Spectrophotometric distances to 44,784 RGB stars predicted with a data-driven model combining spectroscopy from APOGEE DR14 and photometric information from 2MASS, Gaia, and WISE. The columns show 2MASS ID, parallax measurements from Gaia DR2 and their uncertainty, predicted spectrophotometric parallaxes and uncertainties, whether the star is part of our training set or not, and whether it is in sample A or B. For details please refer to Hogg, Eilers & Rix (2018). If the data is being used, please cite Hogg, Eilers & Rix (2018), as well as Gaia, 2MASS, WISE, APOGEE, and SDSS-IV.

{"references": ["http://adsabs.harvard.edu/abs/2017AJ....154...94M", "http://adsabs.harvard.edu/abs/2016A%26A...595A...1G", "http://adsabs.harvard.edu/abs/2006AJ....131.1163S", "http://adsabs.harvard.edu/abs/2010AJ....140.1868W", "https://ui.adsabs.harvard.edu//#abs/2018arXiv181009468H"]}