Table A.3:
Low luminosity class stars, likely members of the Milky Way halo. Columns
are the same as in Table A.1.
| ID |
RA(J2000) |
Dec(J2000) |
V |
V-I |
Spectral type |
Rg |
 |
S/N |
Metallicity |
Comments |
| (1) |
(2) |
(3) |
(4) |
(5) |
(6) |
(7) |
(8) |
(9) |
(10) |
(11) |
| D_8 |
0:14:16.16 |
-39:09:38.16 |
18.945 |
-0.161 |
A5V |
-564.09 |
75 |
69 |
- |
neb. |
| D_30 |
0:14:32.02 |
-39:10:17.03 |
19.746 |
0.139 |
G2-5V |
-326.59 |
34 |
36 |
- |
|
| C1_3 |
0:14:40.77 |
-39:12:01.07 |
19.016 |
-1.017 |
Da |
-192.58 |
106 |
111 |
- |
|
| C2_3 |
0:14:42.07 |
-39:11:17.16 |
19.045 |
-0.020 |
B2V |
-173.70 |
107 |
40 |
- |
|
| C1_7 |
0:14:45.26 |
-39:11:42.36 |
18.455 |
-0.197 |
G0-2V |
-125.18 |
136 |
93 |
- |
neb. |
| C2_7 |
0:14:45.38 |
-39:11:17.16 |
18.440 |
-0.160 |
B3V |
-124.34 |
79 |
55 |
- |
neb. |
| C1_26 |
0:14:55.76 |
-39:12:36.72 |
19.046 |
-0.388 |
B8V |
42.26 |
171 |
40 |
- |
neb. |
| C1_33 |
0:15:03.24 |
-39:11:52.08 |
17.373 |
-0.056 |
G5V |
144.62 |
74 |
131 |
- |
|
| B_1 |
0:15:11.68 |
-39:10:10.57 |
18.120 |
0.191 |
G0-2V |
277.62 |
160 |
117 |
- |
|
| B_14 |
0:15:21.01 |
-39:12:50.05 |
19.677 |
0.006 |
B2V |
413.07 |
179 |
75 |
- |
neb. |
| B_27 |
0:15:28.60 |
-39:13:20.64 |
19.278 |
-0.014 |
A5V |
528.55 |
228 |
43 |
- |
|
| B_29 |
0:15:32.54 |
-39:12:52.56 |
19.572 |
0.326 |
F8V |
585.76 |
157 |
55 |
- |
|
| B_32 |
0:15:38.10 |
-39:12:08.64 |
18.438 |
0.212 |
G5V |
667.73 |
20 |
67 |
- |
|
Source LaTeX |
All tables |
In the text