L3.5V Kirkpatrick09(GrayCorbally): 2MASS J00361617+1821104 - L3.5 (primary optical standard) V-R(L3.5V) = 3.11 ; 2M0036 (see below) V-I(L3.5V) = 5.51 ; 2M0036 (see below) V-J(L3.5V) = 8.96 ; 2M0036 (see below) V-H(L3.5V) = 9.84 ; 2M0036 (see below) V-Ks(L3.5V) = 10.28 ; 2MASS_J00361617+1821104 (Dahn17) V-Ks(L3.5V) = 10.37 ; 2M0036 (see below) => adopt (V-Ks)(L3.5V) = 10.4 [updated 8/17/2020] (J-H)(L3.5V) = 0.989 ; (+-0.13 rms); SIMBAD d<30pc trend for Ldwarfs => adopt (J-H)(L3.5V) = 0.99 [updated 8/6/2020] (H-Ks)(L3.5V) = 0.620 (+-0.09 rms); trend SIMBAD d<30pc L dwarfs => adopt (H-Ks)(L3.5V) = 0.62 [last updated 8/6/2020] M_J(L3.5V) = 12.927 ; EEM fit to L/T dwarfs d<25pc M_Ks(L3.5V) = 11.40 ; fit to SIMBAD L0-T7.5 dwarfs d<25pc (12/2020) M_Ks(L3.5V) = 11.43 ; trend to L/T dwarfs in notes (1/2021) Teff(L3.5V) = 1757 K ; Filippazzo15 calibration (M6V-T9V) Teff(L3.5V) = 1775 K ; Cifuentes20 for CARMENES L3.5V(N=2) Teff(L3.5V) = 1780 K ; Kirkpatrick20 (Table 13 polynomial) => adopt Teff(L3.5V) = 1870K (logT = 3.272) [updated 12/26/2020] # Primary Standard 2MASS J00361617+1821104 = 2M 0036+1821 = WDS J00363+1821 L1.5: Schneider14(near-IR) *L3.5: Reid00,Kirkpatrick00(L3.5V),Gizis00,Kirkpatrick09(pri.opt.stan.),Dieterich14(source?) L4:: Geballe02 One of the earliest L dwarfs within 10pc, indeed a query of SIMBAD for objects with plx>100mas (d<10pc) and L spectral types shows no objects with default types between the L0 companion to LP 388-55 and 2MASS J00361617+1821104. This appears to be the most studied early L dwarf within 10pc, discovered by Reid00(2000AJ....119..369R). V=21.34+-0.06(Dahn02,Dahn17), V=21.43+-0.024(Dieterich14), R=18.32+-0.016(Dieterich14), I=15.92+-0.022(Dieterich14), I=16.11+-0.01(Dahn17), J=12.466+-0.027(2MASS), H=11.588+-0.030(2MASS), Ks=11.058+-0.021(2MASS), K=11.06+-0.02(Dahn02). V-R=3.11+-0.03, V-I=5.51+-0.03, V-J=8.96+-0.04, V-H=9.84+-0.04, V-Ks=10.37+-0.03, plx = 114.20+-0.80(Dieterich14). Vtan=37.6 km/s(Deiterich14). Teffs: 1796+-33K(Dieterich14), 1800K(Cifuentes20), 1900+-100K(Gagne15), 1900K(Golimowksi04), 1923K(Vrba04), 1993K(Dahn02), 2000K(Blake10). logL=-3.95+-0.011(Deiterich14), Rad=0.109+-0.0042Rsun(Dieterich14).