M9V

Kirkpatrick(in GrayCorbally09) call LHS 2924 the primary M9V standard.

Boeshaar85 standard:         LHS 2924 - M9V 
HenryKirkpatrick90 standard: LHS 2924 - M9V 
Kirkpatrick91 standards:     LHS 2924 - M9V (primary standard)
		             LHS 2065 - M9V (secondary standard)
Kirkpatrick97 standard:      LHS 2065 - M9V
Hawley02 standard:           2MASS J0251+2521 - M9V
Henry02 standard:	     LHS 2065 - M9V
			     [Henry02 has LP 944-020 as ">M9V" standard] 
Henry04 standard:            LP 944-020 - M9.0V (primary standard)
Kirkpatrick(GrayCorbally09): LHS 2924 - M9V (primary standard)
Kirkpatrick10 standard:      LHS 2924 - M9V (opt.,near-IR stan.)
Kirkpatrick16 standard:	     LHS 2065 - M9V 

Skiff08 does not flag any stars as M9V MK standards. 

RECONS list shows LP 944-020 as the nearest M9V. 

ReinersBasri09 finds that the mean kinematic age of nearby M7-M9.5
stars is 3.1 Gyr.

(V-Rc)(M9V)    = 2.00  ; sec. stan. LHS 2065 (Bessell91)
(V-Rc)(M9V)    = 2.34  ; non-standard TVLM 513-46546 

(Rc-Ic)(M9V)   = 2.472 ; N=5 M9V *s in Liebert06 (+-0.023 sem, +-0.052 stdev) 
=> adopt (R-I)(M9V)  = 2.472
=> adopt (V-R)(M9V)  = 1.893 (from R-I=2.472 and V-I=4.37)
[go through Henry04 Table 2 to get independent estimate]

(V-Ic)(M9V)    = 4.36  ; sec. standard LHS 2065 
(V-Ic)(M9V)    = 4.37  ; pri. standard LHS 2924 (see below)
(V-Ic)(M9V)    = 4.398 ; non-standard BRI 0021-0214 (see below)
(V-Ic)(M9V)    = 4.66  ; from color sequence for V-Ks=9.06
(V-Ic)(M9V)    = 4.71  ; non-standard TVLM 513-46546
=> adopt (V-Ic)(M9V) = 4.66

(V-Ks)(M9V)    =  8.285 ; non-stan. ESO 207-61 (Henry04)
(V-Ks)(M9V)    = 8.836 ; pri. stan. LHS 2924
(V-Ks)(M9V)    =  8.84 ; non-stan.  SSS2356-3426 
(V-Ks)(M9V)    = 8.858 ; sec. stan. LHS 2065 
(V-Ks)(M9V)    = 8.882 ; non-stan. LP 647-13
(V-Ks)(M9V)    =  8.92 ; non-stan. 2MA1501+2250 
<V-K_CIT>(M9V) =  9.0  ; Beuermann06
(V-Ks)(M9V)    =  9.00 ; non-stan. RG0050-2722
(V-Ks)(M9V)    =  9.06 ; non-stan. BRI1222-1222
(V-Ks)(M9V)    =  9.08 ; non-stan. LHS4039C 
(V-Ks)(M9V)    = 9.09  ; smoothed fit to Dieterich SpT vs V-Ks
(V-Ks)(M9V)    =  9.12 ; non-stan. SSS2307-5009 
(V-Ks)(M9V)    = 9.15  ; sec. stan. LP944-20 (Burgasser14)
(V-Ks)(M9V)    = 9.16  ; non-stan. TVLM 513-46546
(V-Ks)(M9V)    = 9.271 ; non-stan. BRI 0021-0214
(V-Ks)(M9V)    =  9.94 ; non-stan. SIP2045-6332
=> adopt (V-Ks)(M9V) = 9.00  [updated 10/20/2019]
=> adopt (V-J)(M9V)  = 7.702 [need to double check] 
=> adopt (V-H)(M9V)  = 8.389 [need to double check] 
=> adopt (I-Ks)(M9V) = 4.482 [need to double check] 
=> adopt (J-Ks)(M9V) = 1.145 [need to double check] 

