COMMUNICATIONS	       MITTEILUNGEN
                     FROM THE	                   DER
               KONKOLY OBSERVATORY	        STERNWARTE
                      OF THE	         DER UNGARISCHEN AKADEMIE
          HUNGARIAN ACADEMY OF SCIENCES	    DER WISSENSCHAFTEN

                            BUDAPEST - SZABADSAGHEGY


			   No. 79.



			   M. KUN

		  SPACE DISTRIBUTION OF STARS
		 IN A REGION OF CEPHEUS AROUND
			   NGC 7160





			BUDAPEST, 1982




SPACE DISTRIBUTION OF STARS IN A REGION OF CEPHEUS AROUND NGC 7160 ABSTRACT Objective prism spectral types and photographic U, B, V magnitudes have been determined for 1810 stars in a region of 19.5 square degrees of Cepheus centred on the galactic cluster NGC 7160. A catalogue of data together with identification charts is given. The magnitude limit is approximately V=12.5. The field contains a part of the supposed older subsystem of the association Cepheus OB2. The interstellar absorption in the region is smooth. The visual absorption is 1.0m at the distance of the association for the northern part of the field, and is about 1.4m for the southern part. Space densities of the stars have been computed as a function of spectral type and distance from the sun. Concentrations of B and early A type stars are found at 800 pc from the sun. General luminosity functions were derived at 200, 400, 600, 800, 1000 and 1200 pc, and an attempt was made to derive the shape of the luminosity function of the association subgroup. INTRODUCTION This paper is the second part of a study of stellar distributions in the association Cepheus OB2. It was shown by Blaauw (1964) that most OB associations consist of several subgroups of different ages. Simonson and van Someren Greve (1976) suggest that Cep OB2 consists of two subgroups: Cep OB2a is the older and more dispersed one; it is situated between l=100deg - 105deg and b=+2deg - +8deg. The younger subgroup, Cep OB2b, is the open cluster Tr 37 embedded in the HII region IC 1396 at l=99.7deg and b=+3.7deg. In a previous paper (Kun, 1979, hereinafter Paper I) the distribution of main sequence stars and the absorbing matter in the region of IC 1396 was described. It was shown that this group contains a great number of B3-B7 and B8-A1 stars in addition to the earliest type stars defining the group. In the present paper a similar study is made for the supposed older subgroup. The field chosen for this study is centred on the galactic cluster NGC 7160. The coordinates of the plate centre are: alpha(1950)=21h 52m, delta(1950)=+62deg 20' (l=104.6deg, b=+6.4deg). The total area is 19.5 square degrees. The field contains a part of Cep OB2a, the older subgroup of Cep OB2. Since no significant obscuration in this region can be observed, this field should be suitable for the statistical study of the space distribution of the stars. Figure 1 shows the surface distribution of the early type and supergiant members of the association, according to Simonson (1968) and Humphreys (1978). Figure 1: Surface distribution of the members of Cep OB2. Open circles denote blue supergiants and main sequence O stars; squares indicate red supergiants, dots B0V stars, and crosses B1V-B3V stars. OBSERVATIONAL DATA a) Spectral classification Spectra were classified from Kodak IIa-O plates taken with the 5deg ultraviolet transmitting objective prism attached to the 60/90/180 cm Schmidt telescope of Konkoly Observatory. It provides a dispersion of 580 A/mm at H_gamma. Spectra