L5V Hawley02 standard: 2MASS 1507-1627 - L5V Kirkpatrick05 standard: DENIS-P J1228.2-1547 - L5V ("optical anchor") Kirkpatrick09(GrayCorbally): 2MASS J12281523-1547342 (=DENIS-P J1228.2-1547) - L5 (primary optical standard) (Rc-Ic)(L5V) = 2.41 ; 2M1507 (see below) (Rc-Ic)(L5V) = 2.395 ; N=4 L5Vs in Liebert06 (+-0.022 sem, +-0.045 rms) => adopt (R-I)(L5V) = 2.395 (V-Rc)(L5V) = 3.22 ; 2M1507 (see below) (V-Rc)(L5V) = 3.530 ; GJ 1001BC (see below) (V-Ic)(L5V) = 5.62 ; 2M1507 (see below) (V-I_Bes)(L5V) = 6.010 ; GJ 1001BC (V-J)(L5V) = 9.31 ; 2M1507 (see below) (V-J)(L5V) = 9.661 ; GJ 1001BC (V-H)(L5V) = 10.24 ; 2M1507 (see below) (V-H)(L5V) = 10.715 ; GJ 1001BC (V-Ks)(L5V) = 10.82 ; 2M1507 (see below) (V-Ks)(L5V) = 11.374 ; GJ 1001BC (L5V) = 1.74 ; Faherty09 (J-Ks)(L5V) = 1.53 (+-0.23 rms; N=7) ; Schmidt14 (i-z)(L5V) = 2.13 (+-0.06 rms; N=5) ; Schmidt14 (i-J)(L5V) = 4.88 (+-0.09 rms; N=5) ; Schmidt14 (i-Ks)(L5V) = 6.40 (+-0.25 rms; N=5) ; Schmidt14 (z-J)(L5V) = 2.82 (+-0.11 rms; N=6) ; Schmidt14 (J-H)(L5V) = 0.95 (+-0.17 rms; N=7) ; Schmidt14 (H-Ks)(L5V) = 0.60 (+-0.08 rms; N=8) ; Schmidt14 (Ks-W1)(L5V)= 0.61 (+-0.14 rms; N=7) ; Schmidt14 (Ks-W1)(L5V)= 0.685 ; Dupuy12 median N=5 d<50pc (Ks-W1)(L5V)= 0.72 ; Dupuy12 trend => adopt (Ks-W1)(L5V) = 0.68 [updated 12/28/2019] (W1-W2)(L5V)= 0.30 (+-0.12 rms; N=8) ; Schmidt14 M_G(L5V) = 18.053 ; 2MASS J11263991-5003550 M_G(L5V) = 18.2478 ; 2MASSW J1004392-333518 M_G(L5V) = 18.2595 ; 2MASS J14540797-6604476 M_G(L5V) = 18.2971 ; 2MASS J12035812+0015500 M_G(L5V) = 18.4665 ; 2MASS J17502484-0016151 M_G(L5V) = 18.48 ; median SIMBAD d<25pc nearest 10 L5s M_G(L5V) = 18.4913 ; 2MASS J14162408+1348263 M_G(L5V) = 18.6244 ; 2MASSW J1507476-162738 M_G(L5V) = 18.6532 ; 2MASS J05395200-0059019 M_G(L5V) = 18.8283 ; 2MASS J18212815+1414010 M_G(L5V) = 18.938 ; Reyle18 polynomial M_G(L5V) = 19.0577 ; 2MASS J21373742+0808463 => adopt M_G(L5V) = 18.5 [adopted 4/17/2020] M_J(L5V) = 13.588 ; Reyle18 polynomial M_H(L5V) = 12.709 ; Reyle18 polynomial (G-Rp)(L5V) = 1.822 ; Reyle18 polynomial (G-J)(L5V) = 5.331 ; Reyle18 polynomial (J-Ks)(L5V) = 1.578 ; Reyle18 polynomial M_Ks(L5V) = 11.5568 ; 2MASSW J1004392-333518 M_Ks(L5V) = 11.5685 ; 2MASS J14540797-6604476 M_Ks(L5V) = 11.6141 ; 2MASS J12035812+0015500 M_Ks(L5V) = 11.778 ; 2MASS J11263991-5003550 M_Ks(L5V) = 11.7943 ; 2MASS J18212815+1414010 M_Ks(L5V) = 11.88 ; median among nearest 10 L5s in SIMBAD M_Ks(L5V) = 11.9674 ; 2MASSW J1507476-162738 M_Ks(L5V) = 12.0022 ; 2MASS J05395200-0059019 M_Ks(L5V) = 12.0215 ; 2MASS J17502484-0016151 M_Ks(L5V) = 12.1187 ; 2MASS J21373742+0808463 M_Ks(L5V) = 12.133 ; Reyle18 polynomial M_Ks(L5V) = 12.2723 ; 2MASS J14162408+1348263 => adopt M_Ks(L5V) = 11.9 [updated 4/9/2020] Teff(L5V) = 1627 K ; Dupuy17(SaumonMarley08 scale) Teff(L5V) = 1700 K ; 2M 1507 (see below) Teff(L5V) = 1710 K ; Rad vs. logL for BT-Settl 3Gyr [M/H]=0 isochrone for LogL=-4.196 Teff(L5V) = 1712 K ; Dupuy17(Lyon model scale) Teff(L5V) = 1725 K ; GJ1001BC (Deiterich14) => adopt