New H-band Stellar Spectral Libraries for the SDSS-III/APOGEE survey
arXiv:1502.05237 · doi:10.1088/0004-6256/149/6/181
Abstract
The Sloan Digital Sky Survey--III (SDSS--III) Apache Point Observatory Galactic Evolution Experiment (APOGEE) has obtained high resolution (R 22,500), high signal-to-noise ratio ( 100) spectra in the Hband (1.51.7 m) for about 146,000 stars in the Milky Way galaxy. We have computed spectral libraries with effective temperature () ranging from 3500 to 8000 K for the automated chemical analy\-sis of the survey data. The libraries, used to derive stellar parameters and abundances from the APOGEE spectra in the SDSS--III data release 12 (DR12), are based on ATLAS9 model atmospheres and the ASST spectral synthesis code. We present a second set of libraries based on MARCS model atmospheres and the spectral synthesis code Turbospectrum. The ATLAS9/ASST ( = 35008000 K) and MARCS/Turbospectrum ( = 35005500 K) grids cover a wide range of metallicity (2.5 [M/H] 0.5 dex), surface gravity (0 log 5 dex), microturbulence (0.5 8 km~s), carbon (1 [C/M] 1 dex), nitrogen (1 [N/M] 1 dex), and -element (1 [/M] 1 dex) variations, having thus seven dimensions. We compare the ATLAS9/ASST and MARCS/Turbospectrum libraries and apply both of them to the analysis of the observed Hband spectra of the Sun and the K2 giant Arcturus, as well as to a selected sample of well-known giant stars observed at very high-resolution. The new APOGEE libraries are publicly available and can be employed for chemical studies in the Hband using other high-resolution spectrographs.
45 pages, 11 figures; accepted for publication in the Astronomical Journal
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