were widened to 18" on each plate. Exposure times were 30s, 6m and 24m. Criteria described by Seitter (1975) were used in classifying the spectra. In the case of stars later than F8 luminosity classes were also determined. Each star was classified on at least two plates. The number of classified stars is 1810. Figure 2 shows a comparison between the adopted spectral types and those of the Henry Draper Catalogue. This comparison involves 51 stars. There is a tendency in this work to classify the late B and early A stars slightly earlier than the corresponding classification in the HD Catalogue. Lindoff and Lynga (1966) found the same differences between the HD and MK types. Figure 2 MK classification of some early type stars of this field (Simonson, 1968) shows a good agreement with the present classification (Table 1). TABLE 1 HD number Sp. Sp(Simonson) S(HD) 207 198 B0 O9.5II B2 207 951 B1 B2V B8 208 185 B3 B1V A0 208 266 B1 B3V B5 208 761 B2 B3V B5 In accordance with the sharpness of the classification criteria and so that the space densities can be calculated the stars have been grouped into broad spectral ranges. These spectral ranges and the number of stars included in them are given in Table 2. TABLE 2 Spectral range number of stars earlier than B3 36 B3-B7 90 B8-A1 572 A2-A6 270 A7-F1 104 F2-F8 356 gG-gK 207 dG-dK 158 M 17 b) Photographic photometry U, B, V photographic magnitudes were obtained for all the stars that have been classified. Five plates were taken in each colour. The plate-filter combinations and exposure times are those described in Paper I. The plates were measured with the Cuffey irisphotometer of Konkoly Observatory. The photoelectric sequence for the photographic measures was taken from Hoag et al. (1961), Argue (1966) and Simonson (1968). The mean internal errors of the photometry are +-0.06 for both V and B, and +-0.08 for U. In addition to these random errors the ultraviolet filter had a field error in a restricted area. The estimated probable errors of U magnitudes of the stars affected by this field error are about +-0.2m. The limiting magnitude of the spectral classification is about B=13.0m. Figure 3 shows the distribution of the stars of different spectral ranges as a function of apparent B magnitude. The limiting magnitude in V depends on the colour of the stars; on the average, the limiting V is about 12.5m, but for the K stars it is about a magnitude lower. The Q colour differences have been determined for all stars earlier than A2 in order to have an independent spectral classification. For the stars showing a discrepancy between the classified spectra and the Q value taken from Johnson (1958), the average of the two subclasses was adopted for the spectral type. Figure 3 c) Completeness of spectral data Because the region investigated is situated close to the galactic plane, the surface density of stars is high, thus there are a great number of overlapped spectra. It is hard to estimate how the unclassifiable overlapped spectra affect the completeness of our data. Figure 4 gives lgN(m_B) values, where N(m_B) is the total number of stars per square degree brighter than m_B, as a function of B magnitude. McCuskey's study of LF4 (1951) and Kubinec's (1973) work for an adjacent Cepheus region provide values of lgN(m) for comparison with present data; they are also plotted in Fig. 4. Though these surveys are made at slightly lower galactic latitudes, they do allow us to make an estimate of