STRUCTURE OF NGC 2420 ABSTRACT A new examination of the structure of NGC 2420 has been made according to Kholopov's method. 1890 stars were measured between the circles of about 6' and 25' radius centred on the cluster, for which photographic B,V magnitudes and positions were obtained down to the limiting magnitude of plates ( 17.8m in V ) but in constructing the density distributions stars down to 17.5m were chosen. A literature determination of the proper motion of stars in a circle of 12' radius was used to define the place and shape of the C-M diagram. Around this diagram bands of 0.1m, 0.2m and 0.3m width in B-V were drawn to select the members of the cluster. The stars were separated into four groups and surface density distributions were made for the whole cluster and for each subgroup. The distributions of the stars reveal two different parts of the cluster: the core has a radius of 5.1 pc, whereas the halo extends as far as 12.7 pc. The brighter stars belong to the core and many of fainter ones to the halo - as might be expected from the theory. The whole halo seems to be steady against the irregular forces of background stars but the outer part of the halo from 8.2 pc radius is not stable against the tidal force. INTRODUCTION As early as at the beginning of this century Shapley (1916) pointed out that outside an inner dense part in M 67 the density is ten times higher than the density of the background typical in this galactic latitude. According to Shapley the well-defined part with 6.5' radius in M 67 is only the core of a more extensive cluster. In 1922 Trumpler obtained similar result for Pleiades, Praesepe, h Persei, M 11 and M 37. This phenomenon has been investigated fairly accurately by Kholopov (1953, 1968) and Artuhina (1966) since 1953. They have studied about twelve clusters, both open and globular ones and have found that each cluster consists of two main parts: core and halo. A preliminary examination of the open cluster NGC 2420 was made by the author (1977, hereinafter Paper I) in accordance with Cannon's photometry. The area of 12' radius centred on the cluster measured by Cannon proved too small to demonstrate the halo of the cluster which seems to extend further than 12'. The aim of present work is to investigate a larger area around the cluster following Kholopov's method described in Paper I and to define the radius of the halo. OBSERVATIONAL MATERIAL From the observational point of view, the open cluster NGC 2420 is highly appropriate. Its galactic coordinates are: l^II=198 deg, b^II=+20 deg. Because of the high galactic latitude the interstellar reddening has only a small value and the density of the background stars is considerably smaller than in the galactic plane. The observations were carried out with the 60/90/180 cm Schmidt telescope of Konkoly Observatory's mountain station in the period 1976-1977. B,V colours were derived for 1890 stars brighter than 17.8m photographic magnitude. The photometry is based on five plates taken in each colour. The emulsion types, filters and exposure times used are given below: plate filter exposure time B Kodak 103a-O Schott GG_13 2mm 30m V Kodak 103a-D Schott GG_14 2mm 30m The international system is connected with the instrumental system by the equations: V_instr = V - 0.112(B-V) + 0.074 (B-V)_instr = 0.933(B-V) + 0.029 The plates were measured with Konkoly Observatory's Cuffey-type iris photometer using 15 photoelectric standards taken from West's article (1967). The mean errors of the photographically determined colours are +-0.06m in both B and V. The scale of the Schmidt plates did not allow the measurement of the stars in the centre of the cluster. The stars were measured between the circles of about 6' and 25' radius centred on the cluster, as identified on the chart shown in Fig. 6 a,b,c,d. The magnitudes and positions are listed in the Table. The inner part of the cluster was studied by the photometry of West (1967), Cannon and Lloyd (1970) and McClure et al. (1974). There are overlaps between these works and the area measured by the author. Stars in the overlapping areas were used to transform the magnitudes into a common system. The magnitudes were not corrected for interstellar reddening because its values are negligible. According to McClure et al. (1974) E(B-V) = 0.02m and E(U-B) = 0.02m.
Fig. 1 The C-M diagram of NGC 2420
SURFACE DENSITY DISTRIBUTION
When studying the structure of open clusters according to density
distribution we have to pay great attention to the construction of
density distribution curves. In the early fifties Kholopov (1953) began
to deal with this problem and discussed in detail which parts of the
examination need special care.
a. Since in the clusters there are stars of different mass and they play
a different role in the dynamic evolution of clusters, it is very useful
to separate them into different subsystems. For this purpose the cluster
was divided into subsystems by boxes according to Cannon's article on
the C-M diagram (Fig.1). The size of the boxes also depends on the
number of stars belonging to the box. The boxes marked A,B,C,E and F
were treated together because of the small number of stars in each box.
The stars in these boxes all are giants, so they play a similar role in
the dynamic evolution of clusters. Density distributions were made for
the whole cluster and the following subgroups:
A+B+C+E+F group - containing the brightest stars (m~1.2 M_Sun)
D group - containing the turn-off point of the cluster (m~1.2 M_Sun)
G group - where m~1.0 M_Sun
H group - where m~0.8 M_Sun
b. Cannon and Lloyd (1970) determined the proper motion of stars in NGC 2420
in a circle of 12' radius. McClure et al. (1974) using their own photometry
and Cannon's proper motions, made the C-M diagram of the cluster for which
they fitted a theoretical diagram. Around this diagram, bands of 0.1m,
0.2m and 0.3m width in B-V were drawn to investigate that particular width
in which the ratio of member stars to non member stars is suitable. This
means that most of the member stars of the cluster belong to the band but
the number of non member stars is as small as possible. In Fig.2 a,b,c
the cumulative frequency distribution can be seen for different width versus
distance measured from the centre. The number of the stars in a circle of r
radius (N(r)) comes from the number of member stars and background stars.
Supposing uniform distribution of background stars, a parabola can be fitted
for the outer part of the cumulative frequency distribution. According to
the investigation the right width is around 0.2m. Adopting Cannon's result
that the natural width of the C-M diagram of NGC 2420 is less than 0.1m and
taking the error of BV photometry to 0.1m, the final width of the band was
chosen to be 0.15m.
Fig. 2 a,b,c The cumulative frequency distributions for bands of
0.1m, 0.2m and 0.3m width in B-V.
c. The position of the measured stars in the Cartesian coordinate system
on the plate can be found in the Table. The zero point of the coordinate
system is the star named II-1-20 by West (1967). As a first approximation
this point was chosen for the centre of the cluster, but the equal density
curves became asymmetrical. As a second approximation the arithmetical mean
was used for the centre. After correction, the equal density curves are
much more symmetrical (Fig. 3 a,b).
Fig. 3 a,b The equal density curves before the modification of the
centre and after it.
d. In accordance with Kholopov's method described in Paper I the surface
density distribution was made for the whole cluster and for each subgroup.
The curves concern the outermost part of the cluster (Fig. 4 a,b,c,d,e).
Fig. 4 a Density distribution curve for the whole cluster.
Fig. 4 b Density distribution curve for the A+B+C+E+F group.
Fig. 4 c Density distribution curve for G group.
Fig. 4 d Density distribution curve for H group.
Fig. 4 e Density distribution curve for the D group.
DISCUSSION OF THE DENSITY DISTRIBUTIONS
In Paper I, selection of the members of the cluster was based on the proper
motion of stars, but there are no proper motion measurements for the stars in
the outer part of the cluster. To select the cluster members in the present
case a band of suitable width was defined in B-V around the C-M diagram of the
cluster. A comparison could be made between these two methods by deriving the
densities for Cannon's stars selected by both criteria. The curves can be seen
in Fig. 5. The curves made by two different methods are mostly the same within
a sigma error bar, but at that part where the density gradient is highest the
curves are within two sigma error bars. From these examinations the existence
of the different density parts and the place of the inflexion point can be
defined more or less exactly.
Fig. 5 Density distribution curves made by different methods.
In Paper I the density distribution of stars in the centre of the cluster was
discussed. Two different parts could be seen according to the change in the
density gradient. The large negative density gradient of the inner dense part
changes at a radius of about 3.3' and continues with a less steep decline in
the outer less dense part having a radius of 7.4'.
The examination of density distribution is extended in this paper to 25'
from the centre using the band criteria for the selection. The density
distribution of the whole cluster has a small but defined slope as far
as about 18'. Around the central part of NGC 2420 can be seen the halo
of very low density. At the A+B+C+E+F group of bright stars beyond about
7' the cluster cannot be estimated. The curve for this group comes from
the fluctuation of the background stars. The density distributions of
the D,G and H groups have a defined slope except some lower local
minimum. "Defined slope" means the existence of a halo of fainter
stars. The inner part of greater density continues to 3.8 mm which is
equal 7'17" taking into account the 115"/mm scale of Schmidt plates.
This result is almost the same as the value of the less dense part in
Paper I. The border of the outer lower density part is 9.5 mm = 18'13".
Using a distance of 2400 pc (West, 1967) for NGC 2420, the core of the
cluster has a 5.1 pc radius, the halo of the cluster has 12.7 pc.
Salukvadze (1977) obtained a much higher value for the radius of the
core and the halo but I believe it comes only from the fluctuation of
the background stars.
A similar result has been obtained by Archemashvili (1979) for this
cluster. For faint objects the mean radius of core is 5.5' (3.2 pc) and
15.5' (9 pc) for the halo. He got a 2.5' (1.4 pc ) radius for the
brightest stars: this value is consistent with our 3.3' (2.3 pc) data in
Paper I. Taking into account the difference between the used distances
the results are the same within 1 pc.
According to Agekyan and Belozerova (1979) the effective radius of the
halo of the cluster is
R ~ 0.351 N^1/2 / D^1/3
Using N = 300 as the estimated number of member stars in NGC 2420 and
D = 0.12/pc^3, the effective radius of the halo of NGC 2420 is R = 12.3 pc.
D = 0.12/pc^3 is a general value. The density of the background stars at the
present position of the cluster is considerably lower but during its lifetime
this cluster crossed the galactic plane many times, where this effect was much
stronger than nowadays. The R = 12.3 pc effective radius means that the cluster
seems to be stable against the irregular forces of its background stars.
The limiting radius of a cluster, because of the tidal force in the
Galaxy, can be given by the following equation (King, 1962)
r_lim = R_p ( M/3.5 M_g)^1/3
where M means the mass of the cluster, M_g the mass of Galaxy, and R_p
the perigalactic distance of the cluster. Taking R_p = 8.6 kpc of "A"
model from Keenan and Innanen (1974) and using N = 300 value for member
of cluster as before and supposing 1 M_Sun for each, member star and
10^11 M_Sun for the mass of Galaxy, the limiting radius equal 8.2 pc for the
NGC 2420 open cluster. Within this radius the cluster is stable whereas
beyond it the stars evaporate because of the tidal force.
CONCLUSION
The NGC 2420 open cluster consists of a high density core with 5.1 pc radius
and a lower density halo of 12.7 pc. Within the high density core there is a
concentration of the brightest stars with 2.3 pc radius. The halo of the
cluster seems to be stable against the irregular forces of the background stars
and the inner part of halo from 5.1 pc to 8.2 pc is also stable against the
tidal force. The outer part of the halo from 8.2 pc to 12.7 pc is not stable
and is gradually destroyed by the tidal force.
ACKNOWLEDGEMENTS
I am indebted to Dr. B.A. Balazs for calling my attention to this problem and
to Dr. L.G. Balazs for valuable discussions. I am grateful to Mrs. I. Kalman
and Mrs. I. Gal for their assistance in analysing the data.
Budapest - Szabadsaghegy, September 7, 1982
REFERENCES
Agekyan, T.A., Belozerova, M.A. 1979, Astr.Zhu. 56. 9.
Archemashvili, V.M. 1979, Bull.Ac.Sci.Georg. 93. No. 2. 333.
Artuhina, N.M., Kholopov, P.N. 1966, Astr.Zhu. 43. 567.
Cannon, R.D., Lloyd, C. 1970, M.N.R.A.S. 150. 279.
Keenan, D.W., Innanen, K.A. 1974, Ap.J. 189. 205.
King, I. 1962, Astron.J. 67. 471.
Kholopov, P.N. 1953, Astr.Zhu. 30. 426.
Kholopov, P.N. 1968, Astr.Zhu. 45. 786.
McClure, R.D., Forrester, W.T., Gibson, J. 1974, Ap.J. 189. 409.
Paparo, M. 1977, Spatial structure of NGC 2420, in The role of
star clusters in cosmogony and in the study of galactic
structure, Ed. B.A. Balazs, Roland Eotvos Univ. p.47.
Salukvadze, G.N. 1977, Bull.Abastumansk.Astrofiz.Obs. 48. 135.
Shapley, H. 1916, Mt.W.Contr. 117.
Trumpler, R.J. 1922, Allegheny Publ., 6. No. 4.
West, F.R. 1967, Ap.J.Suppl. XIV. 384, 359.
Fig. 6 a Finding chart of the survey stars I.
East-northern part of the field
Fig. 6 b Finding chart of the survey stars II.
East-southern part of the field
Fig. 6 c Finding chart of the survey stars III.
South-western part of the field
Fig. 6 d Finding chart of the survey stars IV.
