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

Neurosurgical management of vertebral lesions in pediatric chronic recurrent multifocal osteomyelitis: patient series

Background: Chronic recurrent multifocal osteomyelitis (CRMO) is a rare pediatric autoinflammatory disorder involving 2 or more inflammatory bone lesions separated in time and space associated with pathological vertebral fractures. There are no current guidelines for the role of pediatric spine surgeons in the management of this condition. The authors demonstrate the importance of close and early involvement of neurosurgeons in caring for patients with CRMO with vertebral involvement. Observations: Fifty-six pediatric patients with clinical and radiographic evidence of CRMO were identified and clinical, radiographic, laboratory, and histopathological data were reviewed. All were evaluated via Jansson and Bristol CRMO diagnostic criteria. Ten had radiographic evidence of vertebral involvement (17.9%). Nine of these had multifocal disease. Five patients had multiple vertebrae affected. Six patients were evaluated for possible surgical intervention and one required intervention due to vertebra plana leading to a progressive kyphotic deformity and significant spinal canal stenosis. Lessons: In conjunction with management by the primary pediatric rheumatology team using nonsteroidal anti-inflammatory drugs, disease-modifying anti-rheumatic drugs, immunotherapies, and bisphosphonates, given the risk of pathological fractures and potential resulting long-term neurological deficits, the authors recommend close monitoring and management by pediatric spine surgeons for any patient with CRMO with vertebral lesions

Neurosurgical management of vertebral lesions in pediatric chronic recurrent multifocal osteomyelitis: patient series.

BACKGROUND: Chronic recurrent multifocal osteomyelitis (CRMO) is a rare pediatric autoinflammatory disorder involving 2 or more inflammatory bone lesions separated in time and space associated with pathological vertebral fractures. There are no current guidelines for the role of pediatric spine surgeons in the management of this condition. The authors demonstrate the importance of close and early involvement of neurosurgeons in caring for patients with CRMO with vertebral involvement. OBSERVATIONS: Fifty-six pediatric patients with clinical and radiographic evidence of CRMO were identified and clinical, radiographic, laboratory, and histopathological data were reviewed. All were evaluated via Jansson and Bristol CRMO diagnostic criteria. Ten had radiographic evidence of vertebral involvement (17.9%). Nine of these had multifocal disease. Five patients had multiple vertebrae affected. Six patients were evaluated for possible surgical intervention and one required intervention due to vertebra plana leading to a progressive kyphotic deformity and significant spinal canal stenosis. LESSONS: In conjunction with management by the primary pediatric rheumatology team using nonsteroidal anti-inflammatory drugs, disease-modifying anti-rheumatic drugs, immunotherapies, and bisphosphonates, given the risk of pathological fractures and potential resulting long-term neurological deficits, the authors recommend close monitoring and management by pediatric spine surgeons for any patient with CRMO with vertebral lesions

The sixth data release of the Sloan Digital Sky Survey

This paper describes the Sixth Data Release of the Sloan Digital Sky Survey. With this data release, the imaging of the northern Galactic cap is now complete. The survey contains images and parameters of roughly 287 million objects over 9583 deg(2), including scans over a large range of Galactic latitudes and longitudes. The survey also includes 1.27 million spectra of stars, galaxies, quasars, and blank sky ( for sky subtraction) selected over 7425 deg2. This release includes much more stellar spectroscopy than was available in previous data releases and also includes detailed estimates of stellar temperatures, gravities, and metallicities. The results of improved photometric calibration are now available, with uncertainties of roughly 1% in g, r, i, and z, and 2% in u, substantially better than the uncertainties in previous data releases. The spectra in this data release have improved wavelength and flux calibration, especially in the extreme blue and extreme red, leading to the qualitatively better determination of stellar types and radial velocities. The spectrophotometric fluxes are now tied to point-spread function magnitudes of stars rather than fiber magnitudes. This gives more robust results in the presence of seeing variations, but also implies a change in the spectrophotometric scale, which is now brighter by roughly 0.35 mag. Systematic errors in the velocity dispersions of galaxies have been fixed, and the results of two independent codes for determining spectral classifications and red-shifts are made available. Additional spectral outputs are made available, including calibrated spectra from individual 15 minute exposures and the sky spectrum subtracted from each exposure. We also quantify a recently recognized underestimation of the brightnesses of galaxies of large angular extent due to poor sky subtraction; the bias can exceed 0.2 mag for galaxies brighter than r = 14 mag