the completeness of the present survey: it is estimated that the survey is complete to B=13.0m. Figure 4: logN(m) versus m. Dashed line refers to McCuskey's LF survey, dotted line Kubinec's (1973) result. The solid line shows the present survey. INTERSTELLAR ABSORPTION By examining Khavtassi's Atlas of Galactic Dark Nebulae it can be seen that the interstellar absorption pattern is relatively smooth in this region. There are two dark nebulae of moderate obscuration in the southern part of the field: Khavtassi 170 and 173. We can distinguish two regions with slightly different reddenings: Figs. 5a and 5b show the E_B-V colour excesses against the uncorrected distance modulus. The higher reddening affects about five hundred stars in the southern part of the field. The solid lines in Figs. 5a and 5b represent the adopted relation between colour excess and distance modulus. The relations between the total visual absorption, a_v and the distance, r are given in Figs. 6a and 6b for the two regions. These were determined from Figure 5 with R=3.0. Figure 5: E_B-V_ versus distance modulus a) for the region of low reddening; b) for the region of high reddening. Dots indicate A0 type stars, crosses F type stars, and open circles photoelectric measurements taken from Hoag et al. (1961), and Simonson (1968). Stars of the association Cep OB2 are situated between distances of 600 and 1100 pc (Simonson, 1968). It can be seen from Fig. 6 that there is no obscuring matter in this region in the northern part of the field, but in the region covered by the dark nebulae an absorption begins about 850 pc. Figure 6 SPACE DENSITIES The stellar space densities can be determined after having corrected the apparent magnitudes of stars for the interstellar absorption. For this purpose Dolan's (1974) matrix method was used. The adopted mean absolute magnitudes and dispersions for the spectral ranges are taken from Allen (1973). The resulting space densities as functions of the distance from the sun are given in Figs. 7-10. The general characteristics of spatial distributions of stars can be summarized as follows: B0-B2 stars: (Figure 7a) The density curve has a sharp maximum at 700 pc, and a "shoulder" between 900-1100 pc. Beyond 1100 pc there is a sudden decrease. As the region is 6.5deg above the galactic plane, and at 1200 pc it corresponds to z=130 pc, not many background stars of this type can be expected. B3-B7 stars: (Fig. 7b) The structure of this curve is similar to the previous one. The maximum is broader than in the case of the earlier group. The shoulder can also be seen. The density of the background slowly decreases between 1100 and 1400 pc, and a faster decrease begins beyond 1400 pc. Figure 7 Figure 8 B8-A1 stars: (Fig. 8a) The density continuously decreases to 600 pc and it has a broad maximum at 800 pc. For comparison, van Rhijn's (1955) density data obtained at l=100deg, b=+7deg are also indicated in Fig. 8a (dashed line). The curve suggests that the place of its maximum indicates the same stellar group as the early type stars. The density maximum at the distance of the association is more pronounced when we consider the distribution of B8-A1 stars in a smaller region around the cluster. Fig. 8b shows this arrangement for a circle of radius of one degree centred on NGC 7160. This region contains 107 B8-A1 stars. Here the density sharply increases to 830 pc, it is nearly constant between 830-1000 pc, and then it decreases similarly