Teff(L5V) = 1710 K (logT = 3.233) [updated 4/17/2020] BC_Ks(L5V) = 3.315 mag ; Filipazzo15 (field) BC_Ks(L5V) = 3.331 mag ; Looper08 BC_K(L5V) = 3.342 mag ; Golimowksi04 BC_Ks(L5V) = 3.37 mag ; Schmidt14 (rms = 0.04) => adopt BC_Ks(L5V) = 3.33 mag [updated 11/1/2019] logL(L5V) = -4.196 ; M_Ks=11.90, BC_Ks=3.33, Mbol=15.23 => adopt logL(L5V) = -4.196 [updated 4/17/2020] => adopt Mbol(L5V) = 15.230 [updated 4/17/2020] Rad(L5V) = 0.09092 Rsun ; logL=-4.196, Teff=1710K => adopt Rad(L5V) = 0.0909 Rsun [updated 4/17/2020] # Examples 2MASS J15074769-1627386 = 2M_1507-1627 L5: Reid00,Cruz03,Reid06(opt),Reid08,Schmidt07,Faherty09(opt) L5.5: Knapp04(IR),Kirkpatrick05,Faherty09(IR) plx=144.08+-2.05(Costa06), plx=136.4+-0.4(Dahn02), V=22.136+-0.1:(Costa06), V=22.9+-0.5(Dahn02), Rc=18.928+-0.097(Costa06), Rc=18.919+-0.013(Liebert06), Ic=16.579+-0.079(Costa06), Ic=16.512+-0.006(Liebert06), J=12.830+-0.027(2M), H=11.895+-0.024(2M), Ks=11.312+-0.026(2M), K=11.40+-0.02(Dahn02). Rc-Ic=2.407(Liebert06), V-Rc=3.22+-0.11(Costa06,Liebert06), V-Ic=5.62+-0.11(Costa06,Liebert06), V-J=9.31+-0.11(Costa06,2M) V-H=10.24+-0.11(Costa06,2M) V-K=10.82+-0.11(Costa06,2M). Teffs: 1629K(Vrba04), 1703K(Dahn02), 1750K(Golimowski04) => adopt Teff = 1700 K. Liebert06 lists the star twice, it appears that the photometry was analyzed in two different sets, I list the values from the set with smaller uncertainties. logL = -4.23 (Antonova13). GJ 1001BC = LHS 102BC = WDS 00046-4044 BC L4.5+L4.5: Reid08(#2) L4.5: Knapp04(cited by Leggett10) *L5+L5: Reid08(#1) L5: Kirkpatrick05, Patten06 (J2000) 00:04:34.86-40:44:06.3 (Stauffer10). GJ 1001A is M3.5 star (Gliese91). Tokovinin08 lists the triple as a 0.26+0.06+0.06 Msun system. WDS lists separation 0.1". Reid08 splits BC into "Ba" (B) having SpT=L4.5, J=13.82, J-H=0.95, J-Ks=0.65 and "Bb" (C) having SpT=L4.5, J=13.90, J-H=0.95, J-Ks=0.65. In another table in the same reference, Reid08 lists the pair as "L5 & L5". Reid06 lists masses of 0.070 & 0.069 Msun if 1 Gyr, and 0.078 and 0.078 Msun if 3 Gyr. Given that Vtan ~ 100 km/s, I'll wager the system is older than 3 Gyr. Knapp04 lists Z-J=1.61 for unresolved BC. plx = 76.86+-3.97 mas (Henry06), 77.02+-2.07 mas (Dieterich14). Dupuy12 lists photometry for B of: J=13.813+-0.034, H=12.735+-0.032, Ks=12.100+-0.035; and C of: J=13.913+-0.036, H=12.885+-0.034, Ks=12.200+-0.037. Unresolved 2MASS photometry of BC: J=13.109+-0.024, H=12.055+-0.026, Ks=11.396+-0.026 (AAA flag). Dieterich14 lists unresolved photometry of BC of: V=22.77+-0.025, R=19.24+-0.045, I=16.76+-0.012. Unresolved colors of BC: V-Ks= 22.77-11.396 = 11.374 +- 0.036, V-J = 9.661 +- 0.035, V-H = 10.715 +- 0.036, V-R = 3.530+-0.052, V-I = 6.01 +- 0.028. Patten06 lists unresolved Spitzer IRAC photometry of [3.6] = 10.36+-0.01, [4.5] = 10.47+-0.01, [5.8] = 10.14+-0.03, [8.0] = 10.13+-0.02. Leggett10 lists unresolved MKO Ymag = 14.32+-0.10 from Hewett06. logL = -4.049+-0.048 (Dieterich14), Rad = 0.105+-0.005 (Deiterich14). Teff = 1725+-21K (Deiterich14).