West-northern part of the field
Table
No. V B-V X Y No. V B-V X Y
1 17.54 0.31 -12.8 1.2 51 16.81 0.68 - 9.9 4.6
2 16.56 0.84 -12.4 1.2 52 14.26 0.70 -10.2 4.9
3 15.51 0.71 -12.1 1.2 53 16.21 1.18 -10.7 5.0
4 14.79 0.43 -12.0 0.9 54 16.36 0.88 -10.8 5.2
5 14.40 0.71 -11.5 0.8 55 17.43 0.89 -10.9 5.4
6 17.45 0.50 -10.9 0.6 56 15.17 0.98 -11.6 5.9
7 17.40 1.11 -10.8 0.4 57 15.71 1.00 -11.2 6.4
8 16.62 0.52 -10.4 0.5 58 14.98 0.44 -11.2 6.6
9 16.98 0.77 -10.2 0.6 59 17.07 0.30 -10.9 6.4
10 17.36 0.17 - 9.9 0.7 60 17.51 0.81 -10.6 6.4
11 15.28 0.25 -10.6 0.9 61* 16.20 0.22 -10.6 6.3
12 14.76 1.19 -10.8 1.0 62* 16.27 0.92 -10.5 6.4
13 13.86 0.58 -11.1 1.0 63 17.69 - -10.1 5.5
14 15.17 0.87 -11.6 1.2 64 17.51 1.32 -10.0 5.9
15 16.83 0.43 -12.0 1.6 65 14.84 0.86 -10.0 6.1
16 14.90 0.83 -11.9 1.7 66 17.44 0.63 - 9.9 6.8
17 17.54 1.10 -11.5 1.6 67 16.85 0.39 -10.0 6.8
18 16.16 0.92 -11.5 1.4 68 16.79 0.45 -10.3 7.3
19 14.18 0.20 -11.3 1.6 69 17.60 - - 9.8 8.1
20 17.06 0.76 -11.2 1.3 70 17.36 0.77 - 9.4 8.5
21 17.49 - -10.5 1.1 71 16.73 0.64 - 9.3 7.6
22 17.51 0.67 -10.5 1.4 72 16.31 0.66 - 8.8 8.1
23 17.51 - -10.8 1.3 73 14.90 0.64 - 8.8 8.6
24 16.53 0.45 -10.7 1.8 74 16.22 0.76 - 9.1 9.1
25 14.79 0.38 -11.0 2.0 75 13.44 0.80 - 8.9 9.3
26 15.55 0.67 -12.3 2.2 76 15.43 0.67 - 8.6 9.0
27 15.31 1.27 -12.5 2.3 77 15.91 0.62 - 8.6 9.3
28 14.25 0.59 -12.7 2.4 78 16.00 1.42 - 7.7 10.1
29 16.64 0.19 -11.1 2.5 79 15.48 0.90 - 7.1 10.4
30 14.56 0.51 -10.7 2.6 80 15.07 1.05 - 6.8 9.3
31 17.49 - -10.2 3.0 81* 14.61 0.63 - 7.5 9.3
32 17.56 0.63 -10.4 3.1 82 16.51 0.60 - 7.8 9.3
33 14.15 0.81 -10.6 3.1 83 17.25 0.91 - 6.0 8.0
34 17.26 0.51 -10.9 3.1 84 14.71 0.45 - 6.3 7.8
35 17.36 1.17 -11.1 2.9 85 17.38 0.34 - 6.6 7.8
36 16.59 0.38 -11.3 2.9 86 16.01 0.53 - 7.1 7.4
37 17.13 - -11.1 3.3 87 17.54 1.03 - 8.1 8.0
38 15.67 1.22 -10.9 3.6 88 14.35 0.71 - 8.0 7.8
39 17.18 0.88 -11.1 3.8 89 17.53 1.18 - 8.6 7.3
40 16.95 1.68 -11.1 4.0 90 17.42 1.25 - 8.8 7.3
41 17.11 0.78 -11.4 4.1 91 16.29 0.73 - 7.8 7.1
42 17.48 0.62 -11.7 3.9 92 12.30 0.39 - 6.1 7.1
43 15.02 0.41 -11.6 4.3 93 14.46 0.63 - 5.8 6.6
44 17.08 0.47 -12.0 4.5 94 14.87 0.55 - 5.8 6.3
45 15.99 0.28 -11.8 4.9 95 16.71 0.46 - 5.9 6.0
46 13.76 0.53 -11.2 4.8 96 15.52 0.65 - 6.6 5.9
47 17.47 1.13 -10.7 4.2 97 16.79 0.14 - 6.7 6.2
48 13.19 0.87 -10.6 3.8 98 11.97 0.45 - 8.0 6.7
49 17.61 0.69 -10.2 3.5 99 17.45 0.43 - 8.1 6.6
50 13.44 0.56 -10.1 3.9 100 15.90 0.80 - 8.3 6.6
Table (Cont.)
No. V B-V X Y No. V B-V X Y
101* 16.40 0.77 - 9.3 6.6 151* 14.84 0.51 - 8.3 2.0
102 16.18 0.39 - 8.6 6.3 152* 11.84 0.87 - 8.0 2.1
103 13.29 0.32 - 8.5 6.2 153 17.27 0.80 - 7.5 2.5
104 16.00 0.87 - 8.5 5.9 154 14.23 0.52 - 7.5 2.7
105 17.22 1.12 - 9.2 5.9 155 15.53 0.80 - 6.2 3.1
106 15.31 0.78 - 9.6 5.8 156 11.16 0.15 - 5.2 3.1
107 17.65 0.83 - 9.4 5.8 157 17.50 0.62 - 5.0 2.9
108 15.13 0.57 - 9.0 5.5 158 14.62 0.26 - 5.0 2.8
109 17.00 0.67 - 9.3 5.1 159 12.97 0.33 - 5.4 2.3
110 17.63 0.67 - 9.4 4.6 160 17.20 0.56 - 6.3 2.4
111 17.57 0.43 - 9.1 4.6 161 15.33 1.29 - 6.3 2.1
112 15.44 0.62 - 8.8 4.5 162 16.71 0.42 - 6.1 2.1
113 17.49 0.88 - 8.7 4.7 163 15.71 0.69 - 5.9 2.1
114 17.36 0.59 - 8.6 5.2 164 16.17 0.51 - 5.4 2.0
115 11.60 0.42 - 8.3 4.9 165 17.09 0.26 - 5.6 1.8
116 16.08 0.98 - 8.3 4.6 166 16.82 0.53 - 6.4 1.4
117 15.95 0.33 - 8.4 4.2 167 17.73 - - 6.8 1.2
118 16.80 0.62 - 8.1 4.2 168 16.91 1.71 - 7.2 1.4
119 17.67 - - 8.2 4.3 169 15.82 1.01 - 7.8 1.4
120 17.42 0.11 - 7.8 4.6 170 15.19 0.54 - 8.3 1.1
121 17.30 0.85 - 7.0 5.5 171 16.66 0.67 - 8.8 1.5
122 14.54 0.72 - 6.5 5.4 172 17.06 0.63 - 9.0 1.5
123 14.24 0.62 - 5.5 5.4 173 16.48 0.76 - 9.0 1.3
124 17.05 0.58 - 5.4 5.1 174 17.33 0.55 - 9.3 1.4
125 16.07 0.54 - 5.5 4.8 175 16.86 0.38 - 9.5 1.4
126 17.77 0.81 - 5.6 4.7 176* 16.56 0.23 - 9.6 1.5
127 16.24 0.32 - 5.7 4.7 177* 16.82 0.19 - 9.6 1.6
128 16.47 0.60 - 6.0 4.9 178 16.04 0.83 - 9.1 0.9
129 16.19 0.70 - 6.0 5.0 179 17.30 1.01 - 9.3 0.3
130 15.11 0.76 - 6.9 4.8 180 12.41 0.48 - 9.0 0.0
131 16.38 1.20 - 6.8 4.7 181 16.42 0.36 - 8.4 0.7
132 17.46 0.34 - 6.5 4.8 182 17.55 0.66 - 8.3 0.9
133 17.70 0.75 - 6.4 4.4 183 16.08 0.71 - 7.6 0.9
134 17.24 1.49 - 5.7 4.1 184 13.72 0.49 - 6.7 0.2
135 17.22 0.50 - 5.3 3.5 185 16.70 0.59 - 6.6 0.5
136 17.51 0.79 - 5.7 3.5 186 16.47 0.32 - 5.7 0.5
137 15.96 0.72 - 6.3 3.8 187 17.61 1.10 - 5.4 0.7
138 17.34 0.47 - 6.6 3.5 188 15.11 0.74 - 5.2 0.4
139 17.49 0.92 - 7.0 4.1 189 13.85 1.31 - 5.0 - 0.1
140 16.79 1.31 - 7.2 3.9 190 12.81 1.14 - 5.3 - 0.4
141 15.94 0.74 - 7.9 3.7 191 17.76 0.61 - 5.5 - 0.1
142 17.30 0.11 - 8.1 3.8 192 15.17 0.79 - 5.9 - 0.7
143 16.18 0.56 - 8.6 3.9 193 13.67 0.52 - 6.6 - 0.4
144 17.49 0.69 - 8.6 3.5 194 15.95 0.74 - 6.7 - 0.2
145 14.54 0.67 - 9.1 3.8 195 17.47 0.66 - 7.0 - 0.1
146 16.75 0.58 - 9.7 3.7 196 17.56 0.63 - 7.1 - 0.1
147 16.81 0.39 - 9.6 3.5 197 16.71 0.94 - 7.2 - 0.1
148 15.70 0.33 - 9.6 3.1 198 15.41 0.63 - 7.0 - 0.4
149 16.22 0.52 - 9.3 2.3 199 17.57 0.76 - 6.8 - 0.8
150* 14.22 1.17 - 8.6 2.0 200 15.47 0.30 - 6.9 - 0.8
Table (Cont.)
No. V B-V X Y No. V B-V X Y
201 15.90 0.52 - 7.6 - 0.6 251 14.98 0.53 -11.2 - 5.9
202 16.76 0.55 - 8.9 - 0.4 252 14.67 0.45 -10.5 - 6.5
203 15.18 0.75 - 9.9 - 0.9 253 17.50 1.43 -10.5 - 6.6
204 15.65 0.20 -10.0 - 1.1 254 15.55 0.81 -10.5 - 6.8
205 17.48 1.09 -10.1 - 1.3 255 13.06 1.02 - 9.9 - 7.2
206 16.66 0.54 -10.3 - 1.2 256 15.69 0.41 - 9.5 - 6.7
207 13.96 0.57 -10.5 - 1.1 257 17.57 0.29 - 9.4 - 6.6
208 17.01 0.09 -10.3 - 1.1 258 17.68 1.08 - 9.4 - 6.1
209 16.84 1.07 -10.6 - 1.0 259* 15.90 0.39 - 9.3 - 6.0
210 14.60 0.50 -11.6 - 0.8 260 14.00 0.51 - 9.3 - 5.9
211 17.30 0.51 -11.7 - 0.3 261 15.46 0.90 -10.2 - 6.0
212 15.91 1.53 -12.1 0.0 262 13.61 0.33 -10.1 - 5.8
213 16.58 0.80 -12.2 - 0.8 263 12.01 0.62 -10.1 - 5.1
214 17.49 0.60 -11.9 - 1.0 264 15.48 0.68 -10.0 - 5.0
215 17.39 1.29 -12.0 - 1.4 265 17.50 - - 9.5 - 5.3
216 14.40 0.49 -10.8 - 1.5 266 17.24 0.67 - 9.4 - 5.3
217 17.61 0.58 -10.3 - 1.6 267 15.20 0.75 - 9.2 - 5.1
218 17.29 0.78 -10.8 - 2.0 268* 12.80 1.72 - 8.7 - 4.8
219 15.13 0.63 -11.0 - 2.0 269 15.13 1.20 - 8.4 - 4.7
220 16.14 0.55 -11.2 - 2.4 270 16.07 0.99 - 8.4 - 4.6
221 17.19 0.69 -11.5 - 2.5 271 16.57 1.64 - 8.3 - 4.5
222 17.68 0.78 -11.6 - 2.5 272 11.87 1.01 - 8.9 - 4.5
223 15.86 1.51 -11.8 - 2.6 273 15.03 0.50 - 9.4 - 4.5
224 15.65 1.15 -11.8 - 2.5 274 11.96 0.58 - 9.1 - 4.3
225 11.81 1.01 -12.2 - 2.6 275 14.39 0.68 - 9.3 - 4.1
226 13.75 0.75 -12.0 - 3.0 276 17.65 1.29 - 9.3 - 3.9
227 17.08 0.74 -11.9 - 3.0 277 17.54 1.16 - 9.3 - 3.7
228 17.13 0.45 -11.8 - 3.1 278 15.95 0.78 - 9.3 - 3.0
229 16.33 0.45 -11.7 - 2.8 279 17.07 0.59 - 9.3 - 2.8
230 15.94 0.40 -11.2 - 2.8 280 17.01 0.43 - 9.2 - 3.1
231 16.53 0.18 -11.1 - 2.9 281 13.96 0.56 - 9.1 - 3.2
232 14.68 0.51 -10.7 - 2.5 282 16.36 0.26 - 9.0 - 3.4
233 16.75 0.87 -10.4 - 2.6 283 16.20 0.33 - 8.9 - 3.8
234 15.07 0.57 -10.3 - 2.5 284 14.19 0.62 - 8.7 - 3.4
235 15.02 0.31 -10.2 - 2.7 285 14.78 0.70 - 8.5 - 3.1
236 15.60 0.52 -10.6 - 2.8 286 14.39 0.53 - 8.3 - 3.1
237 16.50 0.57 -10.2 - 3.4 287 16.84 0.72 - 8.2 - 2.5
238 14.89 0.43 -10.8 - 3.5 288 16.65 0.55 - 8.6 - 4.2
239 15.52 0.42 -11.3 - 3.3 289 15.99 0.60 - 8.6 - 1.9
240 13.01 0.54 -11.2 - 3.5 290 17.03 0.62 - 8.8 - 1.8
241 15.98 0.45 -12.1 - 3.9 291 16.76 0.50 - 9.3 - 1.3
242* 16.05 0.83 -11.1 - 3.8 292 17.60 - - 8.5 - 1.7
243 17.49 0.17 -10.7 - 3.9 293 17.42 0.63 - 7.9 - 2.1
244 17.45 0.50 -10.3 - 4.1 294 15.86 0.36 - 8.0 - 1.7
245 15.30 0.84 -11.0 - 4.4 295 16.77 0.11 - 8.0 - 1.4
246 17.29 0.79 -10.8 - 4.7 296 17.66 0.33 - 8.1 - 1.2
247 17.10 0.65 -10.8 - 4.8 297 17.51 1.43 - 8.2 - 0.7
248 15.39 0.27 -10.9 - 5.2 298 17.02 1.18 - 7.7 - 1.3
249 14.54 0.48 -10.9 - 5.4 299 17.19 0.20 - 7.5 - 1.1
250 15.48 0.69 -11.1 - 5.4 300 13.86 0.48 - 7.3 - 1.4
Table (Cont.)