to the previous curve. Figure 9a A2-A6 stars: (Fig. 9a) The density is constant between 250 and 400 pc, and has a large negative gradient beyond 400 pc. The dashed line indicates the plate limit. A7-F1 stars: (Fig. 9b) The density continuously decreases beyond 300 pc. It stops decreasing at about 650 pc. Unfortunately it is near the plate limit. F2-F8 stars: (Fig. 9c) The curve has a maximum at 250 pc and sharply decreases beyond it. G0-K3 giants: (Fig. 10) The curve is also characterized by the large negative gradient. Figure 9b-c The density of G-K dwarfs has not been calculated; they are very faint, thus the plate limit is about 200 pc. The most significant features of the space density distributions are the presence of the association in the distribution of stars earlier than A2, and the large negative gradients for the later types, and even for the early types at greater distances. In the case of B and early A stars this gradient can be explained by the increasing distance from the galactic plane. In the case of A2-F8 stars, however, there must be a true concentration of stars near the sun. The same phenomenon was found by Kubinec (1973) for an adjacent region, lying exactly in the galactic plane. Figure 10 The ratio of B8-A1 main sequence stars to the G8-K3 giants has been calculated as a function of apparent V magnitude. Because the absolute visual magnitude of these two groups are nearly the same (+0.5m), equal apparent magnitudes correspond to equal distance moduli. It was shown by Sandage (1957) that this ratio has evolutionary implications: N(A)/N(K) is large for the relatively young regions of the Galaxy. Figure 11 gives the ratio N(A)/N(K) as a function of V for both subgroups of Cep OB2. The data for the region of IC 1396 are taken from Paper I. In this region there is an excess of bright K giants; and in both regions the ratio shows a steep increase at V=10. Unfortunately it is not possible to follow this ratio to the fainter stars because the K giants having a V magnitude larger than 11.0 are near the plate limit. The high value of N(A)/N(K) between V=10 and 11 (the corresponding corrected distance moduli are 8.5-9.5 for IC 1396 and 9.0-10.0 for NGC 7160) also indicates an excess of main sequence A stars in the volume of the association. Figure 11 LUMINOSITY FUNCTIONS The stellar luminosity function is defined as the number of stars per cubic parsec with absolute magnitudes in the range M-1/2, M+1/2, at distance r. It can be calculated from the space densities by the formula: The luminosity function has been determined for this field at distances of 200, 400, 600, 800, 1000 and 1200 pc, between the absolute magnitudes -5m and +1m and for the lower distances to +2m. The results are shown in Fig. 12. The dashed lines indicate McCuskey's (1966) luminosity function for the solar neighbourhood. At 200 pc our luminosity function agrees well with this function, and at 1200 pc (at z=130 pc) they are nearly parallel with each other. Between these limits there is an excess of bright stars, showing the presence of the association. Figure 12 Using the resulting space densities we made an attempt to determine the luminosity function of the association subgroups. From the shape of the density curves of B0-B2 and B3-B7 stars an estimate can be made for the density of the field stars at the distance of the association by extrapolating the density values beyond 1100 pc to the smaller distances. Thus the space densities of