. An urban community sample of 462 HIV seropositive, current or former drug-using parents were queried about their children aged 5–15 years old. One hundred ninety-four children were reported by 119 parents. The outcome was children’s externalizing behaviors of ever having been suspended or expelled from school, criminal-justice system involvement, or illicit drug or heavy alcohol use. Independent variables included kin and drug users in parent’s support network. Generalized estimating equations were used to adjust for the potential correlation of children of the same parent. Among parents, 63% were mothers, 57% current opioid or cocaine users, 85% were African American, 35% had AIDS or CD <200, and 53% had high depressive symptoms (CES-D ≥ 16); median age was 38. Among children, median age was 12; 23% lived with the nominating parent, 65% with other family, and 11% in non-kin foster care. While only 34% of parents reported child custody, 43% reported daily contact with their child, and 90% reported high emotional closeness. Parents reported externalizing behaviors among 32% of the children. Logistic regression indicated that externalizing behavior was positively associated with parent’s physical limitations and proportion of illicit drug users in parent’s support network. A significant interaction was found indicating that the effect of parent’s support network-level drug use was greater for children living with versus not living with the parent. The model adjusted for parent’s current drug use and depressive symptoms, which were not significant. Results indicate that while only a minority of these dually affected children lived with the parent, the parents’ physical limitations and embeddedness in drug using support networks, particularly if living with their children, was associated with the children’s maladjustment. It is plausible that these factors interfere with parenting, expose the children to conflict or adverse social influences, or obligate children to assume caregiving for their parent. While dually affected children’s contact with their parents may have important benefits, results suggest it presents ongoing needs for intervention with the children, their parents, and caregivers

Wide-field Precision Kinematics of the M87 Globular Cluster System

We present the most extensive combined photometric and spectroscopic study to date of the enormous globular cluster (GC) system around M87, the central giant elliptical galaxy in the nearby Virgo Cluster. Using observations from DEIMOS and the Low Resolution Imaging Spectrometer at Keck, and Hectospec on the Multiple Mirror Telescope, we derive new, precise radial velocities for 451 GCs around M87, with projected radii from ~5 to 185 kpc. We combine these measurements with literature data for a total sample of 737 objects, which we use for a re-examination of the kinematics of the GC system of M87. The velocities are analyzed in the context of archival wide-field photometry and a novel Hubble Space Telescope catalog of half-light radii, which includes sizes for 344 spectroscopically confirmed clusters. We use this unique catalog to identify 18 new candidate ultracompact dwarfs and to help clarify the relationship between these objects and true GCs. We find much lower values for the outer velocity dispersion and rotation of the GC system than in earlier papers and also differ from previous work in seeing no evidence for a transition in the inner halo to a potential dominated by the Virgo Cluster, nor for a truncation of the stellar halo. We find little kinematical evidence for an intergalactic GC population. Aided by the precision of the new velocity measurements, we see significant evidence for kinematical substructure over a wide range of radii, indicating that M87 is in active assembly. A simple, scale-free analysis finds less dark matter within ~85 kpc than in other recent work, reducing the tension between X-ray and optical results. In general, out to a projected radius of ~150 kpc, our data are consistent with the notion that M87 is not dynamically coupled to the Virgo Cluster; the core of Virgo may be in the earliest stages of assembly

Sloan Digital Sky Survey Data Release 12

Data Release 12 (DR12) is the final data release of the SDSS-III, containing all SDSS observations through July 2014. It includes the complete dataset of the BOSS and APOGEE surveys, and also newly includes stellar radial velocity measurements from MARVELS