No. V B-V X Y No. V B-V X Y
301 15.29 1.52 - 7.1 - 1.2 351 16.66 0.29 - 4.8 - 3.6
302 15.85 0.78 - 6.5 - 1.4 352 15.93 0.43 - 4.3 - 3.8
303 15.84 0.61 - 6.1 - 1.3 353 16.88 0.19 - 4.8 - 3.8
304 17.55 - - 5.9 - 1.3 354 17.52 0.50 - 4.6 - 4.1
305 17.29 0.74 - 5.8 - 1.4 355 15.14 1.11 - 4.4 - 4.4
306 15.03 0.89 - 5.8 - 1.5 356 17.62 0.64 - 4.6 - 4.4
307 16.50 0.18 - 5.3 - 1.2 357 17.76 -0.01 - 5.2 - 4.4
308 16.16 0.16 - 5.3 - 0.8 358 17.43 0.41 - 4.9 - 4.6
309 15.23 0.71 - 5.1 - 0.8 359 16.24 0.18 - 4.0 - 4.7
310 17.30 1.42 - 4.9 - 0.9 360 16.71 0.14 - 4.3 - 5.3
311 17.55 1.06 - 4.7 - 0.4 361 16.15 0.42 - 4.7 - 5.8
312 16.91 -1.60: - 4.5 - 0.7 362 14.34 0.44 - 4.9 - 5.7
313 13.55 0.91 - 4.3 - 1.0 363 14.60 0.46 - 5.1 - 5.2
314 17.54 0.51 - 5.0 - 1.2 364 17.70 0.56 - 5.2 - 5.1
315 15.87 0.29 - 4.5 - 1.5 365 15.63 0.42 - 5.3 - 5.3
316 17.39 0.67 - 4.9 - 1.6 366 15.20 0.62 - 5.5 - 5.3
317 16.20 0.55 - 5.0 - 1.8 367 16.56 0.41 - 5.9 - 5.2
318 16.76 0.46 - 4.9 - 2.0 368 17.62 0.50 - 6.3 - 5.1
319 17.27 1.13 - 4.9 - 2.3 369 17.55 0.90 - 6.4 - 5.4
320 17.60 1.11 - 5.3 - 2.1 370 17.12 0.22 - 6.3 - 5.6
321 14.06 -0.09 - 6.0 - 1.9 371 14.81 0.99 - 5.7 - 5.8
322 17.33 0.41 - 6.1 - 2.1 372 16.96 0.73 - 5.6 - 6.0
323 12.98 0.88 - 6.5 - 2.3 373 13.85 0.52 - 5.7 - 6.2
324 15.10 0.54 - 6.6 - 1.8 374 14.04 0.28 - 5.7 - 6.4
325 12.16 0.42 - 6.8 - 1.8 375 14.80 0.58 - 6.3 - 6.1
326 17.58 - - 6.9 - 2.5 376 17.18 1.51 - 6.4 - 6.3
327 16.50 0.30 - 7.1 - 2.3 377 17.21 1.11 - 6.9 - 5.6
328 14.39 0.21 - 7.5 - 2.4 378 16.58 0.48 - 7.4 - 5.7
329 16.93 0.46 - 7.7 - 2.9 379 17.06 0.76 - 7.6 - 5.3
330 17.48 1.37 - 7.5 - 3.2 380 15.68 0.14 - 7.6 - 5.2
331 17.53 0.67 - 7.9 - 3.7 381 16.95 0.72 - 8.0 - 5.0
332 16.31 0.82 - 7.6 - 3.8 382 15.08 0.19 - 8.3 - 5.6
333* 12.92 1.12 - 7.5 - 4.2 383 15.05 0.47 - 8.0 - 5.9
334* 15.73 0.52 - 7.6 - 4.2 384 15.69 0.77 - 8.3 - 6.4
335 16.96 0.40 - 7.5 - 4.5 385 17.34 0.45 - 8.8 - 6.6
336 16.26 0.22 - 6.6 - 3.4 386 17.59 0.94 - 8.4 - 7.0
337 17.24 0.84 - 6.3 - 3.5 387 17.49 1.47 - 8.9 - 6.9
338 17.55 - - 6.4 - 3.8 388 15.93 0.28 - 8.4 - 7.7
339 17.35 1.28 - 6.0 - 4.0 389 16.53 0.34 - 8.9 - 8.2
340 14.04 0.46 - 5.3 - 4.0 390 17.52 0.21 - 8.8 - 8.5
341 16.79 0.75 - 5.3 - 3.9 391 12.64 0.58 - 8.5 - 8.3
342 16.94 1.04 - 5.5 - 3.8 392 17.02 0.49 - 8.2 - 9.1
343 15.72 0.15 - 5.7 - 3.7 393 16.20 0.76 - 8.1 - 9.2
344 15.84 0.55 - 5.5 - 3.1 394 17.56 0.11 - 8.0 - 9.3
345 17.49 0.88 - 5.2 - 3.1 395 15.91 0.38 - 7.6 - 8.7
346 15.76 0.82 - 5.1 - 2.6 396 16.39 0.66 - 7.8 - 7.6
347 17.00 0.51 - 4.9 - 2.6 397 17.08 1.14 - 7.5 - 7.7
348 16.06 0.57 - 4.8 - 2.7 398 17.10 0.88 - 7.1 - 7.4
349 16.77 0.41 - 4.7 - 3.0 399 15.83 0.77 - 6.8 - 7.7
350 17.07 0.43 - 5.0 - 3.6 400 15.78 -0.27: - 6.7 - 7.4
Table (Cont.)
No. V B-V X Y No. V B-V X Y
401 17.68 0.93 - 6.5 - 6.8 451 17.16 0.40 0.3 -12.0
402* 17.69 0.52 - 5.9 - 7.0 452 17.82 0.58 0.9 -11.4
403 13.35 0.91 - 5.5 - 7.1 453 17.19 0.66 1.6 -11.4
404 15.56 0.41 - 6.1 - 7.6 454 16.61 0.81 1.8 -11.6
405 16.69 0.70 - 5.7 - 7.6 455 14.79 0.36 2.7 -10.8
406 16.16 0.29 - 5.5 - 7.6 456 17.54 0.24 2.4 -10.7
407 15.58 0.70 - 5.5 - 7.8 457 15.14 0.68 2.3 -11.0
408 14.67 0.47 - 5.7 - 7.9 458 11.49 0.12 1.6 -10.8
409 14.73 0.47 - 6.5 - 8.1 459 17.50 0.68 1.5 -10.5
410 16.47 0.82 - 6.8 - 8.1 460 17.62 0.28 0.3 -10.6
411 16.69 0.76 - 7.0 - 8.5 461 16.78 0.60 0.3 -10.8
412 14.47 0.65 - 6.5 - 8.5 462 16.88 -0.06 - 0.3 -11.1
413 16.06 0.75 - 6.6 - 8.6 463 15.91 0.50 - 0.6 -11.1
414 17.42 1.23 - 7.3 - 9.8 464 15.52 0.44 - 1.2 -11.1
415 16.78 0.21 - 6.9 - 9.8 465 17.03 0.94 - 1.9 -11.0
416 15.94 0.30 - 6.6 - 9.6 466 15.24 0.94 - 1.0 -10.2
417 16.02 1.54 - 5.3 - 8.6 467 16.66 0.87 - 1.3 -10.2
418 17.19 1.48 - 5.3 - 9.0 468 16.27 0.21 - 1.7 -10.4
419 17.50 0.93 - 5.3 - 9.1 469 16.31 0.78 - 2.3 -10.6
420 17.43 0.40 - 5.3 - 9.3 470 13.63 0.78 - 3.0 -10.7
421 16.39 0.85 - 5.0 - 9.3 471 17.57 0.88 - 3.0 -10.5
422 17.00 1.12 - 4.7 - 9.1 472 16.18 0.91 - 3.6 -10.4
423 16.04 0.50 - 4.4 - 9.6 473 17.51 - - 3.9 -10.4
424 17.13 0.37 - 4.7 - 9.6 474 17.57 1.13 - 4.3 -10.1
425 15.10 0.39 - 5.1 - 9.6 475 17.06 0.12 - 3.8 -10.1
426 15.10 0.43 - 5.7 - 9.7 476 14.59 0.79 - 3.1 -10.0
427 17.29 0.93 - 5.5 -10.1 477* 16.57 0.67 - 3.1 -10.1
428 16.63 0.87 - 5.2 -10.1 478 12.27 0.56 - 2.6 -10.0
429 17.49 0.78 - 4.9 -10.1 479 17.09 1.40 - 2.8 -10.0
430 14.65 0.42 - 4.6 -10.0 480 14.40 0.87 - 3.2 - 9.5
431 13.69 0.95 - 4.9 -10.3 481* 14.97 2.02 - 2.7 - 9.3
432 16.09 0.22 - 5.5 -10.2 482 16.75 0.78 - 3.1 - 9.2
433 16.87 0.46 - 5.0 -10.6 483 17.31 0.67 - 4.0 - 9.1
434 16.62 0.65 - 5.4 -10.6 484 17.25 0.16 - 3.9 - 8.4
435 16.08 0.54 - 5.4 -11.0 485 16.72 0.29 - 4.4 - 7.8
436 17.59 - - 5.5 -11.1 486 17.40 0.94 - 4.7 - 6.8
437 13.26 0.49 - 5.0 -11.2 487 17.61 0.66 - 4.0 - 6.6
438 13.62 1.02 - 3.7 -11.1 488 17.65 0.80 - 4.6 - 7.2
439 17.64 0.25 - 3.4 -11.3 489 17.11 0.94 - 4.2 - 7.2
440 17.07 0.38 - 3.4 -11.6 490 16.46 0.85 - 3.7 - 7.7
441 16.86 0.67 - 2.9 -11.7 491 11.93 0.58 - 3.6 - 7.3
442 17.88 -0.08 - 2.9 -11.3 492 17.62 0.39 - 2.8 - 7.0
443 17.85 - - 2.4 -11.3 493 17.38 0.21 - 2.5 - 7.0
444 16.22 0.63 - 2.2 -11.3 494 15.49 0.58 - 3.2 - 7.6
445 14.49 0.64 - 2.0 -11.6 495 13.12 0.48 - 2.6 - 8.0
446 16.69 0.43 - 2.3 -12.0 496 16.88 0.72 - 2.5 - 8.1
447 16.53 0.87 - 1.4 -11.9 497 14.05 0.59 - 2.3 - 8.3
448 15.52 0.18 - 1.3 -11.3 498 17.46 0.20 - 2.8 - 8.5
449 17.04 0.30 - 0.9 -11.4 499 15.58 0.33 - 2.9 - 8.7
450 17.66 0.50 - 0.2 -11.2 500 11.95: -1.25: - 2.4 - 8.7
Table (Cont.)