(J-H)(M9V) = 0.68 (+-0.15 rms) ; Schmidt14
(J-H)(M9V) = 0.723 (+-0.009 sem,+-0.024 stdev) ; N=9 M9V Cruz03
(J-H)(M9V) = 0.749 ; EEM: 2MASS colors of 5 M9Vs in DwarfArchives 
=> adopt (J-H)(M9V)  = 0.749

(H-Ks)(M9V)    = 0.481 ; EEM: 2MASS colors of 5 M9Vs in DwarfArchives
(H-Ks)(M9V)    = 0.478 ; trend of Dieterich14 data for V-Ks=9.00
<H-K_CIT>(M9V) = 0.47 ; Beuermann06
(H-Ks)(M9V)    = 0.464(+-0.010 sem,+-0.029 stdev) ; N=9 M9V Cruz03
(H-Ks)(M9V)    = 0.43 (+-0.16 rms) ; Schmidt14 [EEM: mean much bluer than M9V standards]
=> adopt (H-Ks)(M9V) = 0.48 [last updated 5/5/2017]

(J-Ks)(M9V)    = 1.230 ; EEM: 2MASS colors of 5 M9Vs in DwarfArchives
(J-Ks)(M9V)    = 1.20  ; Faherty09
(J-Ks)(M9V)    = 1.191 (+-0.013 sem,+-0.034 stdev) ; N=9 M9V Cruz03
(J-Ks)(M9V)    = 1.12 (+-0.17 rms) ; Schmidt14
<J-K_CIT>(M9V) = 1.12 ; Beuermann06

(i-z)(M9V)   = 1.66 (+-0.14 rms) ; Schmidt14
(i-J)(M9V)   = 3.79 (+-0.29 rms) ; Schmidt14
(i-Ks)(M9V)  = 4.91 (+-0.35 rms) ; Schmidt14
(z-J)(M9V)   = 2.14 (+-0.17 rms) ; Schmidt14

(Ks-L')(M9V) = 0.441  	         ; Dupuy12 polynomial
(Ks-W1)(M9V) = 0.25 (+-0.25 rms) ; Schmidt14
(W1-W2)(M9V) = 0.24 (+-0.27 rms) ; Schmidt14
(W2-W3)(M9V) = 0.42 (+-0.16 rms) ; Schmidt14

(Bp-Rp)(M9V) = 4.7495 ; LHS_2065  sec. stan.
(Bp-Rp)(M9V) = 4.7679 ; LHS_2924  pri. stan.
(Bp-Rp)(M9V) = 4.7890 ; LP_647-13 ter. stan.
(Bp-Rp)(M9V) = 5.0466 ; LP_944-20 sec. stan.
(Bp-Rp)(M9V) = 5.0596 ;  2MASS_J03341218-4953322  M9V
(Bp-Rp)(M9V) = 5.1039 ;  2MASS_J11592743-5247188  M9Ve
=> adopt (Bp-Rp)(M9V) = 4.78 [updated 3/1/2019]

(G-Rp)(M9V) = 1.5754 ; LHS_2065  sec. stan.
(G-Rp)(M9V) = 1.5817 ; LP_647-13 ter. stan.
(G-Rp)(M9V) = 1.5922 ; LP_944-20 sec. stan. 
(G-Rp)(M9V) = 1.5932 ; LHS_2924  pri. stan.
(G-Rp)(M9V) = 1.6012 ; 2MASS_J03341218-4953322  M9V
(G-Rp)(M9V) = 1.6090 ; 2MASS_J11592743-5247188  M9Ve
(G-Rp)(M9V) = 1.619  ; Reyle18 polynomial
=> adopt (G-Rp)(M9V) = 1.59 [updated 3/1/2019]
=> adopt (Bp-G)(M9V) = 3.19 [updated 3/1/2019; Bp-Rp=4.78, G-Rp=1.59]

(Bp-G)(M9V) = 3.1741 ; LHS_2065 
(Bp-G)(M9V) = 3.1747 ; LHS_2924 
(Bp-G)(M9V) = 3.2072 ; LP_647-13 
(Bp-G)(M9V) = 3.4544 ; LP_944-20

