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The NASA exoplanet archive: data and tools for exoplanet research
ABSTRACT.We describe the contents and functionality of the NASA Exoplanet Archive, a database and toolset funded by NASA to support astronomers in the exoplanet community. The current content of theExpand
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Chemical Abundances of Luminous Cool Stars in the Galactic Center from High-Resolution Infrared Spectroscopy
We present chemical abundances in a sample of luminous cool stars located within 30 pc of the Galactic center. Abundances of carbon, nitrogen, oxygen, calcium, and iron were derived fromExpand
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Really Cool Stars and the Star Formation History at the Galactic Center
We present ?/?? = 550-1200 near-infrared H and K spectra for a magnitude-limited sample of 79 asymptotic giant branch and cool supergiant stars in the central ?5 pc (diameter) of the Galaxy. We use aExpand
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The Frequency of Barred Spiral Galaxies in the Near-Infrared*
We have determined the fraction of barred galaxies in the H-band for a statistically well-defined sample of 186 spirals drawn from the Ohio State University Bright Spiral Galaxy Survey. We find 56%Expand
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Near- and Mid-Infrared Photometry of the Pleiades and a New List of Substellar Candidate Members
We make use of new near- and mid-IR photometry of the Pleiades cluster in order to help identify proposed cluster members. We also use the new photometry with previously published photometry toExpand
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A catalog of X-ray point sources from two megaseconds of Chandra observations of the Galactic center
We present a catalog of 9017 X-ray sources identified in Chandra observations of a 2 ◦ × 0. 8 field around the Galactic center. This enlarges the number of known X-ray sources in the region by aExpand
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We present a variability analysis of the early-release first quarter of data publicly released by the Kepler project. Using the stellar parameters from the Kepler Input Catalog, we have separated theExpand
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Carbon Stars in the Hamburg/ESO Survey: Abundances*
We have carried out a detailed abundance analysis using high-dispersion spectra from HIRES at Keck for a sample of 16 carbon stars found among candidate extremely metal-poor (EMP) stars from theExpand
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Near-Infrared and Optical Morphology of Spiral Galaxies
We announce the initial release of data from the Ohio State University (OSU) Bright Spiral Galaxy Survey, a BVRJHK imaging survey of a well-defined sample of 205 bright, nearby spiral galaxies. WeExpand
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An Accurate, Easy-To-Use Abundance Scale for Globular Clusters Based on 2.2 Micron Spectra of Giant Stars
We present a new method for the determination of [Fe/H] for globular clusters. This method is based on moderate-resolution (~1500) near-IR spectroscopy in the K band of six to 10 of the brightestExpand
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