No. V B-V X Y No. V B-V X Y
501 16.41 0.95 - 2.1 - 8.6 551 14.07 1.16 - 1.4 - 8.4
502 17.65 0.36 - 1.9 - 8.4 552 13.55 1.23 - 1.6 - 8.0
503 14.15 0.55 - 2.0 - 8.6 553 17.47 0.92 - 1.3 - 8.0
504 16.41 0.30 - 1.8 - 8.9 554 17.49 0.87 - 0.9 - 8.1
505 17.43 0.80 - 2.0 - 8.9 555 15.48 0.79 - 0.9 - 7.7
506 16.38 0.89 - 2.2 - 9.0 556 16.82 0.55 - 1.0 - 7.6
507 17.36 - - 1.8 - 9.2 557 15.29 0.42 - 1.0 - 7.4
508 14.76 - - 1.6 - 9.4 558 15.82 0.37 - 0.3 - 7.7
509 17.23 0.05 - 1.3 - 9.6 559 16.30 0.84 - 0.3 - 7.2
510 17.57 - - 1.5 - 9.8 560 13.16 0.94 - 0.1 - 7.1
511 13.85 0.97 - 0.8 - 9.7 561 17.49 - 0.1 - 6.9
512 15.29 0.61 - 1.3 - 9.3 562 15.95 0.56 0.0 - 6.7
513 14.64 0.78 - 1.0 - 9.1 563 17.71 0.62 0.5 - 6.5
514 17.33 0.45 - 0.7 - 8.9 564 14.44 0.75 0.9 - 6.3
515 17.45 0.82 - 0.2 - 9.8 565 17.25 1.13 1.2 - 6.3
516 15.38 0.13 - 0.1 - 9.6 566 16.95 0.59 2.0 - 6.3
517 17.07 0.39 - 0.2 - 9.3 567 14.07 0.94 2.5 - 6.4
518 14.84 0.43 - 0.2 - 9.0 568 16.46 0.49 2.9 - 6.9
519 15.05 0.39 0.0 - 8.7 569 14.52 0.49 3.1 - 6.5
520 17.56 0.76 0.0 -10.0 570 16.90 0.37 2.9 - 6.3
521 17.79 - 0.3 - 9.1 571 14.94 0.53 3.0 - 5.8
522 14.60 0.45 0.5 - 8.9 572 17.71 - 2.8 - 5.8
523 13.13 0.45 1.2 - 8.6 573 16.58 0.51 3.1 - 5.4
524 16.62 0.95 1.6 - 9.0 574 16.75 0.54 3.1 - 5.3
525 17.08 0.49 0.8 - 9.4 575 15.96 0.52 2.4 - 5.4
526 15.99 0.62 0.7 - 9.6 576 16.85 0.70 2.3 - 5.2
527 16.73 0.78 0.5 - 9.8 577 14.63 0.36 1.9 - 4.7
528 17.04 -0.02 0.5 -10.0 578 16.18 0.56 1.7 - 4.6
529 15.47 0.37 0.8 -10.1 579 16.93 0.32 1.7 - 5.0
530 17.13 0.66 1.3 - 9.8 580 17.27 0.34 1.9 - 5.1
531* 11.70 0.93 2.0 - 9.7 581 16.74 0.83 1.9 - 5.2
532 16.86 0.82 2.1 - 9.6 582 17.33 0.51 1.7 - 5.3
533 17.51 0.57 2.2 -10.0 583 12.60 0.65 1.8 - 5.8
534 17.17 0.81 2.9 -10.0 584 17.45 1.06 2.2 - 6.1
535 16.38 0.79 2.5 - 9.5 585 13.60 0.45 1.5 - 6.0
536 13.83 0.94 2.7 - 8.8 586 17.76 0.54 1.4 - 5.7
537 16.63 0.36 2.1 - 8.6 587 14.95 0.39 1.2 - 5.6
538 16.59 0.89 2.5 - 8.1 588 17.15 0.35 1.2 - 5.3
539 16.53 0.24 2.2 - 8.0 589 16.19 0.54 1.1 - 5.2
540 17.56 1.19 1.9 - 8.3 590 15.17 1.28 0.8 - 5.1
541 14.07 0.76 2.2 - 7.4 591 17.75 0.72 1.0 - 4.9
542 13.53 0.38 2.4 - 7.1 592 17.31 0.72 1.1 - 4.8
543 17.50 0.20 2.0 - 7.2 593 15.84 0.33 1.1 - 4.6
544 16.71 1.17 1.6 - 7.6 594 17.36 0.54 0.8 - 4.4
545 17.40 0.05 0.9 - 7.9 595 17.57 0.47 0.5 - 5.0
546 15.43 0.41 0.5 - 7.5 596 16.65 0.95 0.2 - 5.3
547 12.84 0.82 0.2 - 7.7 597 17.46 0.75 0.0 - 6.3
548 16.83 0.83 - 0.4 - 8.3 598 16.88 0.79 - 0.6 - 6.8
549 17.39 0.51 - 0.5 - 8.2 599 17.02 0.73 - 1.2 - 6.5
550 17.38 1.37 - 1.4 - 8.5 600 14.42 0.66 - 1.0 - 6.3
Table (Cont.)
No. V B-V X Y No. V B-V X Y
601 13.01 0.78 - 0.8 - 6.2 651 17.50 - - 3.9 - 4.0
602 16.54 0.19 - 0.7 - 6.0 652 17.23 0.68 - 4.3 - 3.6
603 16.92 0.78 - 0.7 - 5.8 653 16.31 0.84 - 3.5 - 3.5
604 17.56 1.17 - 0.5 - 5.3 654 16.62 0.10 - 3.8 - 3.3
605 17.60 - - 0.2 - 5.1 655 17.52 - - 4.0 - 3.3
606 13.10 0.88 0.1 - 4.8 656 15.87 0.74 - 3.7 - 3.0
607 12.07 0.52 - 0.2 - 4.9 657 17.75 0.79 - 4.6 - 2.5
608 - - - - 658 17.47 0.87 - 4.4 - 2.5
609 14.59 0.22 - 0.5 - 4.7 659 17.37 0.98 - 4.1 - 2.0
610 16.81 1.48 - 0.5 - 4.6 660 17.25 0.78 - 4.0 - 1.9
611 17.42 1.15 0.2 - 4.1 661 17.48 1.09 - 3.6 - 2.4
612 16.45 0.50 0.2 - 4.0 662 15.50 0.74 - 3.1 - 2.9
613 15.05 0.58 0.1 - 3.9 663 17.46 1.02 - 2.7 - 3.0
614 14.62 0.63 - 0.4 - 4.0 664 15.02 0.71 - 2.7 - 3.2
615 13.63 1.04 - 0.9 - 4.0 665 16.97 0.52 - 2.3 - 3.6
616 15.66 0.54 - 1.3 - 4.2 666 15.22 0.39 - 2.0 - 3.6
617 17.60 0.45 - 0.7 - 4.3 667 17.47 0.86 - 1.5 - 3.2
618 15.17 0.70 - 0.9 - 4.4 668 17.40 0.71 - 1.3 - 3.3
619 17.19 0.49 - 1.6 - 4.4 669 15.24 0.02 - 1.2 - 3.6
620 17.37 0.30 - 2.0 - 4.8 670 15.34 0.25 - 1.1 - 3.6
621 16.73 0.89 - 1.9 - 4.7 671 17.20 1.23 - 1.0 - 3.4
622 15.98 0.58 - 1.6 - 4.7 672 14.61 0.45 - 0.9 - 3.6
623 14.98 0.75 - 1.2 - 5.1 673 17.09 0.38 - 0.4 - 3.3
624 11.80 0.90 - 1.2 - 5.5 674 16.13 0.33 - 0.5 - 3.2
625 15.07 0.37 - 1.5 - 6.1 675 17.14 0.42 - 0.2 - 3.3
626 15.87 0.46 - 1.7 - 6.3 676 17.11 0.58 0.0 - 3.2
627 13.57 1.00 - 1.7 - 5.5 677 14.99 0.05 - 0.1 - 3.4
628 17.47 -0.05 - 1.6 - 5.1 678 16.63 0.73 0.0 - 3.6
629 16.61 0.41 - 1.8 - 5.3 679 17.17 1.27 0.2 - 3.6
630 16.88 0.74 - 2.0 - 5.2 680 17.49 0.85 0.9 - 3.8
631 15.70 0.40 - 2.2 - 5.1 681 14.45 0.71 1.5 - 3.9
632 15.71 0.57 - 2.3 - 5.3 682 17.50 1.21 1.7 - 4.1
633 15.83 0.67 - 2.4 - 5.9 683 11.35 0.56 2.1 - 4.1
634 16.73 1.03 - 2.6 - 6.2 684 17.44 0.62 2.0 - 4.3
635 17.54 0.37 - 3.0 - 6.1 685 16.46 0.47 2.8 - 3.9
636 17.47 0.52 - 3.3 - 6.0 686 15.41 0.92 2.9 - 4.4
637 17.09 1.04 - 3.3 - 5.5 687 17.26 1.15 3.1 - 4.4
638 15.05 0.51 - 2.6 - 5.8 688 16.77 0.16 3.2 - 4.2
639 16.74 0.44 - 2.8 - 5.5 689 17.03 0.56 3.0 - 3.5
640 15.79 0.59 - 2.8 - 5.1 690 14.44 0.20 3.2 - 3.3
641 16.92 0.31 - 2.7 - 4.7 691 13.39 0.57 3.1 - 3.2
642 17.50 0.43 - 2.7 - 4.5 692 16.49 0.44 2.1 - 3.4
643 16.06 0.23 - 2.0 - 4.1 693 17.66 1.22 2.1 - 3.1
644 16.50 0.54 - 2.0 - 4.1 694 17.38 1.16 2.4 - 3.1
645 16.08 1.23 - 2.5 - 4.1 695 17.53 0.68 2.4 - 2.8
646 17.31 0.38 - 3.1 - 4.1 696 15.46 0.36 2.7 - 2.6
647 15.72 1.13 - 3.1 - 4.6 697 17.75 0.44 3.0 - 2.5
648 16.28 0.83 - 3.1 - 4.7 698 16.22 0.42 2.5 - 2.3
649 17.19 0.57 - 3.1 - 4.8 699 17.43 0.56 2.4 - 2.2
650 15.36 0.63 - 3.6 - 4.2 700* 13.84 1.09 2.5 - 2.0
Table (Cont.)
No. V B-V X Y No. V B-V X Y
701* 15.83 1.46 2.6 - 2.1 751 16.67 0.37 - 3.0 - 1.5
702* 16.89 0.32 2.3 - 1.8 752 12.37 0.48 - 2.5 - 1.8
703 14.45 0.64 1.8 - 1.5 753 11.27 1.36 - 2.2 - 1.5
704 14.43 1.39 1.7 - 1.7 754 17.35 1.42 - 1.9 - 1.8
705 16.42 0.40 2.0 - 1.9 755 17.13 1.33 - 1.8 - 1.8
706 15.18 0.32 2.0 - 2.1 756* 15.17 0.90 - 1.9 - 1.2
707 14.55 0.48 2.0 - 2.2 757 17.08 0.85 - 1.9 - 1.0
708 14.67 0.53 1.6 - 2.6 758 17.35 1.08 - 2.9 - 1.0
709* 14.07 0.17 1.7 - 3.1 759 17.37 1.31 - 3.1 - 1.1
710* 15.12 0.73 1.5 - 3.1 760 15.32 1.56 - 3.3 - 0.9
711* 12.97 1.46 0.5 - 3.1 761 17.03 1.27 - 3.4 - 1.1
712* 14.82 0.67 0.4 - 3.1 762 16.85 0.84 - 3.9 - 1.0
713 15.13 0.57 0.8 - 2.9 763 16.80 0.45 - 3.5 - 0.6
714 16.71 0.70 0.9 - 2.9 764 17.48 0.74 - 3.5 - 0.4
715 17.29 1.15 0.5 - 2.8 765 16.70 0.50 - 3.4 - 0.4
716 14.77 0.33 0.5 - 2.5 766 17.27 0.79 - 3.3 - 0.5
717 13.47 0.45 0.3 - 2.3 767 17.59 1.23 - 2.7 - 0.3
718 15.94 0.46 0.6 - 2.0 768 16.38 0.92 - 3.2 - 0.1
719 16.92 0.42 1.0 - 2.0 769 16.93 0.66 - 3.6 - 0.1
720 16.40 0.63 1.3 - 1.9 770 16.67 0.56 - 3.9 - 0.1
721 16.58 0.52 0.5 - 1.7 771 17.42 0.85 - 4.2 - 0.4
722 15.02 0.41 - 0.3 - 2.0 772 17.28 0.92 - 4.2 - 0.2
723 15.17 0.40 - 0.5 - 1.9 773 17.06 0.96 - 4.4 - 0.1
724 15.87 0.84 - 0.6 - 2.1 774* 15.43 0.70 - 4.7 0.1
725 16.90 0.93 - 0.5 - 2.4 775 17.75 1.38 - 5.0 0.2
726 14.74 0.70 - 0.2 - 2.7 776 16.41 0.56 - 4.9 0.7
727 12.36 0.85 - 0.3 - 2.7 777* 15.52 0.56 - 4.9 0.9
728 11.05 0.90 - 0.6 - 2.7 778 16.42 1.19 - 4.9 1.1
729 13.77 0.49 - 1.1 - 3.0 779 14.53 0.54 - 5.0 1.5
730 17.29 0.20 - 1.4 - 2.9 780 15.82 1.24 - 4.9 1.4
731 14.69 0.85 - 1.5 - 2.7 781 15.74 0.65 - 4.8 1.3
732 17.01 1.24 - 1.5 - 2.5 782 15.89 -0.62: - 4.7 1.0
733 15.03 0.43 - 1.2 - 2.5 783 17.43 1.29 - 4.4 0.8
734 17.58 1.28 - 0.9 - 2.6 784 16.01 0.91 - 4.5 0.6
735 17.38 1.08 - 0.8 - 2.2 785 17.07 0.61 - 4.6 0.4
736 15.96 0.28 - 0.8 - 1.8 786 17.08 0.90 - 4.3 0.2
737* 15.24 0.22 - 1.1 - 1.8 787 15.60 1.03 - 4.2 0.2
738* 12.93 0.84 - 1.1 - 1.8 788 16.19 0.60 - 3.8 0.1
739 14.42 1.26 - 1.3 - 1.7 789 17.53 0.37 - 3.6 0.9
740 16.17 0.84 - 1.7 - 2.2 790* 14.66 0.18 - 3.5 0.7
741* 16.35 0.89 - 1.9 - 2.2 791 17.23 0.87 - 3.5 0.4
742 15.36 0.31 - 2.1 - 2.3 792 15.84 0.42 - 3.2 0.4
743 17.21 0.19 - 2.0 - 2.9 793 16.87 0.63 - 2.7 0.2
744 17.02 1.14 - 2.1 - 2.9 794 15.93 0.58 - 2.6 0.4
745 14.84 0.54 - 2.6 - 2.2 795 17.02 1.20 - 2.5 0.4
746 14.92 0.84 - 2.8 - 2.3 796 16.81 0.07 - 2.6 0.6
747 14.46 0.43 - 2.8 - 2.1 797 16.71 0.31 - 2.8 0.7
748 16.10 1.28 - 3.0 - 1.9 798 16.64 0.43 - 2.9 0.9
749 17.28 0.64 - 3.3 - 1.7 799 17.31 1.44 - 2.9 1.0
750* 14.31 1.20 - 3.2 - 1.6 800 16.36 0.74 - 2.6 1.0
Table (Cont.)