(G-V)(M9V) = -3.2346 ; sec. stan. LP_944-20
(G-V)(M9V) = -3.07   ; trinomial fit through late Ms
(G-V)(M9V) = -3.0313 ; sec. stan. LHS_2065
(G-V)(M9V) = -2.971  ; median M9V d<60pc (N=9) in SIMBAD (likely biased blue?)
(G-V)(M9V) = -2.9585 ; ter. stan. LP_647-13  
(G-V)(M9V) = -2.9501 ; pri. stan. LHS_2924
=> adopt (G-V)(M9V) = -3.00 [updated 12/10/2018]

M_G(M9V)    = 15.543 ; Reyle18 polynomial
M_G(M9V)    = 15.80  ; trend for late Ms & early Ls within 20pc
M_G(M9V)    = 16.09  ; Smart19 (N=17; rms=0.36)

M_J(M9V)    = 11.124 ; Reyle18 polynomial
M_H(M9V)    = 10.413 ; Reyle18 polynomial
M_Ks(M9V)   =  9.949 ; Reyle18 polynomial

(G-J)(M9V)  =  4.575 ; Reyle18 polynomial
(J-Ks)(M9V) =  1.133 ; Reyle18 polynomial

Mv(M9V) = 19.15 ; sec. stan. LHS 2065 (Burgasser14)
Mv(M9V) = 19.27 ; EEM fit for Mdwarfs for V-Ks=9.00 (rms=0.48)
Mv(M9V) =  19.29 ; Kirkpatrick94
Mv(M9V) = 19.33 ; Dieterich14 calibration for V-Ks=9.00 (rms=0.25)
Mv(M9V) = 19.36 ; non-stan LP 647-13 (Burgasser14)
Mv(M9V) = 19.37 ; pri. stan. LHS 2924
Mv(M9V) = 19.42 ; median Mv from Dieterich14 (N=9 M9V stars)
Mv(M9V) = 19.66 ; sec. stan. LP 944-20 (Burgasser14)
=> adopt Mv(M9V) = 19.40 mag [last updated 10/18/2019; M_Ks=10.40, V=9.00]

M_Ks(M9V) =  10.24 ; Dupuy12 polynomial
M_Ks(M9V) = 10.27 ; EEM fit to Dieterich14 for V-Ks=9.00
M_Ks(M9V) = 10.29 ; pri. stan. LHS 2065 (Burgasser14)
M_Ks(M9V) = 10.33 ; Deiterich14 calibration for V-Ks=9.00
M_Ks(M9V) = 10.36 ; Mv=19.36, V-Ks=9.00
M_Ks(M9V) = 10.38 ; median SIMBAD <60pc M9V N=4
M_Ks(M9V) =  10.44 ; non-stan. 1RXS J1159-5247 (Burgasser14)
M_Ks(M9V) = 10.51 ; sec. stan. LP 944-20
M_Ks(M9V) = 10.51 ; median M_Ks for Dieterich14 N=9 M9Vs
M_Ks(M9V) =  10.52 ; non-stan LP 647-13 (Bugasser14)
M_Ks(M9V) = 10.53 ; pri. stan. LHS2924
M_Ks(M9V) =  10.57 ; Dupuy12 mean 
M_Ks(M9V) =  10.80 ; non-stan LEHPM 1-3396 (Burgasser14)
=> adopt M_Ks(M9V) = 10.40 mag [updated 10/18/2019; Mv=19.40, V-Ks=9.00]

Teff(M9V)  =   2578 K ; RojasAyala12(mean N=1 M9V stars)
Teff(M9V)  =  2480 K ; Dupuy17(Lyon model scale)
Teff(M9V)  =  2470 K ; Dupuy17(SaumonMarley08 scale)
Teff(M9V)  = 2450 K ; pri. stan. LHS 2924 (recent median)
Teff(M9V)  =   2438 K ; mean photometric Teff
Teff(M9V)  = 2420 K ; sec. stan. LHS 2065 (recent median)
Teff(M9V)  = 2400 K ; Rajpurohit18 N=1 M9V stars
Teff(M9V)  = 2398 K ; median N=9 M9V Teffs from Dieterich14 ***
Teff(M9V)  =   2396 K ; Golimowski04 
Teff(M9V)  = 2281 K ; EEM N=25 Teffs
Teff(M9V)  =  2123 K ; non. stan. LP 944-20 (median Teff)
=> adopt Teff(M9V) = 2400 K (logT = 3.380) [updated 10/18/2019]

