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Table 1

Spectral types and photometry for stars in the region.

ID RA Dec V B − V Sp. classa Sourceb RVc AV
(2000) (2000) [mag] [mag] [mag]

TYC 9414-0186-1 10:59:06.97 –77:01:40.30 11.66  ±  0.15 1.26  ±  0.32 G9 V (2) A 5.58  ±  0.72 2.76  ±  0.26
TYC 9410-1931-1 10:59:29.16 –76:11:15.50 11.29  ±  0.11 1.72  ±  0.32 G4 III (1) A 0.86  ±  0.45 0.77  ±  0.14
TYC 9410-2587-1 10:59:39.81 –76:24:15.60 11.17  ±  0.08 0.51  ±  0.10 G2 V (1) A
TYC 9410-0532-1 11:01:25.94 –76:45:07.40 9.83  ±  0.03 0.47  ±  0.04 A9 V (1) A 4.43  ±  0.29 0.87  ±  0.09
HD 95883 11:01:28.86 –75:39:51.98 7.33  ±  0.01 0.13  ±  0.02 A2 Vn... (1) B 3.55  ±  0.47 0.28  ±  0.08
TYC 9414-0642-1 11:03:11.57 –77:21:04.28 11.48  ±  0.11 1.11  ±  0.22 G2 V (1) A 6.32  ±  2.96 3.01  ±  0.17
TYC 9414-0150-1 11:03:31.68 –76:56:04.89 10.69  ±  0.05 0.37  ±  0.06 A2 (2) C 4.97  ±  0.32 1.61  ±  0.17
TYC 9410-2633-1 11:03:36.31 –75:59:03.40 10.76  ±  0.07 0.55  ±  0.09 G4 V (2) A 0.18  ±  6.15  <0.09
TYC 9410-2362-1 11:04:10.22 –76:22:18.20 10.89  ±  0.06 0.73  ±  0.09 A7 V (2) A 1.30  ±  0.36 0.68  ±  0.17
TYC 9410-2504-1 11:04:37.92 –76:19:00.90 11.37  ±  0.10 0.63  ±  0.15 F8 V (1) A 9.22  ±  1.53 1.03  ±  0.13
TYC 9410-2172-1 11:04:43.80 –76:16:45.20 11.47  ±  0.11 0.90  ±  0.21 F5 V (2) A 1.21  ±  0.76 0.55  ±  0.28
TYC 9410-1907-1 11:06:07.52 –75:55:09.10 10.58  ±  0.05 0.94  ±  0.08 F8 III (1) A 2.72  ±  0.30 1.09  ±  0.12
TYC 9410-2117-1 11:08:23.42 –75:56:34.20 11.12  ±  0.08 1.03  ±  0.16 M2 V (1) A
N0136-0067899 11:09:07.70 –76:18:14.80 11.87  ±  0.10 1.10  ±  0.10 K7 III (2) A
TYC 9410-2426-1 11:12:50.73 –75:58:07.00 9.82  ±  0.03 0.48  ±  0.03 F0 (2) C 5.02  ±  0.45 0.93  ±  0.14
PPM 371023 11:12:54.83 –75:52:11.93 9.15  ±  0.02 1.40  ±  0.04 K5 (2) C 2.25  ±  4.14  <0.44
TYC 9410-2449-1 11:13:26.29 –76:19:23.30 11.60  ±  0.12 0.61  ±  0.17 G2 V (2) A
TYC 9414-0649-1 11:13:48.08 –77:50:12.37 11.59  ±  0.14 1.26  ±  0.30 G7 III (1) A 2.62  ±  0.98 0.91  ±  0.17
TYC 9414-0462-1 11:14:09.38 –77:14:49.50 10.93  ±  0.08 1.85  ±  0.29 K3 III (2) A 3.30  ±  0.62 1.90  ±  0.36
TYC 9414-0260-1 11:14:11.23 –77:01:15.10 10.96  ±  0.07 0.51  ±  0.08 F2V (2) A 8.68  ±  0.77 1.32  ±  0.22
TYC 9414-0392-1 11:14:29.64 –77:07:06.40 11.19  ±  0.09 0.73  ±  0.13 G2 V (1) A 4.64  ±  1.46 0.47  ±  0.11
TYC 9414-0046-1 11:14:45.15 –76:58:20.80 11.33  ±  0.09 1.22  ±  0.21 G4 III (1) A 3.44  ±  0.61 1.35  ±  0.14
TYC 9410-1825-1 11:15:17.32 –76:08:56.70 11.70  ±  0.12 0.30  ±  0.14 B9 V (1) A 3.62  ±  0.51 1.26  ±  0.19
TYC 9410-2634-1 11:15:30.57 –76:29:02.30 11.68  ±  0.14 1.37  ±  0.30 F8 V (1) A 1.01  ±  0.44 0.86  ±  0.17
TYC 9410-2731-1 11:15:57.31 –76:29:08.50 11.27  ±  0.10 2.23  ±  0.37 M0 III (2) A 3.04  ±  0.65 2.04  ±  0.47
TYC 9410-2612-1 11:17:30.79 –76:27:07.90 10.07  ±  0.04 2.03  ±  0.17 M3 III (1) A 3.02  ±  0.67 1.27  ±  0.56
TYC 9414-0080-1 11:18:19.91 –77:07:16.70 9.98  ±  0.03 1.10  ±  0.06 G7 III (2) A 2.99  ±  0.40 0.56  ±  0.07
TYC 9410-0488-1 11:18:21.19 –76:40:56.00 10.80  ±  0.07 2.27  ±  0.29 K6 III (1) A 1.22  ±  0.46 0.91  ±  0.13
TYC 9410-1231-1 11:19:54.76 –75:38:38.21 10.27  ±  0.04 0.52  ±  0.05 A5 (2) C 1.87  ±  0.32 0.69  ±  0.14
TYC 9415-0403-1 11:20:07.20 –76:55:24.00 11.69  ±  0.12 0.43  ±  0.15 A6 V (1) A 3.72  ±  0.70 0.94  ±  0.15
TYC 9411-0934-1 11:20:47.70 –76:37:11.30 11.73  ±  0.15 1.69  ±  0.35 K4 III (2) A 4.19  ±  1.57 1.32  ±  0.69
TYC 9411-1630-1 11:21:50.85 –76:37:25.70 10.38  ±  0.05 1.92  ±  0.19 K4 III (2) A 2.44  ±  0.81 1.32  ±  0.67
HD 99418 11:24:51.67 –76:36:42.59 9.22  ±  0.02 1.32  ±  0.04 G9 III: (1) B 4.26  ±  0.18 1.49  ±  0.11
HD 99558 11:25:47.95 –76:30:29.15 9.13  ±  0.02 1.19  ±  0.03 K0 III (1) B 4.90  ±  0.53 0.91  ±  0.23
HD 99591 11:26:04.34 –75:43:34.95 9.37  ±  0.02 0.54  ±  0.03 F7 V (2) C 0.51  ±  10.18 0.03  ±  0.25

Notes. 

(a)

The number in parenthesis gives the estimated uncertainty of the spectral class, in sub-classes;

(b)

source of spectral classification: A – this work, B – Michigan Spectral Survey (Houk & Swift 1999), C – SIMBAD database;

(c)

in a few cases unphysical results were obtained for RV. These likely indicate non-standard spectral classes. Those values have been omitted and marked by – and the resulting visual extinctions were not used in the analysis.

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