No. V B-V X Y No. V B-V X Y
801 16.43 0.86 - 2.9 1.1 851 17.43 0.99 - 4.5 4.9
802 16.89 0.60 - 3.1 1.0 852 16.98 0.73 - 4.8 5.0
803 16.23 0.53 - 3.3 1.0 853 13.59 0.56 - 4.9 5.8
804 15.02 0.39 - 3.3 1.2 854 17.54 1.43 - 4.7 5.6
805 17.05 0.48 - 3.5 1.2 855 17.32 0.61 - 4.6 5.8
806 17.10 0.56 - 4.1 1.0 856 17.46 0.79 - 3.7 6.0
807 16.39 1.09 - 4.2 1.3 857 15.91 0.35 - 3.6 6.0
808 16.88 1.12 - 4.4 1.4 858 16.02 0.41 - 3.1 5.6
809 16.74 0.69 - 4.1 1.8 859 16.56 0.92 - 3.1 5.5
810 16.76 0.77 - 3.3 1.8 860 17.25 1.40 - 2.5 5.3
811 16.67 0.52 - 2.9 1.4 861 17.20 0.78 - 2.9 5.8
812 16.46 0.37 - 2.7 1.4 862 17.59 1.02 - 3.0 6.2
813 16.92 0.61 - 2.9 2.5 863 17.60 0.99 - 2.9 6.2
814 17.26 0.81 - 3.2 2.3 864 14.73 0.60 - 2.6 6.7
815 17.00 1.06 - 3.8 2.1 865 12.21 0.54 - 2.7 6.8
816 17.58 0.53 - 3.8 2.3 866 14.39 0.36 - 3.5 6.9
817 16.80 0.69 - 3.9 2.2 867 14.44 0.48 - 3.2 6.6
818 17.37 - - 4.1 2.3 868 16.28 0.59 - 3.0 6.5
819 14.42 0.51 - 4.6 2.4 869 15.70 0.54 - 3.1 6.4
820 17.01 0.26 - 3.9 2.6 870 12.30 0.99 - 3.3 6.4
821 17.22 0.41 - 3.6 2.9 871 17.53 0.98 - 3.4 6.3
822 17.28 1.69 - 3.9 3.0 872 15.33 0.24 - 3.6 6.6
823 17.41 0.61 - 4.2 2.8 873 16.73 0.08 - 4.0 6.5
824 16.19 0.44 - 4.5 2.9 874 15.64 1.90 - 4.3 6.4
825 17.62 0.91 - 4.6 3.2 875 16.98 0.65 - 4.3 6.7
826 16.52 0.45 - 4.3 3.0 876 17.28 1.12 - 3.9 7.0
827 15.63 1.52 - 4.0 3.2 877 17.39 0.06 - 4.5 7.1
828 16.65 1.19 - 2.7 3.1 878 15.71 0.38 - 5.4 7.3
829 11.85 1.04 - 2.3 3.3 879 17.10 0.40 - 5.3 7.3
830 17.50 0.85 - 2.4 3.5 880 15.03 1.01 - 4.7 7.3
831 17.66 0.66 - 2.5 3.6 881 17.01 0.88 - 4.1 7.4
832 15.85 1.02 - 2.7 3.9 882 12.78 0.63 - 3.6 7.7
833 17.59 - - 2.5 4.0 883 14.62 0.93 - 3.4 7.4
834 15.24 0.64 - 2.9 4.0 884 17.34 1.61 - 3.1 7.7
835 17.04 1.21 - 2.9 4.1 885 16.75 1.70 - 3.1 7.5
836 12.89 0.84 - 3.1 4.1 886 16.74 0.43 - 2.8 7.4
837 15.04 0.32 - 4.0 3.9 887 16.88 0.57 - 2.5 7.9
838 16.08 0.43 - 4.5 4.1 888 16.71 1.32 - 2.8 7.9
839 14.98 0.35 - 5.0 3.9 889 15.21 0.46 - 2.8 8.3
840 17.31 -0.12: - 5.1 3.9 890 13.78 1.16 - 2.8 8.9
841 17.10 0.55 - 4.2 4.5 891 17.45 - - 2.6 9.1
842 15.81 0.52 - 3.9 4.7 892 17.22 0.87 - 2.2 9.4
843 11.59 0.45 - 3.6 4.7 893 17.63 1.35 - 2.0 9.7
844 17.36 0.04 - 3.3 4.7 894 13.25 0.89 - 2.3 9.5
845 16.70 0.74 - 3.5 5.0 895 17.18 1.07 - 2.8 9.3
846 13.66 0.40 - 3.6 5.2 896 16.83 0.87 - 3.1 9.2
847 17.42 1.22 - 3.8 5.4 897 14.38 0.45 - 3.4 9.1
848 16.19 0.66 - 3.9 5.1 898 17.36 1.94 - 3.3 9.0
849 14.60 0.17 - 4.1 4.9 899 17.56 1.70 - 3.4 8.8
850 17.65 0.33 - 4.3 5.0 900 17.35 0.88 - 3.5 8.5
Table (Cont.)
No. V B-V X Y No. V B-V X Y
901 17.29 0.44 - 3.7 8.3 951 16.72 0.51 - 4.5 11.4
902* 14.85 0.62 - 4.0 7.9 952 15.87 1.01 - 4.6 11.2
903* 14.43 0.74 - 4.1 7.9 953 17.13 1.75 - 4.6 11.1
904* 12.55 0.45 - 4.2 7.8 954 17.47 - - 3.0 11.4
905 17.44 2.03 - 4.6 7.7 955 16.00 0.69 - 3.0 11.3
906 15.76 0.60 - 4.5 8.2 956 17.13 0.39 - 2.9 11.0
907 17.47 0.96 - 3.9 8.4 957 17.66 - - 2.5 10.4
908 17.41 1.35 - 3.9 8.7 958 17.61 - - 2.3 10.4
909 17.36 0.82 - 4.1 8.8 959 17.30 0.77 - 2.0 10.4
910 16.46 0.78 - 4.1 9.3 960 17.24 - - 1.7 10.5
911 13.92 0.45 - 3.9 9.3 961 17.38 - - 1.5 10.7
912 17.43 - - 3.7 9.7 962 17.41 0.84 - 2.3 11.6
913 16.24 0.81 - 3.3 10.5 963 16.49 0.61 - 2.6 12.3
914 17.58 1.34 - 3.7 10.9 964 17.50 1.05 - 2.4 12.4
915 17.38 0.60 - 4.5 10.4 965 15.27 0.79 - 2.2 11.9
916 17.13 - - 4.3 10.4 966 16.25 1.41 - 1.8 11.7
917 14.73 0.53 - 4.5 10.6 967 17.24 0.82 - 1.8 11.9
918 17.43 0.81 - 4.7 10.3 968 17.49 1.31 - 1.7 12.1
919 17.47 1.69 - 4.8 9.8 969 17.67 - - 1.8 12.3
920 17.36 0.56 - 4.9 9.6 970 16.48 0.42 3.2 - 1.8
921 16.39 0.72 - 4.7 9.4 971 16.81 0.63 3.0 - 1.6
922 15.96 0.61 - 4.8 9.1 972* 16.69 0.31 2.6 - 1.7
923 15.67 1.12 - 4.9 8.9 973* 17.19 0.60 2.6 - 1.6
924 15.33 0.39 - 5.4 8.3 974* 15.50 0.60 2.5 - 1.4
925 16.71 0.31 - 5.7 8.4 975 17.49 0.91 3.6 - 1.6
926 17.11 0.41 - 5.9 8.5 976 14.36 0.66 3.5 - 1.3
927 17.13 1.33 - 5.6 9.1 977 17.14 0.77 3.2 - 1.2
928 17.46 1.17 - 6.2 9.0 978 15.77 0.46 3.2 - 1.1
929 17.55 1.16 - 6.3 9.6 979 17.46 0.45 3.0 - 0.8
930* 14.02 -0.11 - 6.0 9.8 980 17.16 0.27 3.2 - 0.6
931* 12.60 0.17 - 5.9 9.7 981 15.20 0.43 3.2 - 0.6
932 16.82 0.40 - 5.5 9.9 982 15.40 0.87 2.8 - 0.7
933 17.22 1.16 - 5.3 10.0 983 17.03 0.69 2.5 - 0.7
934 14.94 0.75 - 5.4 10.0 984 16.20 0.35 2.0 - 1.0
935 14.45 0.81 - 5.9 10.3 985 17.60 0.61 1.8 - 0.9
936 17.41 1.71 - 6.3 10.9 986 17.60 0.70 1.8 - 0.7
937 17.70 0.36 - 6.3 11.0 987 16.77 1.43 1.7 - 0.4
938 16.99 0.47 - 6.0 10.9 988 15.99 1.08 2.2 - 0.6
939 15.92 0.79 - 5.9 10.9 989 14.36 0.81 2.2 - 0.4
940 17.00 1.08 - 5.6 10.7 990 14.71 0.51 2.4 - 0.3
941 17.68 0.45 - 5.2 10.4 991 15.86 0.59 2.3 - 0.2
942 16.39 1.32 - 5.3 10.7 992 15.39 0.54 1.9 0.5
943 17.10 -0.01 - 5.2 11.0 993 17.55 0.73 1.7 0.5
944 13.55 0.38 - 5.2 11.2 994 17.52 0.75 1.6 0.8
945 17.49 1.23 - 5.6 11.3 995 15.66 0.30 1.6 1.0
946 17.48 0.97 - 4.1 12.1 996 16.39 0.15 1.7 1.1
947 15.27 1.14 - 4.0 12.1 997 15.46 0.40 1.9 1.1
948 17.26 1.41 - 4.0 11.9 998 15.18 0.50 2.2 1.3
949 14.56 0.41 - 4.0 11.8 999 16.58 0.34 2.3 1.2
950 15.02 0.88 - 4.3 11.6 1000 17.45 - 2.2 0.9
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1001 16.97 1.20 2.8 1.2 1051 16.01 0.67 - 0.5 2.3
1002 14.52 0.39 2.8 1.0 1052 16.01 0.32 - 0.7 2.5
1003 17.47 1.25 2.8 0.9 1053 15.41 0.64 - 0.5 2.5
1004 17.12 0.68 3.0 0.8 1054* 12.09 1.05 - 0.3 2.5
1005 14.91 0.62 2.9 0.7 1055* 17.30 1.31 - 0.2 2.7
1006 17.27 - 2.6 0.5 1056* 17.58 - - 0.1 2.8
1007 13.97 0.72 2.4 0.2 1057 17.30 0.96 - 0.3 2.8
1008* 14.51 1.06 3.0 0.2 1058 17.12 0.89 - 0.4 3.0
1009 17.55 0.29 3.3 0.5 1059 16.20 1.02 - 0.5 2.9
1010* 14.07 0.90 3.4 0.5 1060 17.36 0.69 - 0.4 2.8
1011 15.52 0.97 3.6 0.4 1061 17.51 0.40 - 0.5 2.7
1012 15.36 0.48 3.7 0.5 1062 17.59 1.12 - 0.7 2.8
1013 15.88 0.92 3.7 0.9 1063 15.27 0.23 - 0.8 2.8
1014 11.60 0.35 3.2 0.9 1064* 14.74 0.68 - 1.1 2.8
1015 16.15 0.64 3.1 1.2 1065 15.04 0.45 - 1.2 3.0
1016 17.72 - 3.0 1.3 1066 16.51 0.70 - 1.1 3.1
1017 16.69 1.03 3.4 1.4 1067 17.27 0.55 - 1.2 3.2
1018 16.92 0.30 2.9 1.9 1068 16.20 0.55 - 1.9 2.9
1019 17.22 0.82 2.8 1.5 1069 17.28 0.86 - 1.9 3.0
1020 16.79 0.47 2.6 1.7 1070 15.42 0.39 - 1.5 3.5
1021 14.60 0.42 2.4 1.9 1071 16.81 0.41 - 1.1 3.5
1022 16.68 0.10 2.2 2.0 1072 17.38 0.87 - 0.8 3.3
1023 15.77 0.26 2.2 1.9 1073 16.96 0.34 - 0.8 3.5
1024 14.83 0.50 2.2 1.8 1074 13.92 1.02 - 0.5 3.8
1025* 13.04 0.47 2.3 1.6 1075 15.25 0.76 - 0.2 3.7
1026* 12.26 0.87 2.2 1.7 1076 16.64 0.61 - 0.2 3.5
1027 16.20 0.27 2.1 1.6 1077 16.17 0.51 0.3 3.6
1028 17.30 0.45 2.0 1.5 1078 17.51 0.81 1.1 4.2
1029 15.65 0.33 1.8 1.6 1079 14.49 0.95 1.1 4.6
1030 17.36 0.74 2.0 1.8 1080 17.55 - 0.7 4.7
1031 17.17 -0.29: 1.8 2.2 1081 16.22 0.47 0.7 4.4
1032 14.61 0.99 1.7 2.1 1082 17.00 0.94 0.5 4.3
1033 16.94 0.47 1.4 2.1 1083 16.02 0.15 0.8 4.1
1034* 15.67 0.40 1.1 2.0 1084 16.04 0.42 0.5 4.1
1035 13.12 0.44 1.0 1.9 1085 16.55 0.30 0.1 4.1
1036 15.18 0.74 0.7 2.1 1086 17.36 0.99 0.0 4.3
1037 16.70 0.58 0.8 2.4 1087 16.73 0.63 - 0.1 4.2
1038 16.44 0.61 0.7 2.5 1088 14.07 1.03 - 0.4 4.3