the true association members can be estimated. A somewhat less reliable estimation can be made for the density of the B8-A1 members using van Rhijn's data for the density of the field. His survey was made near the assumed border of Cep OB2. Figure 13: Luminosity functions of the two subgroups of Cep OB2 and those of the underlying field, derived from the stellar densities. Open circles denote the field and dots the association. Dashed line: Cep OB2a, solid line: Cep OB2b. Dotted line: Limber's (1960) initial luminosity function. On the basis of these extrapolated densities the luminosity functions of the two subgroups have been calculated. For the region of IC 1396 the density curves given in Paper I were used. The resulting luminosity functions are shown in Fig. 13 together with the so obtained field star luminosity functions. It can be seen that the gradients of the luminosity functions of the two subgroups do not differ significantly from each other nor from the standard initial luminosity function published by Limber (1960). The smaller values obtained for Cep OB2a may indicate the more dispersed nature of this group. The relative proportions of stars of different absolute magnitudes, however, are remarkably similar in the two subgroups. The supergiants are not included in these luminosity functions, but according to Humphreys (1979) the number of supergiants is nearly the same for the two subgroups. This close similarity of the two subgroups indicates that they were produced under similar physical conditions. ACKNOWLEDGEMENT I thank to Mrs. I. Kalman, Mrs. I. Gal, Mr. I. Toth and Mr. L. Sturmann for their help in data processing. REFERENCES Allen, C. W., 1973, Astrophysical Quantities, Athlone Press, London Argue, A. N., 1966, M. N. R. A. S. 133, 475. Blaauw, A. A., 1964, Ann. Rev. Astron. Ap. 2., 164. Dolan, J. F., 1974, Astron. Astrophys. 35. 105. Hoag, A. A., Johnson, H. L., Iriarte, B., Mitchell, R. I., 1961, Publ. U.S. Naval Obs., 2nd Series, XVIII, Part VII. Humphreys, R. M., 1978, Ap. J. Suppl. 38, 309. Johnson, H. L., 1958, Lowell Bull. No. 90. Khavtassi, J., 1960, Atlas of Galactic Dark Nebulae, Abastumani Astrophysical Obs. Kubinec, W. R., 1973, Publ. Warner and Swasey Obs. Vol. 1, No. 3. Kun, M., 1979, Mitt. Sternw. Budapest No. 72. (CoKon 72) Limber, D. N., 1960, Ap. J. 131, 168. Lindoff, U., Lynga, G., 1966, Medd. Lund Obs. Series 2, No. 146. McCuskey, S. W., 1951, Ap. J. 113, 672. McCuskey, S. W., 1966, Vistas in Astronomy 7, 156. Sandage, A. R., 1957, Ap. J. 125, 435. Seitter, W. C., 1975, Bonner Spectral Atlas II, Ferd. Dummler Verlag, Bonn Simonson, S. C., 1968, Ap. J. 154, 923. Simonson, S. C., van Someren Greve, H. W., 1976, Astron. Astrophys. 49, 343. van Rhijn, P. J., 1955, Publ. Kapteyn Astr. Lab. Groningen No. 57 Finding chart of the survey stars I. North-eastern part of the field Finding chart of the survey stars II. Northern part of the field Finding chart of the survey stars III. North-western part of the field Finding chart of the survey stars IV. South-western part of the field Finding chart of the survey stars V. Southern part of the field Finding chart of the survey stars VI. South-eastern part of the field CATALOGUE Spectra and UBV data of the survey stars No. Sp. V B-V U-B remarks 1 A0 8.59 0.13 -0.24 BD+61deg 2266 2 A0 8.46 0.07 -0.10 BD+61deg 2265 3 B7 10.65 0.10 -0.31 4 gK 8.63 1.01 1.29 BD+61deg 2259 5 A2 11.44 0.14 0.28 6 G0 9.26 0.50 0.19 BD+61deg 2256 7 A2 11.92 0.24 0.38 8 gK 