BCv(M9V) = -4.867 mag ; EEM fit to Casagrande data for Teff=2350K
BCv(M9V) = -5.641 mag ; sec. stan. LHS 2065 (Leggett01 using IAU2015 scale)
BCv(M9V) = -5.85  mag ; BC_Ks = 3.15, V-Ks=9.00
BCv(M9V) = -6.053 mag ; LP 944-20 (Leggett01 using IAU2015 scale)
=> adopt BCv(M9V) = -5.85 mag [last updated 3/8/2018; BC_Ks=3.15, V-Ks=9.00]

BC_K(M9V) = 3.21+-0.07 ; sec. stan. LHS 2065 (Golimowski04)
BC_K(M9V) = 3.183 mag  ; non-stan. BRI 0021-0214 (Leggett01, IAU2015 scale)
BC_K(M9V) = 3.158 mag  ; Leggett01 polynomial for I-K=4.482
BC_K(M9V) = 3.157 mag  ; sec. stan. LHS 2065 (Leggett01, IAU2015 scale)
BC_K(M9V) = 3.151 mag  ; trend for M0V-M9V for M9V 
BC_K(M9V) = 3.149 mag  ; Golimowki04(SpT function)
BC_Ks(M9V)= 3.12  mag  ; Schmidt14 (rms = 0.04)
BC_K(M9V) = 3.103 mag  ; Leggett01 polynomial for J-K=1.145
BC_Ks(M9V)= 3.099 mag  ; sec. stan. LP 944-20 (Leggett01 on IAU2015 scale)
=> adopt BC_K(M9V) = 3.15 mag [last updated 3/8/2018]

logL(M9V) =  -3.77 ; non-standard LP 944-20 (Leggett01)
logL(M9V) = -3.542 ; median (N=9) logL for M9Vs from Dieterich14
logL(M9V) = -3.512 ; M_Ks=10.36, BC_K=3.16 => Mbol = 13.67
logL(M9V) =  -3.49+-0.02 ; sec. stan. LHS 2065 (Golimowski04)
logL(M9V) =  -3.49 ; sec. stan. LHS 2065 (Leggett01)
=> adopt logL(M9V) = -3.51 dex [last updated 3/8/2018]
=> adopt Mbol(M9V) = 13.52 mag [last updated 3/8/2018]

Mass(M9V) = 0.079+-0.020 Msun ; GJ 2005C (Benedict16)
Mass(M9V) = 0.079 Msun ; Mann18 calib for M_Ks=10.36
=> adopt Mass(M9V) = 0.079 Msun [last updated 8/1/2018]

Radius(M9V) = 0.101 Rsun ; median (N=9) M9V radius from Dieterich14

# Primary Standard

LHS 2924 = L 271-25 = GJ 3849 = NN 3849 (J1426+3324)
 *M9V: Boeshaar85(dM9),GiampapaLiebert86,HenryKirkpatrick90,Kirkpatrick91(pri),Kirkpatrick93,Boeshaar94(dM9),Hawley97(M9c),ReidGizis05(M9.0Ve),Kirkpatrick(GrayCorbally09)(pri),Kirkpatrick10
  M7V: Bessell91
  L0: Schmidt10