1039 12.62 0.96 1.1 2.2 1089 15.99 0.83 - 0.7 4.2
1040 15.51 0.46 1.3 2.3 1090 13.35 0.73 - 0.8 4.6
1041 17.39 0.77 1.7 2.5 1091 16.79 0.46 - 1.1 4.4
1042 14.52 0.49 1.4 2.7 1092 16.26 0.31 - 1.1 4.1
1043 16.88 0.90 0.9 2.8 1093 17.07 0.25 - 1.4 4.1
1044 16.29 0.36 0.7 2.8 1094 16.91 0.46 - 1.6 4.1
1045 15.43 0.35 0.5 2.7 1095 16.87 0.76 - 1.6 4.4
1046 17.49 0.91 0.3 3.0 1096 17.60 - - 1.4 4.6
1047 17.34 0.52 - 0.4 2.0 1097 15.85 0.24 - 2.2 4.5
1048 15.63 0.49 - 0.4 2.1 1098 17.60 0.96 - 2.5 4.4
1049 17.33 0.38 - 0.8 2.0 1099 14.72 0.70 - 2.3 4.7
1050 15.19 0.44 - 0.7 2.1 1100 17.74 - - 2.3 5.0
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1101 15.90 0.64 - 2.1 4.6 1151 16.96 0.40 - 0.2 7.5
1102 13.54 0.34 - 1.1 4.9 1152 17.37 0.91 0.4 7.3
1103 14.82 0.50 - 0.1 4.7 1153 17.39 0.68 1.0 7.1
1104 15.78 1.09 0.1 4.8 1154 17.33 0.17 1.4 7.4
1105 17.60 0.65 0.1 4.9 1155 16.69 0.85 1.7 7.4
1106 16.31 0.90 0.2 5.0 1156 16.46 0.97 1.6 7.6
1107 17.66 - 0.1 5.3 1157 15.24 0.33 1.5 8.2
1108 17.41 0.30 0.2 5.5 1158 17.53 1.08 1.1 8.6
1109 17.45 0.55 0.2 5.7 1159 17.44 - 1.0 8.4
1110 17.35 1.11 0.1 5.7 1160 17.08 0.81 1.0 8.2
1111 16.37 0.35 0.0 5.5 1161 17.50 - 0.9 8.2
1112 14.64 0.40 - 0.2 5.5 1162 17.88 0.31 0.6 8.5
1113 15.23 0.58 - 0.6 5.0 1163 17.53 0.66 0.9 8.8
1114 16.33 1.27 - 1.1 5.2 1164 16.97 1.21 0.8 9.1
1115 17.14 0.73 - 1.2 5.3 1165 16.98 0.59 0.4 9.1
1116 17.55 0.94 - 1.8 5.5 1166 15.90 1.01 0.3 8.9
1117 17.47 - - 2.1 6.3 1167 16.21 0.89 0.0 8.9
1118 17.60 0.27 - 2.1 6.2 1168 16.19 0.37 0.1 9.1
1119 16.74 0.57 - 1.8 6.0 1169 17.34 1.22 0.2 9.0
1120 17.35 1.32 - 1.6 6.0 1170 17.68 - 0.2 9.3
1121 16.84 0.96 - 1.4 5.8 1171 14.43 0.44 0.3 9.5
1122 16.50 0.65 - 1.3 5.7 1172 16.19 0.68 - 0.7 9.4
1123 15.93 0.72 - 1.1 5.7 1173 16.81 0.57 - 0.2 9.5
1124 17.10 - - 0.9 5.9 1174 16.56 0.54 - 0.1 9.8
1125 16.55 0.48 - 0.4 5.9 1175 16.79 1.12 0.6 9.8
1126 17.65 0.71 - 0.1 6.2 1176 16.83 0.76 0.8 9.8
1127* 14.12 0.58 0.6 6.6 1177 17.24 - 1.1 9.6
1128 14.95: 3.07: 0.6 6.7 1178 17.33 1.28 1.0 10.0
1129 17.62 0.72 0.2 6.7 1179 16.58 0.87 1.4 10.2
1130 13.19 1.59 0.2 6.6 1180 14.34 0.76 1.3 10.3
1131 15.52 1.72 - 0.4 6.5 1181 16.31 0.62 1.1 10.4
1132 17.69 0.68 - 1.0 6.7 1182 17.50 - 0.9 10.7
1133 17.31 0.56 - 0.8 6.9 1183 17.36 0.93 1.2 11.2
1134 16.30 1.37 - 0.7 7.0 1184 16.59 0.37 1.2 11.3
1135 15.31 0.43 - 0.9 7.0 1185 17.47 0.92 0.6 11.2
1136 17.59 0.63 - 1.1 7.2 1186 17.45 0.79 0.4 10.9
1137 15.28 0.70 - 1.1 7.3 1187 16.92 1.69 0.5 11.9
1138 16.85 1.65 - 1.3 7.4 1188 16.30 0.71 0.2 11.8
1139 14.82 0.40 - 1.7 6.9 1189 16.60 0.69 - 0.1 11.4
1140 15.16 0.65 - 1.8 7.2 1190 17.61 - 0.0 11.2
1141 17.52 0.47 - 1.7 7.3 1191 16.85 1.83 0.1 11.1
1142 16.14 0.37 - 1.8 7.9 1192 17.19 1.02 0.2 10.6
1143 15.56 0.72 - 1.5 8.4 1193 17.47 1.10 0.2 10.7
1144 16.31 1.73 - 1.3 8.7 1194 15.86 0.67 0.1 10.4
1145* 17.14 1.00 - 1.1 8.7 1195 16.04 0.17 - 0.7 10.5
1146* 17.51 1.19 - 1.1 8.8 1196 14.66 0.96 - 0.8 10.5
1147 17.27 1.59 - 0.9 8.4 1197 17.33 1.02 - 0.8 10.8
1148 17.19 0.60 - 0.3 8.4 1198 16.42 0.52 - 1.1 11.0
1149* 16.38 1.81 0.0 7.8 1199 14.67 0.13 - 0.9 11.8
1150* 16.00 1.04 0.0 7.7 1200 16.25 0.45 - 1.2 12.7
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1201 17.60 0.73 - 0.8 12.9 1251 15.98 1.31 3.5 8.8
1202 17.43 1.14 - 0.3 12.7 1252 15.86 0.50 3.7 8.7
1203 14.72 0.72 - 0.2 12.2 1253 17.29 - 3.5 8.6
1204 16.26 0.39 0.1 12.4 1254 14.85 0.70 3.8 8.3
1205 15.62 1.67 0.6 12.6 1255 17.50 - 3.8 8.0
1206 15.80 0.77 2.3 12.4 1256 16.27 0.72 4.7 8.3
1207 15.16 1.09 2.8 12.1 1257 17.47 0.85 4.7 8.1
1208 17.45 0.95 3.9 12.2 1258 16.81 0.78 4.8 7.9
1209 16.14 0.74 4.2 11.9 1259 16.17 0.57 4.5 7.9
1210 15.46 0.66 4.4 11.3 1260 15.25 0.98 4.2 7.7
1211 14.35 0.70 4.7 11.0 1261 15.67 0.36 4.5 7.4
1212 16.43 0.44 4.8 10.8 1262 15.83 0.68 4.5 7.2
1213 17.35 0.77 4.7 10.6 1263 16.37 0.56 4.5 7.0
1214 16.61 0.43 4.4 11.0 1264 17.18 0.09 4.6 6.8
1215 16.86 0.03 4.0 11.3 1265 14.88 0.74 4.2 6.4
1216 15.06 0.74 3.0 11.5 1266 45.75 0.73 3.0 6.3
1217 17.11 0.74 2.5 11.5 1267 17.33 - 3.2 6.4
1218 16.78 0.40 2.0 11.5 1268 15.35 0.53 3.2 6.5
1219 17.39 0.62 1.8 11.5 1269 17.26 0.67 3.6 7.1
1220 15.64 0.53 1.5 11.9 1270 16.36 0.95 3.6 7.4
1221 17.47 1.37 1.7 10.6 1271 15.63 0.39 3.3 7.8
1222 17.56 - 1.9 10.8 1272 14.30 0.63 3.1 8.0
1223 15.30 0.98 2.2 10.7 1273 16.35 1.31 2.9 8.3
1224 17.58 - 2.2 11.1 1274 17.51 0.80 2.6 8.6
1225 17.05 0.36 2.4 11.0 1275 11.06 1.32 2.5 8.3
1226 16.71 1.71 2.9 10.8 1276 16.42 1.15 2.6 7.9
1227 17.20 1.66 2.6 10.5 1277 14.48 0.47 2.2 7.6
1228 16.09 0.71 3.2 10.1 1278* 12.42 1.03 2.9 7.7
1229 15.83 0.63 4.2 9.8 1279* 17.14 0.78 3.0 7.7
1230 15.92 1.06 4.0 10.0 1280 17.53 - 3.1 7.3
1231 13.30 0.39 4.2 10.1 1281 17.51 1.32 2.8 7.1
1232 15.88 0.41 4.6 10.0 1282 17.49 0.39 2.7 7.0
1233 14.94 1.09 4.9 10.0 1283 16.48 0.92 2.7 6.8
1234 11.96 1.01 5.0 9.2 1284 17.14 1.15 2.8 6.6
1235 15.74 0.93 5.2 9.0 1285 17.33 0.76 2.7 6.4
1236 17.32 0.54 5.0 8.9 1286 17.47 0.76 2.6 6.0
1237 14.43 0.62 4.6 9.0 1287 15.59 0.54 2.2 6.3
1238* 17.24 0.85 4.3 9.2 1288 16.11 1.03 2.0 6.9
1239* 15.45 1.27 3.8 9.2 1289 17.18 0.66 1.9 6.9
1240* 15.96 0.69 3.7 9.3 1290 17.29 - 1.4 7.0
1241 17.37 - 3.3 9.5 1291 16.21 0.93 1.5 6.7
1242 17.56 0.32 2.9 9.5 1292 16.03 0.89 1.2 6.4
1243 15.85 0.24 2.8 9.3 1293 14.93 0.84 1.5 6.4
1244 16.53 0.83 2.5 9.2 1294 14.93 0.48 1.6 5.9
1245 17.28 0.85 2.3 9.3 1295 16.88 1.18 1.7 5.9
1246 16.44 1.07 2.1 9.8 1296 16.47 0.36 1.6 5.7
1247 17.47 - 1.5 9.0 1297 16.54 0.62 1.5 5.5
1248 17.41 0.01 2.0 9.0 1298 17.38 0.93 1.3 5.7
1249 16.16 1.29 2.0 9.0 1299 11.11 0.47 1.0 5.5
1250 15.27 0.41 3.4 8.9 1300 17.22 1.34 1.3 5.1
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1301 14.15 0.38 1.6 5.1 1351 15.49 1.07 3.0 2.6
1302 16.55 0.74 2.4 5.3 1352 17.28 0.56 3.1 2.7
1303 15.03 0.63 3.1 5.3 1353 16.85 1.21 3.7 2.7
1304* 15.05 0.53 3.2 5.6 1354 17.02 0.77 3.9 2.3
1305* 14.92 0.77 3.3 5.5 1355 17.26 1.10 4.1 2.7
1306 17.41 0.41 3.5 5.6 1356 16.71 0.49 4.0 2.9
1307 16.94 1.26 3.5 5.3 1357 16.66 0.80 4.4 2.9
1308 17.39 0.06 3.8 5.3 1358 16.90 0.78 4.4 2.8
1309 17.29 0.90 3.7 5.5 1359 17.05 0.69 4.4 2.3
1310 16.94 0.75 3.7 5.8 1360 17.44 0.80 4.2 1.8
1311 14.56 0.31 4.0 5.8 1361 16.34 0.36 4.6 1.9
1312 16.18 0.61 4.1 3.9 1362 14.29 0.80 4.8 2.3
1313 13.19 0.31 3.9 3.9 1363 - - - -
1314 14.73 0.57 3.7 3.9 1364 17.20 1.03 5.2 2.7
1315 16.84 0.93 3.6 4.1 1365 15.30 0.61 5.3 3.1
1316 16.05 0.73 3.7 4.3 1366 17.51 0.59 5.7 3.3
1317 17.32 1.35 3.3 4.6 1367 14.77 0.19 5.5 3.6
1318 15.04 0.63 3.0 3.9 1368* 16.04 0.53 4.8 3.7
1319 17.37 - 3.2 3.9 1369 16.55 0.33 4.6 3.7
1320 16.46 0.88 3.9 3.7 1370 17.66 0.50 4.8 3.9
1321* 15.89 1.10 4.2 3.5 1371 13.06 1.07 4.9 3.9
1322* 16.92 0.81 4.3 3.5 1372 14.13 0.47 5.0 4.0
1323 14.91 0.21 3.9 3.2 1373 16.72 0.38 4.6 4.3
1324 14.60 0.45 3.4 3.3 1374 15.05 1.66 4.4 4.6
1325 17.70 0.13 2.7 3.0 1375 14.74 0.54 4.8 5.2
1326 16.53 0.51 2.7 3.4 1376 14.81 0.45 4.4 5.0
1327* 14.73 0.98 2.8 3.6 1377 15.64 0.34 4.6 5.3
1328 14.37 1.44 2.4 4.0 1378 16.77 0.46 4.6 5.5
