Inverted-Gaussian best fit parameters to 15272A DIB feature in APOGEE red clump spectra
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In McKinnon+2023, we fit inverted-Gaussians to the 15272A DIB feature in APOGEE red clump stellar spectra. This dataset was generated using the individual-visit spectra from APOGEE DR16, and the spectra were shifted to the heliocentric frame before finding the 15272A DIB feature. We present the best fit paramters of DIB velocity (assuming the rest-frame wavelength is 15272.42A as per Zasowski+2015), Gaussian width, and height here as well as the names of the targets and observations where the feature was observed.
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Zenodo创建时间：
2024-02-01