  Kirkpatrick91 calls LHS 2924 the primary M9 dwarf standard, and
  cites GiampapaLiebert86 and Boeshaar85. Discussed at length in
  Probst & Liebert (1983, ApJ, 274, 245).
  plx=90.8+-1.3(Dahn02,Monet92), V=19.58(Leggett92,Monet02),
  V=19.58+-0.04(Dahn02), V=19.74(Bessell91,Gliese91,vanAltena95),
  I=15.3(Bessell91), V-I=4.44(Bessell91),
  V-I=4.37(Monet92,Leggett92,Kirkpatrick95), K_CIT=10.67(Leggett92),
  (V-Ks)_CIT=8.91(Leggett92), K-L'(MKO)=0.65(Leggett92),
  J=11.990+-0.021(2MASS), H=11.225+-0.029(2MASS0,
  K=10.744+-0.024(2MASS), (V-Ks)=8.836(Leggett92,2MASS),
  Mv=19.37+-0.03(Leggett92, Dahn02),
  M_Ks=10.534+-0.039(2MASS,Dahn02). LHS2924 is a JHK photometric
  standard for MKO system: J=11.885+-0.013(Leggett06),
  H=11.251+-0.010(Leggett06),
  K=10.721+-0.013(Leggett06). Mass=0.105+-0.042Msun(Jenkins09).
  Teffs: 1665K(Jenkins09), 1950+-150K(Probst83,Blackbody!),
  2080K(Tinney93), 2100K(Jones97), 2120K(Tsuji97),
  2200K(Casagrande08*), 2300K(ReidHawley05*), 2350K(Jones96),
  2367K(Dahn02*), 2437K(Bessell93), 2450K(Basri00*),
  2492K(Rojas-Ayala12*), 2550K(Lyubchik12*,average),
  2600K(Pavlenko02*), 2625K(Kirkpatrick93). Recent average is ~2450K.
   
# Secondary Standard

LHS 2065 = GJ 3517 = 2MASS J08533619-0329321
 *M9V: Kirpatrick91(pri),Kirkpatrick97(stan),Leggett01,Henry02,Henry04,ReidGizis05(M9.0Ve),Leggett10,Kirkpatrick11,Kirkpatrick16(stan)
  M7Ve: Bessel91

  Not listed in Hawley97,Reid04.  plx=117.3+-1.5
  mas(Monet92,vanAltena95), V=18.80(Leggett92), V =
  18.80+-0.03(Dahn02), V=18.74(Bessell91,Henry04),
  V=18.94(Dieterich14), Rc=16.74(Bessell91,Henry04),
  V-R=2.00(Bessell91), Ic=14.54(Bessell91,Henry04),
  V-I=4.36(Leggett92,Monet92,Leggett01,Kirkpatrick95),
  V-I=4.20(Bessell91), I=14.44(Leggett01), K_CIT=9.98(Leggett92),
  (V-Ks)_CIT=8.82(Leggett92), V-Ks = 8.80(Henry04),
  J=11.212+-0.026(2MASS), H=10.469+-0.026(Leggett92),
  Ks=9.942+-0.024(2MASS), (V-Ks)=8.858(Leggett92,2MASS),
  Mv=19.15+-0.04(Monet92,Dahn02), M_Ks=10.288+-0.037(Monet92,2MASS).
  BC_K = 3.18 (Leggett01). Leggett01: fbol = 1.45e-13 W/m^2 => mbol =
  13.099 mag => BC_Ks = 13.099 - 9.942 = 3.157 => BCv = 13.099 - 18.74
  = -5.641.  Patten06 lists Spitzer IRAC photometry of [3.6] =
  9.41+-0.02, [4.5]=9.39+-0.03, [5.8]=9.22+-0.01, [8.0] = 9.13+-0.01.
  Teffs: 2050K(Casagrande08), 2100K(Leggett01*), 2150K(Tinney93),
  2250K(Irwin91), 2400K(Golimowski04*), 2420K(Gautier07*),
  2441K(Dahn02*), 2453K(Bessell93), 2564K(RojasAyala12*) => recent
  median is Teff=2420K.

LP 944-20 = BRI 0337-3535
 *M9V: Tinney98,Kirkpatrick99(footnote#8),Kirkpatrick(unpub.,DwarfArchives),Leggett01,Geballe02,Henry04
  M9.5V: Reid04

