Standard Stars in VSP

The 2009 Landolt UBVRI Equatorial Standard Fields are being added to VSP. Descriptions of all the fields are included in the tables below. In order to plot them you need to enter the coordinates and size of the field you want. This table gives the field center coordinates of the fields. Quick link to VSP

NOTES:

  • Field GD71 was taken out because it overlapped onto the comparison star sequence for Z and RU Tauri.
  • No single stars or stars with less than 5 observations are included as standards.

Field Name

 RA(J2000.0)

 Dec(J2000.0)

 FOV

Range V

 Range B−V

SA92

 00:55:15.5

+00:47:26

 70x 70

 10.60 ↔ 15.92

 +0.32 ↔ +1.64

F 11

 01:04:25.0

+04:12:31

 10x 10

 12.06 ↔ 14.47

 −0.24 ↔ +0.84

SA93

 01:55:01.8

+00:49:52

 60x 60

 11.55 ↔ 12.01

 +0.49 ↔ +1.08

PG0220+132

 02:23:36.9

+13:27:47

 10x 10

 14.22 ↔ 15.77

 −0.13 ↔ +0.94

PG0231+051

 02:33:38.5

+05:19:00

 15x 15

 12.77 ↔ 16.10

 −0.32 ↔ +1.44

F 24

 02:35:17.0

+03:42:54

 15x 15

 11.76 ↔ 13.82

 −0.20 ↔ +1.13

SA94

 02:55:56.1

+00:43:29

 70x 70

 11.20 ↔ 14.29

 +0.30 ↔ +1.42

SA95

 03:54:26.8

+00:13:48

 70x 70

 10.01 ↔ 16.27

 −0.21 ↔ +2.00

SA96

 04:52:17.3

+00:03:50

 70x 70

 10.59 ↔ 13.78

 +0.18 ↔ +1.34

SA97

 05:57:55.8

+00:05:54

 60x 60

 9.78 ↔ 14.09

 +0.20 ↔ +1.87

SA98

 06:52:03.5

−00:19:27

 30x 30

 9.54 ↔ 17.80

 +0.00 ↔ +2.19

Ru149

 07:24:15.2

−00:32:12

 15x 15

 11.48 ↔ 14.49

 −0.13 ↔ +1.11

Ru152

 07:29:59.9

−02:05:38

 15x 15

 11.08 ↔ 15.02

 −0.19 ↔ +0.88

SA99

 07:54:50.0

−00:33:13

 60x 60

 9.40 ↔ 11.15

 −0.16 ↔ +1.25

SA100

 08:53:14.3

−00:37:56

 60x 60

 9.15 ↔ 13.03

 +0.16 ↔ +1.32

PG0918+029

 09:21:32.1

+02:47:01

 15x 15

 12.27 ↔ 14.49

 −0.27 ↔ +1.04

PG0942−029

 09:45:11.5

−03:08:04

 15x 15

 13.68 ↔ 14.95

 −0.30 ↔ +0.89

SA101

 09:56:35.0

−00:29:46

 60x 60

 9.74 ↔ 16.50

 +0.26 ↔ +1.5

GD 108

 10:00:47.8

−07:32:41

 10x 10

 13.56 ↔ 15.06

 −0.21 ↔ +0.84

PG1047+033

 10:50:08.3

 −00:01:18

 15x 15

 12.45 ↔ 14.75

 −0.29 ↔ +0.69

SA102

 10:56:04.1

−00:30:46

 60x 60

 9.90 ↔ 10.07

 +0.66 ↔ +1.08

G163 50/51

 11:07:44.4

−05:12:50

 15x 15

 11.29 ↔ 14.47

 +0.04 ↔ +1.50

SA103

 11:56:30.1

−00:35:35

 60x 60

 9.86 ↔ 11.84

 +0.37 ↔ +1.09

SA104

 12:43:10.2

−00:33:59

 70x 70

 9.37 ↔ 16.09

 +0.44 ↔ +1.5

PG1323−086

 13:25:52.4

−08:49:47

 15x 15

 12.08 ↔ 14.00

 −0.14 ↔ +0.76

SA105

 13:37:43.6

−00:20:08

 70x 70

 10.27 ↔ 12.54

 +0.25 ↔ +1.42

PG1407−013

 14:10:30.0

−01:27:40