1329 13.57 1.23 2.5 4.4 1379* 17.52 1.04 5.4 6.0
1330 16.91 0.63 2.5 4.6 1380 11.51 0.31 5.6 6.5
1331 17.40 0.17 2.4 4.8 1381 17.53 0.95 5.4 6.6
1332 17.27 1.00 2.2 4.6 1382 16.99 0.83 5.1 6.9
1333 16.91 0.46 1.8 4.7 1383 14.48 0.50 5.0 7.4
1334 13.55 0.35 1.9 4.3 1384 16.45 0.80 5.5 7.8
1335 17.46 1.27 1.7 4.2 1385 17.08 0.58 5.7 7.9
1336 17.37 -0.16: 1.5 3.7 1386 15.79 0.30 6.0 8.0
1337 17.04 0.76 1.1 3.5 1387 15.72 0.57 5.8 8.4
1338 15.15 0.51 1.0 3.2 1388 17.48 - 4.9 8.9
1339 16.89 0.66 1.2 3.3 1389 17.30 - 5.8 8.9
1340 17.34 0.88 1.4 3.1 1390 15.68 0.56 5.7 9.5
1341 17.42 0.35 1.5 3.2 1391 15.18 0.59 5.2 9.7
1342 16.20 0.23 1.7 3.3 1392 17.50 0.70 5.4 9.9
1343* 13.10 0.71 1.8 3.3 1393 15.93 0.66 5.0 11.6
1344 14.49 0.94 2.2 3.3 1394 16.85 0.75 5.3 11.3
1345 13.96 0.28 2.1 3.1 1395 16.14 0.97 5.7 11.5
1346 17.06 0.42 2.1 2.9 1396 17.48 - 6.1 10.9
1347 17.40 0.61 2.2 2.7 1397 17.45 0.83 6.0 10.8
1348 16.87 0.37 2.2 2.6 1398 17.03 0.26 5.9 10.7
1349 16.49 0.41 2.6 2.5 1399 13.15 0.28 6.2 10.6
1350 17.01 0.42 2.6 2.7 1400 16.16 0.21 6.0 10.2
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1401 15.07 0.60 7.0 10.3 1451 16.50 1.50 10.4 6.0
1402 14.90 0.48 7.2 10.3 1452 17.37 1.07 10.9 6.1
1403 17.30 0.75 7.5 10.4 1453 16.20 0.61 11.3 6.0
1404 16.71 0.27 7.5 9.9 1454 17.59 0.44 11.0 5.9
1405 14.13 0.77 8.0 9.8 1455 16.32 0.74 11.9 5.2
1406 16.20 0.08 8.4 9.6 1456 17.37 0.60 11.2 5.2
1407 17.34: -0.96: 8.4 9.3 1457 17.12 1.10 10.5 5.3
1408 17.36 1.27 8.2 9.0 1458 17.02 0.65 10.6 5.1
1409 17.07 - 8.0 8.9 1459 17.30 - 8.6 5.4
1410 17.15 1.10 7.8 8.9 1460 17.60 0.00 8.2 5.6
1411 15.73 0.14 7.5 9.5 1461 16.90 1.68 8.7 6.2
1412 17.31 - 6.2 9.7 1462 16.48 0.85 8.9 6.8
1413 17.07 0.69 7.0 9.3 1463 15.71 1.21 8.4 6.5
1414 17.38 - 7.1 9.2 1464 14.48 0.61 8.2 6.5
1415 16.28 0.84 6.6 8.9 1465 17.40 0.40 8.0 6.2
1416 16.09 0.23 6.6 8.8 1466 17.44 0.42 7.6 6.9
1417 12.22 0.32 6.2 8.4 1467 15.46 0.58 7.2 6.7
1418 16.02 0.51 6.7 8.2 1468 15.74 0.50 6.9 7.4
1419 15.70 0.44 7.2 8.7 1469 16.84 0.12 6.5 7.9
1420 17.53 0.89 7.3 8.0 1470 17.46 0.69 6.3 7.6
1421 14.08 0.35 7.5 8.1 1471 17.39 1.23 6.0 7.2
1422 17.53 0.79 7.9 8.2 1472 17.47 1.02 5.7 6.9
1423 15.07 0.71 7.7 7.9 1473 17.17 0.30 6.2 7.0
1424 17.06 0.76 7.7 7.8 1474 15.77 0.79 5.9 6.0
1425 16.68 0.53 7.5 7.4 1475 15.95 0.51 6.1 5.6
1426 15.96 1.12 8.1 7.9 1476 14.45 0.55 6.2 5.4
1427 17.33 0.45 8.3 7.7 1477 17.10 0.05 6.3 5.3
1428 11.32 0.98 8.7 7.7 1478 17.55 0.58 6.2 5.3
1429 15.24 0.43 8.7 8.7 1479 16.24 0.66 5.9 5.0
1430 17.24 0.22 9.2 9.2 1480 17.32 0.84 5.2 4.7
1431 13.38 0.56 9.7 8.8 1481 12.00 0.93 6.0 4.7
1432 17.37 1.06 9.3 8.5 1482 14.58 0.35 6.3 4.3
1433 17.39 0.58 9.6 8.4 1483 17.40 0.90 7.0 4.4
1434 16.76 1.51 10.1 8.2 1484 15.85 0.68 7.4 4.6
1435 15.70 0.27 9.9 8.1 1485 15.14 0.19 6.5 5.3
1436 16.79 0.42 9.0 8.1 1486 17.01 0.73 6.7 6.1
1437 14.12 0.69 9.7 7.7 1487 16.24 0.77 7.1 5.9
1438 17.48 1.09 9.4 7.7 1488 17.52 0.45 6.9 5.5
1439 17.32 - 9.0 7.3 1489 14.25 0.95 7.2 5.5
1440 14.87 0.84 9.4 6.9 1490 12.26 0.73 7.5 5.5
1441 12.71 0.56 9.6 6.5 1491 16.95 0.45 7.6 5.4
1442 15.49 0.73 9.9 6.8 1492 13.59 0.48 8.0 5.4
1443 17.27 - 10.7 7.1 1493 15.98 0.53 7.7 5.2
1444 17.05 0.91 10.1 6.6 1494 17.26 0.76 7.5 5.2
1445 17.43 - 9.8 6.3 1495 11.47 0.47 7.9 4.8
1446 15.17 0.98 9.6 6.1 1496 16.93 0.78 9.5 4.5
1447 15.78 0.77 9.4 5.9 1497 13.26 0.56 9.7 4.3
1448 17.12 0.86 9.4 5.8 1498 17.27 1.04 10.8 4.1
1449 15.85 0.72 9.2 5.8 1499 12.39 0.68 10.8 4.3
1450 12.61 1.06 9.8 5.8 1500 17.61 1.06 11.2 4.4
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1501 13.76 0.90 11.7 3.9 1551 16.57 0.61 7.4 3.3
1502 17.40 0.87 12.0 3.7 1552 15.94 0.82 7.6 3.3
1503 15.31 1.38 12.0 3.3 1553 14.48 0.41 7.9 3.1
1504 14.57 1.29 12.1 2.6 1554 17.25 0.61 7.2 2.7
1505 14.55 0.99 12.4 2.0 1555 15.28 1.05 7.1 2.5
1506 17.52 1.01 11.5 1.9 1556 15.33 0.81 7.5 2.1
1507 16.36 0.41 11.3 1.9 1557 16.94 0.58 7.6 1.9
1508* 16.02 0.63 11.6 2.3 1558 13.18 0.79 7.8 1.6
1509 15.42 0.58 11.6 2.8 1559 16.01 0.77 8.0 1.4
1510 17.40 0.85 11.4 2.5 1560 15.08 0.51 7.9 1.0
1511 17.55 0.47 11.2 2.5 1561 16.38 0.61 7.6 1.1
1512 16.13 0.79 11.3 3.0 1562 17.44 0.81 7.4 1.4
1513 17.37 1.06 11.5 3.4 1563 14.54 0.77 7.1 1.4
1514 16.19 0.64 11.0 3.6 1564 16.12 0.16 6.8 2.6
1515 17.25 1.00 10.7 3.5 1565 14.71 0.66 6.6 3.1
1516 16.90 0.43 10.6 3.2 1566 15.78 0.57 5.4 2.6
1517 13.93 0.44 10.5 2.5 1567 17.26 0.44 5.3 2.2
1518 14.45 0.84 10.4 2.2 1568* 17.24 0.52 5.0 2.1
1519 13.21 0.64 10.4 3.4 1569* 14.52 0.69 5.0 2.0
1520 15.35 1.30 10.1 3.9 1570 17.29 0.94 4.3 1.7
1521 16.88 0.99 10.1 3.7 1571 17.44 0.07 - -
1522 17.38 0.89 9.9 3.4 1572 16.62 0.75 4.1 1.2
1523 15.88 0.66 9.7 3.8 1573 17.66 0.31 4.2 0.3
1524 16.85 0.78 9.5 3.8 1574 14.86 0.30 4.1 0.0
1525 16.59 0.58 9.4 3.5 1575 17.57 0.72 4.3 - 1.3
1526 17.72 0.63 8.9 3.2 1576 17.39 1.04 3.8 - 1.6
1527 16.01 0.98 9.0 2.9 1577 17.49 1.17 3.6 - 2.3
1528 16.13 0.58 9.2 2.9 1578 16.79 0.35 4.0 - 2.5
1529 15.98 0.78 9.8 2.4 1579 17.54 0.52 4.1 - 2.6
1530 17.40 0.37 9.6 2.1 1580 15.41 0.71 4.1 - 2.7
1531 17.17 0.88 9.8 1.9 1581 16.89 1.03 3.9 - 2.8
1532 15.91 0.88 9.8 1.7 1582 15.65 0.25 4.4 - 3.3
1533 11.06 1.50 9.1 1.6 1583 15.82 0.24 3.8 - 4.5
1534 16.93 0.57 9.1 2.0 1584 17.14 0.09 4.0 - 5.2
1535 15.05 0.35 8.3 2.8 1585 12.71 1.06 3.8 - 6.0
1536* 17.10 0.60 8.8 4.3 1586 16.17 1.71 3.8 - 6.2
1537* 17.69 0.36 8.8 4.4 1587 16.81 1.17 4.0 - 6.3
1538 17.45 0.64 8.4 4.3 1588 16.69 0.42 3.7 - 6.4
1539 17.40 - 7.7 4.2 1589 15.98 0.56 3.6 - 7.1
1540 14.86 0.83 7.6 3.7 1590 16.11 0.37 3.4 - 7.6
1541 17.46 0.57 6.6 3.7 1591 17.40 0.38 3.9 - 8.0
1542 16.27 0.81 6.2 3.9 1592 15.40 0.83 3.8 - 8.6
1543 17.38 1.01 5.5 4.1 1593 17.59 0.46 3.2 - 8.9
1544 16.50 1.43 5.3 4.0 1594 14.77 0.30 3.6 - 9.6
1545 17.21 1.00 5.6 3.9 1595 17.01 0.20 3.5 -10.3
1546 16.53 1.16 5.9 3.8 1596 14.40 0.47 3.2 -11.2
1547 17.53 0.36 6.2 3.4 1597 16.04 0.32 3.9 -11.0
1548 17.20 0.99 6.5 3.0 1598 16.94 0.42 3.9 -10.6
1549 15.24 0.58 6.6 3.3 1599 16.60 0.81 4.1 -10.6
1550 13.33 0.58 7.2 3.3 1600 15.45 0.66 4.2 -10.3
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1601 17.30 0.21 4.2 - 9.4 1651 14.18 1.13 6.4 - 7.0
1602 15.91 0.62 4.5 - 9.7 1652 17.45 0.63 7.0 - 7.3
1603 15.38 0.75 5.3 -10.3 1653 16.49 0.50 7.0 - 7.4
1604* 15.57 0.54 5.5 -10.3 1654 16.84 0.60 6.9 - 7.7
1605 17.52 0.59 5.9 -10.1 1655 17.43 0.59 7.6 - 8.1
1606 16.21 0.80 6.3 -10.0 1656 14.03 0.94 8.5 - 8.2
1607 13.56 0.27 6.5 - 9.9 1657 17.40 0.35 8.7 - 7.4
1608 17.31 0.65 6.7 - 9.7 1658 15.29 0.56 8.5 - 7.5
1609 15.40 0.37 6.2 - 9.9 1659 13.59 0.55 8.2 - 7.6
1610 16.81 1.23 6.0 -10.0 1660 16.98 0.41 7.9 - 7.6
1611 17.42 0.47 5.5 -10.0 1661 15.04 0.67 7.9 - 6.7
1612 15.76 0.30 5.2 - 9.8 1662 16.32 0.35 8.0 - 6.3
1613 16.18 0.40 5.5 - 9.5 1663 15.26 0.59 7.6 - 6.2
1614 15.28 0.56 5.4 - 9.3 1664 17.14 0.24 7.8 - 6.1
1615 15.09 0.91 5.2 - 9.2 1665 13.17 0.44 8.0 - 5.9
1616 15.58: 2.80: 3.9 - 9.1 1666 15.72 0.25 7.8 - 5.6
1617 17.41 0.55 4.0 - 9.0 1667 12.44 0.80 8.2 - 5.6
