NEW H-BAND STELLAR SPECTRAL LIBRARIES FOR THE SDSS-III/APOGEE SURVEY

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 ( ) spectra in the H-band (∼1.5-1.7 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 analysis 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 ASSϵT spectral synthesis code. We present a second set of libraries based on MARCS model atmospheres and the spectral synthesis code Turbospectrum. The ATLAS9/ASSϵT ( = 3500-8000 K) and MARCS/Turbospectrum ( = 3500-5500 K) grids cover a wide range of metallicity (−2.5 [M/H] +0.5 dex), surface gravity (0 ≤ 5 dex), microturbulence (0.5 8 km s−1), 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/ASSϵT and MARCS/Turbospectrum libraries and apply both of them to the analysis of the observed H-band 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 H-band using other high-resolution spectrographs.