 15x 15

 12.46 ↔ 15.18

−0.26 ↔ +1.15

SA106

 14:42:10.5

−00:17:41

 70x 70

 9.34 ↔ 11.60

 +0.33 ↔ +1.36

PG1525−071

 15:28:14.0

−07:15:35

 15x 15

 13.51 ↔ 16.39

−0.21 ↔ +1.12

SA107

 15:38:48.6

−00:13:29

 70x 70

 9.04 ↔ 16.05

 +0.12 ↔ +1.60

PG1633+099

 16:35:34.6

 +09:48:23

 15x 15

 12.97 ↔ 15.26

 −0.19 ↔ +1.14

SA108

 16:37:19.0

−00:14:22

 60x 60

9.06 ↔ 12.69

 +0.18 ↔ +1.4

PG1657+078

 16:59:31.3

 +07:43:04

5x 15

14.03 ↔ 16.16

0.14 ↔ +1.07

SA109

 17:44:54.6

−00:15:48

 60x 60

 9.33 ↔ 14.64

 +0.33 ↔ +1.74

SA109 SF1

 17:45:31.2

 −00:23:44

10x 10

 9.33 ↔ 10.35

 +0.61 ↔ +1.47

SA110

 18:42:20.5

+00:11:05

60x 60

 10.03 ↔ 16.25

 +0.31 ↔ +2.53

SA111

 19:37:49.7

+00:21:35

 60x 60

8.96 ↔ 13.19

 +0.21 ↔ +1.96

SA112

 20:42:06.7

+00:13:14

 60x 60

 9.90 ↔ 12.10

 +0.15 ↔ +1.60

Mark A

 20:43:58.7

−10:46:24

 15x 15

 13.26 ↔ 15.91

 −0.25 ↔ +0.94

G26 7

21:31:16.6

 −09:48:41

15x 15

12.01 ↔ 13.45

 +0.56 ↔ +1.66

SA113

 21:42:07.6

+00:22:31

 60x 60

 10.00 ↔ 15.66

+0.28 ↔ +1.34

G93 48

 21:52:17.8

+02:22:23

 15x 15

 12.42 ↔ 13.66

 −0.01 ↔ +1.32

PG2213−006

 22:16:20.6

−00:19:57

5x 15

 12.64 ↔ 15.11

 −0.21 ↔ +0.79

SA114

 22:41:53.5

+00:49:02

 60x 60

 9.24 ↔ 12.64

 −0.04 ↔ +1.49

GD 246

 23:12:24.2

+10:47:43

 15x 15

 12.96 ↔ 14.37

 −0.32 ↔ +0.92

PG2336+004

 23:38:40.9

+00:42:44

 15x 15

 11.27 ↔ 15.88

 −0.16 ↔ +0.69

SA115

 23:42:53.1

+01:05:49

 60x 60

 9.69 ↔ 12.49

 +0.47 ↔ +1.03


The 2007 Landolt UBVRI Standard Fields around -50 degress declination are all available in VSP now. The table below gives the coordinates for the field centers of these fields.
Quick link to VSP

Field Name

RA(2000.0)

Dec(2000.0)

JL 163

00 10 42.6

−50 14 10

T Phe

 00 30 34.4

−46 28 08

MCT 0401-4017

 04 03 01.2

−40 11 28

LB 1735

 04 31 34.7

−53 37 13

MCT 0436-4616

 04 38 34.2

−46 10 10

MCT 0550-4911

 05 51 53.9

−49 10 31

LSS 982

 08 10 29.1

−40 30 34

WD 0830-535

 08 31 56.5

−53 40 52

WD 1056-384

 10 58 15.9

−38 44 07

WD 1153-484

 11 56 03.6

−48 39 50

LSE 44

13 52 45.0

−48 09 17

LSE 259

 16 53 45.1

−56 00 16

MCT 2019-4339

 20 22 51.5

−43 29 24

JL 82

 21 36 01.0

−72 47 51

JL 117

22 54 55.5

−72 22 59

This is another excellent example of a volunteer driven project that would either take forever or not get done at all if the staff were required to do the leg work. I would personally like to express my sincere gratitude to Terry Bohlsen for making this possible. 

Mike Simonsen