10.39 1.90 2.60 9 A2 10.32 0.15 -0.04 10 A0 12.37 0.54 0.48 11 K0 12.67 1.06 0.69 12 A0 11.22 0.14 0.11 13 G8III 8.48 0.85 0.64 BD+61deg 2249 14 F8 11.67 0.47 0.03 15 A0 12.08 0.33 0.15 16 A2 11.60 0.18 0.27 17 A2 13.02 0.44 0.31 18 A0 12.60 0.30 0.17 19 A2 11.80 0.59 0.18 20 G0 10.24 0.49 0.07 BD+61deg 2238, blend 21 A0 12.08 0.38 0.27 22 G5III 11.00 1.29 0.96 23 B6 9.63 0.23 -0.06 BD+61deg 2237 24 A0 11.78 0.74 0.35 25 K0III 10.71 0.97 0.94: blend 26 A0 11.63 0.25 0.28 27 A2 11.68 0.11 0.13 28 B5 10.23 0.11 -0.51 29 K0III 11.05 1.11 1.08 30 A0 12.80 0.62 0.15 31 A0 13.04 0.35 0.10 32 A0 13.03 0.48 0.16 33 A0 12.26 0.81 0.19 34 F8 8.39 0.40 -0.13 BD+62deg 2016 35 K2III 10.72 1.29 1.22 36 B6 9.68 0.08 -0.04 BD+62deg 2015 37 A5 11.56 0.22 0.26 38 A0 11.68 0.67 0.04 39 F5 11.17 0.71 0.22 40 F5 10.55 0.40 -0.07 41 G2 11.28 0.62 0.13 42 A2 11.91 0.27 0.07 43 G5 11.64 0.50 0.09 44 A6 10.12 0.21 0.01 45 G5IV 11.06 0.66 0.26 46 A2 10.78 0.12 -0.11 47 G8III 9.64 1.39 0.72 48 F8 11.32 0.55 0.01 49 A0 11.68 0.26 0.24 50 F4 10.75 0.42 0.11 51 G2 10.19 1.17 0.95 52 A0 11.44 0.09 0.18 53 K5 5.05 1.50 1.85 BD+62deg 2029 54 A2 10.95 0.97 0.58 55 A0 12.52 0.30 -0.05 56 F8 11.80 0.53 -0.03 57 M2III 9.05 1.68 1.98 BD+62deg 2031 58 B6 10.85 0.14 -0.42 59 B6 11.33 0.13 -0.29 60 A0 12.43 0.18 0.16 61 B8 11.42 0.09 0.05 62 F0 11.68 0.39 0.12 63 F0 11.98 0.34 0.28 64 A2 9.88 0.16 0.11 BD+62deg 2035 65 F2 12.60 0.42 0.18 66 F2 9.68 0.39 0.06 BD+62deg 2036 67 K0III 10.03 1.08 1.21 68 G0 11.36 0.57 0.26 69 A0 12.38 0.21 0.08 70 F8 11.71 0.42 -0.02 71 G5 10.89 0.99 1.16 72 A2 10.73 0.16 0.26 BD+62deg 2254 73 G0 11.81 0.39 0.12 74 A0 7.91 0.03 0.07 BD+62deg 2039 75 B4 10.60 0.07 -0.49 76 A5 11.59 0.37 0.16 77 G8 10.20 1.03 1.08 78 B5 9.90 0.04 -0.48 BD+61deg 2263 79 K5V 9.45 1.77 2.43 80 F2 11.26 0.58 0.06 81 F2 11.42 0.35 0.09 82 K0II 10.26 1.42 1.65 83 F8 11.24 0.55 0.07 84 B2 9.28 0.45 -0.01 BD+62deg 2051 85 A0 10.70 0.34 -0.07 86 F8 9.07 0.51 0.01 BD+62deg 2049 87 G8 9.87 0.68 0.12 88 A0 10.50 0.31 0.16 89 A0 11.44 0.40 0.21 90 A0 10.94 0.36 0.29 91 A0 11.09 0.18 0.13 92 K0III 9.25 1.34 1.43 BD+62deg 2041 93 F0 12.37 0.39 0.37 94 F8 11.28 0.52 0.09 95 A2 11.79 0.23 0.21 96 K0III 9.61 0.97 1.16 97 A2 12.34 0.06 0.22 98 A7 11.86 0.20 0.33 99 K0III 10.95 0.95 0.96 100 F8 10.60 0.85 0.34 101 A2 11.89 0.29 0.17 102 G5IV 10.98 0.28 0.44 103 G0V 11.66 0.52 0.17 104 G2V 11.05 0.69 0.15 105 A2 8.38 1.07 0.15 BD+62deg 2030 106 A4 11.74 0.18 0.19 107 A0 10.75 0.11 -0.36 108 G0 11.53 0.16 -0.09 109 K0III 10.91 0.62 0.48 110 G8III 11.03 1.08 0.74 111 dM 10.37 1.55 1.96 112 B3 11.32 0.22 -0.39 BD+62deg 2028 113 K0 5.10 1.55 1.79 114 A0 11.45 0.37 0.19 blend 115 A0 12.57 0.35 -0.14 116 B1 9.61 -0.02 -0.63 BD+62deg 2020 117 G5 10.90 0.43 -0.03 118 F6 11.40 0.59 0.14 119 A2 11.58 0.61 0.24 120 A2 12.02 0.30 0.16 121 A0 11.55 0.15 0.07 122 G5III 8.44 0.63 0.27 BD+62deg 2014 123 F8 11.81 0.77 0.09 124 A0 12.02 0.32 0.09 125 K0III 11.18 1.56 1.19 126 F2 11.53 0.43 0.14 127 A2 11.64 0.16 -0.01 128 A0 13.48 0.83 0.04 129 A0 12.22 0.89 0.38 130 A0 12.79 0.40 0.05 131 F8 10.78 0.47 -0.03 132 A7 9.72 0.36 0.27 BD+62deg 2024 133 K0V 10.50 0.96 0.61 BD+62deg 2026 134 G5V 9.79 0.90 0.69 BD+62deg 2028 135 F8 11.34 0.52 0.11 136 A0 10.22 0.21 -0.03 137 A2 12.01 0.38 0.19 138 G0 11.88 0.45 0.18 139 A2 10.72 0.30 0.21 140 Me 12.13 1.41 1.19 141 A4 12.05 0.49 0.32 142 F8 10.51 0.53 -0.01 143 A0 11.82 0.29 0.12 blend 144 F8 12.00 0.41 0.04 145 A5 10.14 0.24 0.33 146 G0 10.34 0.47 