1618 17.60 0.94 4.2 - 8.7 1668 17.20 0.34 8.5 - 5.7
1619 15.81 0.20 4.6 - 8.3 1669 16.73 0.08 8.7 - 5.7
1620* 14.61 0.70 4.8 - 8.4 1670 14.71 0.96 9.2 - 6.2
1621 16.03 0.68 4.9 - 8.8 1671 17.55 - 9.9 - 7.3
1622 14.93 0.42 6.0 - 9.1 1672 17.33 0.92 9.8 - 6.7
1623 16.28 0.39 6.2 - 9.0 1673 15.74 0.51 10.1 - 6.1
1624* 11.08 0.88 6.9 - 9.1 1674 17.41 0.35 10.4 - 5.6
1625 16.00 0.36 7.0 - 8.6 1675 16.45 0.87 10.3 - 5.3
1626 16.30 0.47 6.8 - 8.3 1676 14.85 0.37 10.7 - 5.2
1627 15.69 0.12 6.5 - 8.6 1677 16.66 0.83 11.0 - 5.0
1628 16.46 1.09 6.4 - 8.9 1678 17.63 0.89 11.2 - 5.0
1629 17.35 0.32 6.3 - 8.3 1679 17.07 0.67 11.4 - 4.6
1630 16.77 0.41 5.7 - 8.2 1680 17.46 0.96 10.9 - 4.9
1631 16.31 0.41 6.2 - 7.9 1681 14.89 0.57 10.1 - 4.9
1632 16.60 0.36 5.7 - 7.6 1682 13.24 0.59 10.0 - 5.1
1633 11.13 0.95 4.8 - 7.5 1683 15.92 0.12 9.7 - 5.5
1634 17.56 0.73 4.3 - 7.4 1684 17.03 -0.22: 9.0 - 5.0
1635 14.83 0.39 4.5 - 7.1 1685 16.91 0.34 9.0 - 4.8
1636 13.44 0.38 3.2 - 7.0 1686 17.39 0.72 9.2 - 4.7
1637 14.61 1.07 4.1 - 6.6 1687 17.47 0.62 8.7 - 4.6
1638 14.68 0.43 5.2 - 5.8 1688 17.52 0.56 8.0 - 4.1
1639 15.48 - 5.6 - 6.0 1689 16.85 0.46 7.9 - 4.1
1640 15.33 0.76 5.2 - 6.2 1690 15.43 0.47 7.9 - 4.3
1641 15.09 0.32 5.2 - 6.8 1691 14.75 0.41 8.1 - 4.6
1642 15.68 0.05 5.5 - 6.3 1692 17.23 1.63 7.7 - 5.1
1643 14.01 0.30 5.7 - 6.3 1693 15.48 0.35 7.6 - 5.2
1644 16.63 0.30 5.9 - 6.0 1694 16.01 0.53 7.2 - 4.8
1645 13.92 0.44 6.1 - 6.1 1695 17.29 0.41 7.3 - 4.4
1646 17.13 0.74 6.5 - 6.2 1696 16.85 0.35 7.1 - 4.2
1647 16.77 0.36 6.7 - 6.4 1697 16.07 0.33 7.2 - 4.1
1648 17.51 1.37 6.1 - 6.3 1698 16.49 0.36 7.0 - 4.1
1649 17.47 0.18 5.9 - 6.7 1699 17.39 0.50 6.8 - 4.0
1650 16.14 0.91 6.1 - 6.7 1700 13.69 0.89 6.5 - 4.2
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1701 17.60 1.02 6.4 - 4.4 1751 16.74 0.41 9.5 - 3.0
1702 15.27 0.07 6.5 - 5.6 1752 16.15 0.66 9.3 - 2.8
1703 17.51 0.26 6.0 - 5.7 1753 16.21 0.54 9.7 - 2.4
1704* 12.04 0.61 6.3 - 4.7 1754 14.92 -1.54: 9.8 - 2.8
1705 12.71 0.65 6.2 - 4.8 1755 14.17 1.10 10.2 - 2.9
1706 15.63 0.66 6.2 - 4.3 1756 16.24 0.70 10.4 - 2.9
1707 16.76 0.24 5.9 - 4.2 1757 13.68 1.14 10.6 - 3.0
1708 15.87 0.79 5.7 - 4.3 1758 15.74 0.86 11.1 - 3.3
1709 15.23 0.66 5.6 - 4.9 1759 17.23 1.73 11.7 - 4.0
1710 17.82 0.52 5.3 - 4.9 1760 14.75 0.71 11.9 - 3.4
1711 17.51 0.94 4.9 - 5.0 1761 17.51 1.16 12.1 - 3.2
1712 17.42 1.05 4.7 - 3.2 1762 13.91 0.72 12.4 - 2.4
1713 17.05 1.08 4.8 - 3.6 1763 12.72 0.49 11.4 - 2.4
1714 15.79 0.47 5.0 - 3.6 1764 16.98 0.01 12.0 - 2.1
1715 17.51 0.53 5.5 - 3.5 1765 17.05 0.58 12.3 - 1.9
1716 15.81 0.76 6.1 - 3.6 1766 16.65 0.30 11.4 - 1.8
1717 17.27 1.19 6.3 - 3.3 1767 14.82 0.71 10.8 - 1.4
1718 15.30 0.35 6.1 - 3.4 1768 14.28 0.64 10.8 - 0.2
1719 16.13 0.55 5.9 - 3.4 1769 16.18 1.43 11.2 - 1.3
1720 17.59 0.54 5.8 - 3.3 1770 15.42 0.74 11.6 - 1.3
1721 16.50 0.35 5.7 - 3.0 1771 14.52 0.34 11.9 - 1.6
1722 16.34 0.82 5.1 - 3.0 1772 17.62 - 12.2 - 1.4
1723 17.60 0.69 5.3 - 2.7 1773 17.55 - 12.0 - 0.9
1724 17.36 -0.03 5.8 - 2.7 1774 17.59 - 12.1 - 0.4
1725 16.15 0.86 5.9 - 2.9 1775 16.76 1.05 11.0 - 0.6
1726 17.69 0.96 6.5 - 2.2 1776 13.55 0.92 10.6 - 1.0
1727 16.58 1.15 6.5 - 2.3 1777 14.57 0.78 10.3 - 1.1
1728 17.38 0.30 7.3 - 1.3 1778 16.52 0.62 9.7 - 0.6
1729 15.38 0.43 7.2 - 1.5 1779 15.36 0.73 9.6 - 1.2
1730 17.22 0.50 7.2 - 1.7 1780 15.96 0.33 9.3 - 1.8
1731 14.22 0.86 7.3 - 1.8 1781 16.03: 2.24: 9.2 - 2.1
1732 17.50 - 7.2 - 2.1 1782 14.56 0.59 9.1 - 2.1
1733 16.35: 2.37: 7.5 - 2.1 1783 17.30 1.65 8.9 - 2.7
1734 12.92 0.63 7.2 - 2.3 1784 15.72 0.52 8.7 - 2.4
1735 16.43 0.36 7.4 - 2.7 1785 15.05 0.39 8.4 - 2.1
1736 16.46 0.14 7.4 - 2.8 1786 16.32 0.80 8.7 - 1.8
1737 16.66 1.37 7.4 - 3.0 1787 16.64 0.72 9.1 - 1.4
1738 17.41 0.95 7.8 - 3.1 1788 16.37 0.34 9.2 - 1.2
1739 15.71 0.11 8.2 - 4.0 1789 16.93 0.56 9.2 - 0.7
1740 12.95 0.60 8.4 - 3.8 1790 17.43 0.75 8.3 - 0.8
1741 16.99 0.24 8.5 - 3.6 1791 15.91 0.98 8.2 - 1.1
1742 14.61 0.36 8.2 - 3.2 1792 16.80 0.99 7.8 - 1.1
1743 15.25 0.47 8.4 - 3.3 1793 17.61 0.53 7.7 - 0.6
1744 15.70 0.82 8.5 - 3.3 1794 17.41 0.37 7.5 - 0.9
1745 13.57 1.01 8.6 - 3.2 1795 17.31 0.70 7.2 - 0.7
1746 17.39 0.81 10.0 - 4.3 1796 17.53 - 7.1 - 1.1
1747 15.81 0.43 10.7 - 4.0 1797 14.87 0.83 6.8 - 0.9
1748 15.72 0.54 10.4 - 3.7 1798 14.04 0.37 6.8 - 0.6
1749 17.26 0.86 9.8 - 3.4 1799 15.72 0.84 6.5 - 0.5
1750 15.46 0.56 9.3 - 3.3 1800 16.15 0.36 6.3 - 0.6
Table (Cont.)
No. V B-V X Y No. V B-V X Y
1801 17.54 0.11 5.8 - 0.9 1851* 14.44 0.43 8.7 0.8
1802 15.71 0.47 5.5 - 1.4 1852 16.74 0.38 8.8 - 0.4
1803 16.10 0.41 5.8 - 1.8 1853 17.42 0.72 9.1 - 0.2
1804 16.88 0.98 5.9 - 1.9 1854 16.43 0.63 9.3 0.0
1805 15.86 0.41 5.6 - 1.9 1855 17.00 0.69 9.6 0.0
1806 17.36 1.30 5.4 - 1.8 1856* 17.24 1.45 9.8 - 0.1
1807 16.23 0.92 4.9 - 2.1 1857* 15.50 0.82 9.9 0.0
1808 16.80 0.49 4.5 - 2.3 1858 16.46 -0.39: 9.8 0.4
1809 16.48 0.36 5.1 - 1.6 1859 15.28 0.79 9.6 0.6
1810 16.12 0.94 5.0 - 1.5 1860 17.02 - 9.3 0.6
1811 15.60 0.34 4.9 - 1.4 1861 15.62 0.34 9.2 1.0
1812 15.66 0.38 4.8 - 1.3 1862 16.83 0.37 9.1 1.3
1813 17.09 0.49 5.0 - 1.2 1863 17.59 0.88 9.9 1.6
1814 15.52 0.60 4.9 - 0.4 1864 17.28 1.17 10.3 1.9
1815 17.21 0.23 4.6 - 0.2 1865 13.37 0.47 10.6 1.5
1816 17.36 1.22 5.0 0.1 1866 13.56 - 10.4 1.3
1817 17.58 0.54 5.2 0.5 1867 13.75 0.32 10.3 1.1
1818 17.44 0.25 5.0 0.7 1868 17.77 0.62 10.7 1.2
1819 15.68 0.66 4.9 1.0 1869 17.25 0.46 10.6 0.1
1820 16.06 0.33 5.0 1.5 1870 17.56 0.89 10.8 0.2
1821 14.76 0.33 5.5 1.8 1871 15.52 1.00 10.8 0.4
1822 14.42 0.43 5.6 1.3 1872 16.68 0.08 11.0 0.3
1823 15.96 1.24 5.5 1.1 1873 15.19 0.59 11.6 0.4
1824 16.55 0.84 5.5 1.0 1874 15.94 0.53 11.3 0.8
1825 16.56 0.26 5.7 0.6 1875 13.98 0.55 11.2 1.5
1826 15.57 0.65 5.5 0.4 1876 15.59 0.57 11.7 1.9
1827 15.61 0.55 5.4 0.1 1877 16.75 0.30 11.9 2.1
1828 17.61 1.13 5.6 - 0.2 1878 17.22 1.13 12.4 2.3
1829 17.27 0.73 6.2 - 0.1 1879 16.44 0.89 12.3 2.1
1830 17.32 0.91 6.2 0.2 1880 17.33 1.07 12.6 1.9
1831 17.43 0.96 6.0 0.1 1881 14.00 1.29 12.8 2.0
1832 16.56 0.28 6.0 0.5 1882 16.94 1.31 12.8 1.9
1833 17.54 0.87 6.1 0.7 1883 16.60 0.35 12.5 1.5
1834 16.94 0.55 6.5 0.9 1884 17.11 0.44 12.6 1.3
1835 17.55 - 6.5 1.7 1885 16.96 0.09 12.7 1.1
1836 17.39 0.55 6.9 1.3 1886 17.62 1.00 12.0 1.1
1837 16.30 0.92 6.8 1.1 1887 14.03 0.44 12.1 1.0
1838 14.63 1.15 7.0 1.0 1888 16.41 1.92 12.4 0.7
1839 12.91 1.08 7.1 1.0 1889 15.83 1.16 12.5 0.5
1840 16.57 0.52 7.1 0.2 1890 17.05 0.66 12.6 0.7
1841 15.02 0.38 8.1 - 0.4
1842 17.51 0.54 8.3 - 0.1
1843 17.75 0.89 8.2 0.4
1844 14.91 0.54 7.9 0.2
1845 16.97 0.26 7.7 0.7
1846 17.28 1.16 7.7 0.9
1847 17.25 1.58 8.2 1.6
1848 15.26 0.76 8.8 1.6
1849 16.86 0.96 8.8 1.2
1850 17.59 1.15 9.0 1.1
NOTES TO THE TABLE
A * at the right upper side of the running number denotes that the
photographic image of the measured star is distorted by a neighbouring
star.
A colon beside the V and B-V colours denotes that the star is measured
only on one or two plates or the measured magnitudes obtained from
different plates have large dispersion.