  But this seems way too low for an M9V. Leggett01 lists M-m=1.51,
  I=14.16, I-J=3.48, J-H=0.70, H-K=0.45, K=9.53, K-L'=0.81 (JHKL' on
  UKIRT-IRCAM3 system, I is Cousins).  V=19.2:(Ribas03),
  V=18.70+-0.026(Dieterich14), Rc=16.39+-0.007(Dieterich14),
  Ic=14.01+-0.011(Dieterich14), Ic=14.16+-0.03(Dahn02,Leggett01),
  J=10.725+-0.021(2MASS), J=10.700(Kirkpatrick97),
  H=10.017+-0.021(2MASS), H=10.030(Kirkpatrick97),
  K=9.52+-0.03(Dahn02), K=9.52(Kirkpatrick97), K=9.58(Tinney96),
  Ks=9.548+-0.023(2MASS), J-H=0.70+-0.04(Dahn02),
  H-K=0.50+-0.04(Dahn02).  Plx=201.4+-4.2 mas (Tinney96, Dahn02),
  Plx=155.89+-1.03 mas (Dieterich14; d=6.41+-0.04 pc). Leggett01: fbol
  = 2.20e-13 W/m^2 => mbol = 12.647 (IAU2015 scale) => BC_Ks = 12.647
  - 9.548 = 3.099 => BCv = 12.647 - 18.70 = -6.053. BC_Ks =
  3.21+-0.07(Ribas03). V-Ks = 18.70 - 9.548 = 9.152.  Ribas03
  estimates logL=-3.79+-0.04, and predicts masses of 0.049-0.055 Msun
  (due to its young inferred age). Dieterich14 estimates
  logL=-3.579+-0.010 dex, radius 0.101+-0.006 Rsun. Dieterich14
  photometry and parallax consistent with Mv=19.664+-0.030,
  M_J=11.689+-0.025, M_Ks=10.512+-0.027.  Teffs: 1764K(Jenkins09),
  2100+-100K(Leggett01), 2123K(Gautier07), 2138+-68K(Dahn02),
  2312+-71K(Dieterich14), 2400K(Basri00) => median Teff = 2123K

# Tertiary Standard

LP 647-13 = 2MASS J01095117-0343264 = NLTT 3868
  M9V: Cruz02(M9e),Cruz03,Reid03,Lodieu05,Cruz07,Schmidt07,Reiners09,Faherty09

  Not considered a standard star in any publications, but all
  published types appear to be in agreement on M9V.  plx =
  97.55+-2.04mas(Weinberger16). Vmag = 19.31 (Winters15),
  Vmag=18.65(Salim03). J=11.694+-0.021, H=10.931+-0.026,
  Ks=10.428+-0.025(2MASS). V-Ks = 19.31 - 10.428 = 8.882.

# Other Stars

BRI 0021-0214 = DY Psc = 2MASS J00242463-0158201
 *M9.0V: Henry04
  M9.5: Leggett01,Geballe02,Lodieu05,Dieterich14

  V=19.42(Reid04), V=19.81+-0.031(Dieterich14),
  Rc=17.47+-0.015(Dieterich14), Rc=17.301+-0.006(Liebert06),
  Ic=15.15+-0.012(Dieterich15), Ic=15.022+-0.003(Liebert06),
  I=15.07(vanAltena95).  J=11.992+-0.035(2MASS),
  H=11.084+-0.022(2MASS), Ks=10.539+-0.023(2MASS).  Henry04 didn't
  list a Vmag, but Rc=17.42, Ic=15.16 from Dahn02.  Adopting Vmag from
  Reid04 and Ic from Liebert06, V-Ic = 4.398. Adopting Vmag from
  Dieterich14 and Ks from 2MASS: V-Ks = 9.271. Leggett06 reports MKO
  JHK photometry (it is a standard). Note that the colors are almost
  identical to the M9V standards. plx = 82.5+-3.4 mas (VanAltena95),
  80.71+-0.95mas(Weinberger16).
  Mv=19.345+-0.040(Dieterich14,Weinberger16),
  M_Ks=10.074+-0.034(2MASS,Weinberger16), Teff=2284K(Gautier07).
  Leggett01: fbol = 8.17e-14 W/m2 => mbol = 13.722 (IAU2015 scale) =>
  BC_Ks = 13.722 - 10.539 = 3.183, BCv = 13.722 - 19.81 = -6.088.

BRI 1222-1222
  M9V: Kirkpatrick95,Kirkpatrick97

  Teff=2496+-100K(Dahn02)

TVLM 868-110639
 *M9V: Kirkpatrick95,Kirkpatrick97,Henry04

  Ic=15.79(Tinney93, Tinney95,vanAltena95,Henry04), I=15.8(Martin94),
  Y=13.494+-0.002(UKIDSS, Lawrence12), J=12.614+-0.023(2MASS),
  H=11.842+-0.022(2MASS), Ks=11.347+-0.021(2MASS).
  Teff=1975K(Tinney93), 2451+-112K(Dahn02).

