L6V Kirkpatrick99 standard: 2MASSs J0850359+105716 - L6V Hawley02 standard: 2MASS 0103+1935 - L6V Kirkpatrick05 standard: 2MASSs J0850359+105716 - L6V ("optical anchor") Reid08 standard: 2MASS J08503593+1057156 - L6 (pri. stan.) Kirkpatrick09(GrayCorbally): 2MASS J08503593+1057156 - L6 (primary optical standard) Kirkpatrick10 standard: 2MASS J10101480−0406499 - L6V (primary near-IR standard) Teff(L6V) = 1311 K ; 2MASS J02572581−3105523 (Kirkpatrick20) Teff(L6V) = 1483 K ; Filippazzo15 calibration (M6V-T9V) Teff(L6V) = 1513 K ; Kirkpatrick20 (Table 13 polynomial) Teff(L6V) = 1528 K ; Dupuy17(SaumonMarley08 model scale) Teff(L6V) = 1551 K ; Rad vs. logL for BT-Settl 3Gyr [M/H]=0 isochrone for LogL=-4.384 Teff(L6V) = 1616 K ; Dupuy17(Lyon model scale) Teff(L6V) = 1750 K ; Cifuentes20 for CARMENES L6V(N=1) => adopt Teff(L6V) = 1550 K (logT = 3.190) [updated 4/17/2020] (R-I)(L6V) = 2.117 ; star #32 (J0850+1057) in Liebert06 (R-I)(L6V) = 2.579 ; star #177 (J2151-2441) in Liebert06 => adopt (R-I)(L6V) = 2.348 (L6V) = 1.75 ; Faherty09 (J-Ks)(L6V) = 1.54 (+-0.23 rms; N=8) ; Schmidt14 (J-H)(L6V) = 0.96 (+-0.13 rms; N=8) ; Schmidt14 (J-H)(L6V) = 1.060 (+-0.13 rms) ; SIMBAD trend for d<30pc L dwarfs => adopt (J-H)(L5V) = 1.06 [updated 8/6/2020] (z-J)(L6V) = 2.76 (+-0.07 rms; N=6) ; Schmidt14 (H-Ks)(L6V) = 0.59 (+-0.15 rms; N=8) ; Schmidt14 (H-Ks)(L6V) = 0.654 (+-0.09 rms); trend SIMBAD d<30pc L dwarfs => adopt (H-Ks)(L6V) = 0.654 [updated 8/6/2020] (Ks-W1)(L6V)= 0.75 (+-0.14 rms; N=7) ; Schmidt14 (Ks-W1)(L6V)= 0.76 ; Dupuy12 median N=4, d<50pc (Ks-W1)(L6V)= 0.794 ; Dupuy12 trend => adopt (Ks-W1)(L6V) = 0.76 [updated 12/28/2019] (W1-W2)(L6V)= 0.34 (+-0.05 rms; N=7) ; Schmidt14 BC_K(L6V) = 3.315 mag ; Golimowksi04 BC_Ks(L6V) = 3.315 mag ; Looper08 BC_Ks(L6V) = 3.298 mag ; Filipazzo15 (field) BC_Ks(L6V) = 3.26 mag ; Schmidt14 (rms = 0.07 mag) => adopt BC_Ks(L6V) = 3.30 mag [updated 11/1/2019] M_G(L6V) = 18.938 ; Reyle18 polynomial M_G(L6V) = 18.92 ; Kiman19 (rms=0.17; N=2) M_J(L6V) = 13.588 ; Reyle18 polynomial M_J(L6V) = 13.891 ; EEM fit to L/T dwarfs d<25pc => adopt M_J(L6V) = 13.89 [updated 12/30/2020] M_H(L6V) = 12.709 ; Reyle18 polynomial (G-Rp)(L6V) = 1.822 ; Reyle18 polynomial (G-Rp)(L6V) = 1.77 ; Kiman19 (N=1) (G-J)(L6V) = 5.331 ; Reyle18 polynomial (J-Ks)(L6V) = 1.578 ; Reyle18 polynomial M_Ks(L6V) = 11.7488 ; 2MASS J09153413+0422045 M_Ks(L5V) = 11.9 ; L5V adopted M_Ks(L6V) = 12.133 ; Reyle18 polynomial M_Ks(L6V) = 12.19 ; fit to SIMBAD L0-T7.5 dwarfs d<25pc (12/2020) M_Ks(L6V) = 12.22 ; trend to L/T dwarfs in notes (1/2021) M_Ks(L7V) = 12.5 ; L7V adopted M_Ks(L6V) = 12.5025 ; 2MASS J10101480-0406499 M_Ks(L6V) = 12.5049 ; 2MASSI J0103320+193536 M_Ks(L8V) = 12.9 ; L8V adopted M_Ks(L6V) = 12.9612 ; 2MASSW J1036530-344138 M_Ks(L6V) = 13.2131 ; 2MASS J13314894-0116500 => adopt M_Ks(L6V) = 12.2 [adopted 12/30/2020] logL(L6V) = -4.384 ; M_Ks=12.4, BC_Ks=3.30, Mbol=15.700 => adopt logL(L6V) = -4.384 [updated 4/17/2020] => adopt Mbol(L6V) = 15.700 [updated 4/17/2020] Rad(L6V) = 0.08912 Rsun ; logL=-4.384, Teff=1550K => adopt Rad(L6V) = 0.0891 Rsun [updated 4/17/2020] # Primary Standard 2MASS J08503593+1057156 *L6: Kirkpatrick05(opt.anchor),Kirkpatrick09(pri.opt.stan.) # Examples 2MASSI J0103320+193536 Optical: L6: Kirkpatrick00,Cruz03,Allen06,Faherty09,Burgasser10(Kirkpatrick00),Kirkpatrick10,Bardalez14,Schneider14,Schmidt15 L6.0{beta}: Faherty12,Gagne14,Faherty16,Best18 Near-IR: L5.4: Bardalez14 L6.0: Burgasser10(Cruz04) L6: Gagne14 L6{beta}: Faherty16 L6{beta} or L6:INT-G: Best18 L6.2: Gagne15 L6pec: Gagne15 L7: Kirkpatrick10,Martin17,Schneider14 Unclear if optical or near-IR: L6{beta}: Gagne15,Fillipazzo15 Gagne15 calls it an Argus member. 2MASS J02572581−3105523 *L6: Kirkpatrick20(near-IR) L8: Kirkpatrick20(opt.) Teffs: 1311+-88K(Kirkpatrick20), plx=102.3651+-0.6073mas.