Mapping the Extinction Curve in 3D: Structure on Kiloparsec Scales. R(V) and Distance Catalog.

R(V) and distance measurements used in Schlafly et al. (2017). The R(V) measurements come from Schlafly et al. (2016), while the distance measurements come from Ness et al. (2016). The catalog contains the following fields: l: f8, Galactic longitude of star b: f8, Galactic latitude of star mag: 10f4, PS1 grizy, 2MASS JHK, WISE W1 & W2 magnitudes of star err: 10f4, uncertainties in magnitude magint: 10f4, Estimated intrinsic magnitudes of star from APOGEE stellar parameters and Schlafly et al. (2016), corresponding to mag. An overall constant or gray term is undetermined. ep: f4, E(B-V) to star from Schlafly et al. (2016) rpv: f4, R'(V) from Schlafly et al. (2016) x: f4, Extinction curve parameter x to star from Schlafly et al. (2016) rpvx: f4, R'(V) estimated from x flags: i4, See below. distance_ness2016: f4, Distance estimate from Ness et al. (2016) for star Description of flags: 0: ep < 0.3, rpv and rpvx will be particularly uncertainty 1: photometry with uncertainty of less than 0.2 available in fewer than seven bands; use with caution 2: photometry with uncertainty of less than 0.2 available in fewer than 9 bands. 3: uncertainty in g, r, or W2 photometry greater than 0.2, rpv will be unreliable. 4: significant uncertainty in rpvx, use with caution.