1 Stephens & Boesgaard 2002AJ....123.1647S
 2 A(Li)=1.59 and EW(Li)=16.5+/-1.0 Boesgaard et al. 2005ApJ...633..398B
 3 Carney et al. 1994, Cat. J/AJ/107/2240
 4 Casagrande et al. 2010, Cat. J/A+A/512/54
 5 Estimated from 12Gyr [{alpha}/Fe]=+0.3 Yale-Yonsei isochrones (Demarque et 
 5  al. 2004ApJS..155..667D) with Lejeune et al. (1998, Cat. J/A+AS/130/65)
 5  color transformations using the Teff and assuming evolutionary status of 
 5  Carney et al. (1994, Cat. J/AJ/107/2240) and/or MV value of Schuster et al. 
 5  (2006, Cat. J/A+A/445/939) and/or the Hipparcos-based parallax
 6 Adopted here
 7 The Yale-Yonsei dwarflike log g values inferred from Teff and distance are 
 7  in considerably better agreement than the subgiantlike logg values inferred 
 7  from the Teff and Schuster et al. (2006, Cat. J/A+A/445/939) MV values. We 
 7  thus assume dwarf evolutionary status and adopt the Carney et al. (1994,
 7  Cat. J/AJ/107/2240)-based values
 8 Reddy & Lambert 2008MNRAS.391...95R
 9 Estimated from 12Gyr [{alpha}/Fe]=+0.3 Yale-Yonsei isochrones (Demarque et 
 9  al. 2004ApJS..155..667D) with Lejeune et al. (1998, Cat. J/A+AS/130/65) 
 9  color transformations using the Teff and assuming subgiant/dwarf status 
 9  inferred by Reddy & Lambert (2008MNRAS.391...95R)
10 SB 1 with P=347-days and e=0.38 according to Latham et al. (2002,
10  Cat. J/AJ/124/1144)-the double-lined nature of the star is detected in our 
10  spectrum
11 Axer et al. 1994A&A...291..895A
12 Binary with 25" separation and 5.5 photographic magnitude brightness 
12  difference (Allen et al. 2000, Cat. J/A+A/356/529)
13 Zhang & Zhao 2005MNRAS.364..712Z
14 The log g value of Reddy & Lambert (2008MNRAS.391...95R) is 0.5dex larger 
14  than that implied for their spectroscopic Teff by the Yale-Yonsei 
14  isochrones. The logg value is determined from our Teff value assuming dwarf 
14  status implied by the results of Reddy & Lambert (2008MNRAS.391...95R) and 
14  Zhang & Zhao (2005MNRAS.364..712Z)
15 Zhang & Zhao (2003ChJAA...3..453Z) find EW(Li)=37.4m{AA} and A(Li)=2.20
16 Alonso & Martinez-Roger 1996, Cat. J/A+AS/117/227
17 Cenarro et al. 2007, Cat. J/MNRAS/374/664
18 Ivans et al. 2003ApJ...592..906I
19 James 2000, Ph.D. thesis, Univ. Texas, Austin
20 Ivans et al. (2003ApJ...592..906I) find EW(Li)=32.7m{AA} and A(Li)=2.35
21 Schuster et al. 2006, Cat. J/A+A/445/939
22 Boesgaard et al. (2005ApJ...633..398B) find A(Li)=2.28 and EW(Li)=34.5+/-1.4
23 Simmerer et al. 2004, Cat. J/ApJ/617/1091
24 Binary with 0.8" separation and a photographic brightness difference of 2mag 
24  resolved by speckle interferometry (Rastegaev et al. 2007, Cat. 