TVLM 513-46546
 *M9.0V: Henry04

  V=19.87(Henry04), Rc=17.53(Henry04), Ic=15.16(Henry04),
  J=11.866+-0.022(2MASS), H=11.181+-0.030(2MASS),
  Ks=10.706+-0.024(2MASS). V-Rc = 19.87 - 17.53 = 2.34.  V-Ic = 19.87
  - 15.16 = 4.71.  V-Ks = 19.87 - 10.706 = 9.16.  plx = 94.5+-0.6 mas
  (Henry04) => Mv = 19.747, M_Ks=10.583+-0.028(2MASS,Henry04).
  Teff=2404K(Gautier07)

2M 0140+27 = 2MASS J01400263+2701505 = LSPM J0140+2701 = binary ALP 5 (sep=31.8")
  M8.5: Allen07
  M9: Rice10 
  M9.5V: Reid02(in Glebocki05)

  J=12.487+-0.021(2MASS), J=12.51+-0.02(Allen07,IRTF),
  H=11.820+-0.022(2MASS), Ks=11.432+-0.021(2MASS),
  Ks=11.44+-0.02(Allen07,IRTF). Dist=17.3 pc(Allen07), 19.4+-3.5 pc
  (Lepin05). Teff=2753K(Rice10)

ESO 207-61 (J070753.3-490050)
 *M9V: Henry04
  M8.5V: Kirkpatrick11,Lodieu05(M8.5e)

  Henry04 lists V=20.39, Rc=18.63, Ic=16.23.  V=20.39
  (vanAltena95,Henry04), V=20.99(Jenkins09, source unknown = they say
  "Hipparcos", which is nonsense). J=13.228+-0.026(2MASS),
  H=12.538+-0.030(2MASS), Ks=12.105+-0.024(2MASS). plx = 54.10+-4.50
  (Dupuy12,Tinney96). Adopting V=20.39 and 2MASS K: V-K=8.285.
  Mv = 19.06 (Jenkins09,Tinney96), M_Ks=10.771+-0.182(Tinney96,2MASS). 

2MASS J14112131-2119503 = DENIS J141121.2-211950
 *M9V: Cruz03,Kendall04,Cruz07,Schmidt07,Reiners09,Gagne14(optical),Burgasser15
  M8: Gagne14(near-IR)
  M8.5\beta: Gagne15

  No published V magnitude. Teffs: 2600+-200K(Gagne15)

# Comments

The only M9V stars in the dwarf archive
(http://spider.ipac.caltech.edu/staff/davy/ARCHIVE/index.shtml) as of
July 2013 are:

2MASS J03393521-3525440 = LP 944-20 
2MASS J08533619-0329321 = LHS 2065 (sec. standard, see above; Kirkpatrick91)
2MASS J12245222-1238352 = BRI 1222-1222 (Kirkpatrick95)
2MASS J14284323+3310391 = LHS 2924 (pri. standard, see above; Henry90)
2MASS J15101685-0241078 = TVLM 868-110639 (Kirkpatrick95)

# V-K vs. Mv
V-Ks  Mv    M_Ks
8.285 19.06 10.771+-0.182 ; non-standard ESO 207-61 (Henry04)
8.836 19.37 10.534+-0.039 ; pri. stan. LHS 2924
8.84                      ; non-stan.  SSS2356-3426 
8.858 19.15 10.288+-0.037 ; sec. stan. LHS 2065 (Dieterich14 has 9.00)
8.92                      ; non-stan. 2MA1501+2250 
9.00                      ; non-stan. RG0050-2722
9.06                      ; non-stan. BRI1222-1222 
9.08                      ; non-stan. LHS4039C 
9.12                      ; non-stan. SSS2307-5009 
9.16  19.75 10.583+-0.028 ; non-stan. TVLM 513-46546
9.152 19.66 10.512+-0.027 ; sec. stan. LP944-20 (Burgasser14)
9.271 19.35 10.074+-0.034 ; non-stan. BRI 0021-0214 
9.94                      ; non-stan. SIP2045-6332 

adopt V-Ks=9.00