24  J/other/AstBu/62.235)
25 Fulbright 2000, Cat. J/AJ/120/1841
26 Gravity estimated from our adopted Teff and/or Hipparcos-based MV value 
26  using an 8Gyr Yale-Yonsei isochrone
27 Gratton et al. 2003, Cat. J/A+A/404/187
28 Zhang & Zhao 2006, Cat. J/A+A/449/127
29 Clementini et al. 1999MNRAS.302...22C
30 Jonesell et al. 2005, Cat. J/A+A/440/321
31 Fulbright (2000, Cat. J/AJ/120/1841) finds EW(Li)=13.0 and A(Li)=1.70
32 Gratton et al. 1996, Cat. J/A+A/314/191
33 Bensby et al. 2005, Cat. J/A+A/433/185
34 Sousa et al. 2011, Cat. J/A+A/526/A99
35 Edvardsson et al. 1993, Cat. J/A+A/275/101
36 Ramirez et al. 2007, Cat. J/A+A/465/271
37 Reddy et al. 2006, Cat. J/MNRAS/367/1329
38 The Teff and log g values of Axer et al. (1994A&A...291..895A) are 200K 
38  hotter and >=0.7dex smaller than other photometric and spectroscopic 
38  determinations-we do not utilize their values here
39 Zhang et al. 2009, Cat. J/ApJ/706/1095
40 Ishigaki et al. 2010PASJ...62..143I
41 Schuster & Nissen 1989A&A...222...69S, Cat. II/180
42 Tomkin et al. 1992AJ....104.1568T
43 Pilachowski et al. 1993ApJ...407..699P
44 Cavallo et al. 1997PASP..109..226C
45 Gratton et al. 2000, Cat. J/A+A/354/169
46 Beers et al. 1999, Cat. J/AJ/117/981
47 Teff uncertainty is adopted
48 Ryan & Norris 1991AJ....101.1865R
49 The Hipparcos parallax and spectroscopic gravity estimates indicate that the 
49  dwarf status inferred from Carney et al. (1994, Cat. J/AJ/107/2240) is 
49  incorrect
50 Nissen & Schuster 2010A&A...511A..10C
51 Carney et al. 1997AJ....114..363C
52 Yong & Lambert 2003, Cat. J/PASP/115/22
53 Gravity estimated from both our adopted Teff and/or the Hipparcos-based MV 
53  value using the 12Gyr Yale-Yonsei isochrone
54 Jones et al. 1995PASP..107..632J
55 Carney et al. (1997AJ....114..363C) find EW(Li)=11.2m{AA} and 
55  A(Li)=0.89+/-0.15
56 The low Li and negligible parallax suggest subgiant status
57 Mishenina & Kovtyukh 2001
58 Valenti & Fischer 2005
59 Fulbright (2000, Cat. J/AJ/120/1841) finds EW(Li)=16.0 and A(Li)=1.34, and 
59  Shi et al. (2007A&A...465..587S) find A(Li)=1.60
60 Fuhrmann 1998A&A...338..161F
61 Fulbright (2000, Cat. J/AJ/120/1841) finds EW(Li)=7.9m{AA} and A(Li)=1.37 and
61  Gutierrez et al. (1999A&AS..137...93G) find EW(Li)<13m{AA}
62 Mishenina et al. 2000A&A...353..978M
63 The spectroscopic gravity of Valenti & Fischer (2005, Cat. J/ApJS/159/141) is
63  a factor of 2.5 smaller than that implied by the Yale-Yonsei isochrones for 
63  their Teff value. We adopt the isochrone value implied by our adopted Teff 
63  and the Hipparcos-based MV value
64 Nissen et al. 2007A&A...469..319N
65 Nissen et al. 2004, Cat. J/A+A/415/993
66 Caffau et al. 2005A&A...441..533C
67 Rebolo et al. (1988A&A...192..192R) find EW(Li)=37m{AA} and A(Li)=2.24
68 Latham et al. (2002, Cat. J/AJ/124/1144) find SB1 with P=6083 days and 
68  e=0.52, and Horch et al. (2002AJ....123.3442H) used speckle interferometry 
68  to detect a companion with {rho}=0.15" separation
69 Gutierrez et al. (1999A&AS..137...93G) find EW(Li)=26m{AA}, and White et al. 
69  (2007, Cat. J/AJ/133/2524) find EW(Li)=37m{AA}.