0.12 147 A4 11.82 0.31 0.15 148 A0 10.54 0.18 -0.04 blend 149 F2 12.59 0.52 0.24 150 A0 11.27 0.14 0.32 151 A0 12.00 0.07 0.06 152 G0 11.18 0.43 0.15 153 B7 10.50 0.11 -0.35 154 F0 11.47 0.28 0.12 155 B3e 10.64 0.28 -0.40 156 G8III 9.30 1.30 0.89 BD+62deg 2050 157 M 5.57 1.67 1.99 BD+62deg 2048 158 F0 8.66 0.36 0.13 BD+62deg 2044 159 A0 10.83 0.40 0.31 160 B2 7.37 0.06 -0.52 BD+62deg 2045 161 A0 10.55 0.25 0.20 162 K0III 7.59 0.97 1.01 BD+62deg 2047 163 A2 10.38 0.29 0.25 164 B6 8.79 0.14 -0.48 BD+62deg 2042 165 B3 9.95 0.25 -0.41 BD+62deg 2043 166 Ap 10.88 0.34 0.15 167 M 9.06 1.55 2.05 BD+63deg 1817 168 A0 11.53 0.46 0.09 169 A0 11.59 0.03 0.19 170 A5 11.07 0.59 0.35 171 K2III 10.58 1.48 1.48 172 B6 10.35 0.17 -0.33 173 B7 9.93 0.18 -0.22 BD+62deg 2035 174 K2III 10.18 1.25 1.34 175 F0 11.00 0.31 0.09 176 A7 11.36 0.31 0.21 177 A7 10.80 0.34 0.09 BD+62deg 2033 178 A4 10.08 0.26 -0.02 BD+62deg 2034 179 K2III 8.99 1.43 1.74 BD+62deg 2037 180 A2 10.58 0.54 0.09 181 F2 12.86 0.76 0.02 182 A5 11.96 0.36 0.21 183 A0 11.17 0.19 0.01 184 B1 7.99 0.29 -0.61 BD+63deg 1807 185 G0V 11.57 0.65 0.15 186 A0 11.74 0.26 0.01 187 F2 12.06 0.60 0.00 188 dK 9.29 1.06 0.73 BD+63deg 1806, blend 189 K3V 9.93 1.83 1.93 190 gG5 6.81 0.87 0.53 BD+62deg 2032 191 A4 10.92 0.29 0.09 192 A2 11.47 0.22 0.08 193 A0 11.33 0.20 -0.23 194 B6 9.63 0.00 -0.55 BD+62deg 2025 195 B6 9.02 -0.05 -0.48 BD+62deg 2023 196 A7 9.45 0.21 -0.12 BD+62deg 2022 197 A0 9.23 0.03 0.01 BD+62deg 2027 198 F0 10.63 0.33 0.09 199 A2 11.49 0.22 0.27 200 K0III 9.06 1.07 0.81 BD+62deg 2019 201 A2 9.98 0.16 -0.14 202 K5III 8.39 1.76 2.19 BD+62deg 2018 203 F0 9.79 0.24 0.06 BD+62deg 2017 204 F0 11.54 0.32 0.06 205 A0 11.92 0.37 0.16 206 A2 10.89 0.36 -0.01 207 G0III 10.72 0.60 0.06 208 A7 11.73 0.34 0.07 209 A2 12.04 0.48 0.02 210 A0 12.36 0.00 0.08 211 F2 9.49 0.31 -0.04 BD+63deg 1803 212 F4 10.32 0.45 -0.31 213 G0III 10.38 0.62 -0.18 BD+63deg 1805 214 B8 10.80 0.28 -0.01 215 G8V 11.68 0.55 0.28 216 B0 11.06 0.18 -0.86 217 A0 11.41 0.26 0.11 218 A0 11.45 0.17 -0.03 219 A0 10.78 0.32 -0.34 220 A0 11.58 0.12 -0.32 221 A5 9.09 0.18 -0.14 BD+63deg 1809 222 A2 9.74 0.29 -0.10 BD+63deg 1810 223 A3 8.57 0.29 -0.64 BD+63deg 1814, blend 224 K0III 8.13 1.03 0.88 BD+63deg 1812 225 F2 11.61 0.60 0.14 226 G8III 10.79 0.66 0.03 BD+63deg 1804 227 A2 11.52 0.26 0.17 228 G8 11.64 0.97 0.23 229 G5 11.86 0.51 -0.12 230 dG 11.73 0.59 0.16 231 F2 12.04 0.92 0.34 blend 232 A4 10.21 0.33 0.09 BD+63deg 1801 233 A0 12.64 0.38 0.18 234 F0 12.34 0.70 -0.02 235 F5 10.10 0.40 -0.08 BD+63deg 1799 236 A0 9.46 0.13 0.01 BD+63deg 1797 237 F8 12.10 0.47 -0.21 238 A2 12.25 0.47 0.17 239 A0 12.85 0.45 -0.06 240 G0 10.65 0.58 0.14 241 F8 11.7 0.63 0.04 242 F0 9.91 0.60 0.26 BD+63deg 1796 243 K0III 10.18 1.24 0.85 244 A0 12.17 0.52 0.08 245 G0 11.51 1.14 0.08 246 A5 12.40 0.69 0.09 247 A0 12.01 0.36 -0.17 248 K0III 8.11 0.95 0.75 BD+63deg 1800 249 F0 11.30 0.41 -0.13 250 F5 11.20 0.55 -0.28 251 A2 11.76 0.35 0.05 252 K0III 10.77 1.26 1.15 253 A0 11.90 0.28 -0.10 254 B6 10.11 0.34 -0.49 255 F0 11.24 0.73 0.03 256 A0 11.93 0.42 -0.07 257 A0 12.84 0.53 0.09 258 K0III 10.12 0.98 0.52 259 A7 11.14 0.56 0.11 260 A5 12.10 0.52 -0.22 261 K0V 11.63 1.13 0.62 262 F8 11.94 0.56 0.13 263 A0 11.81 0.17 0.23 264 F5 11.25 0.56 -0.19 265 G8III 10.06 1.12 0.68 266 B8 11.03 0.11 -0.38 267 G8III 10.92 0.99 0.66 268 F5 11.68 0.44 0.01 269 K0III 10.66 1.12 0.95 270 B8 10.75 0.36 0.22 271 B8 10.99 0.96 0.62 272 B6 10.26 -0.02 -0.57 BD+63deg 1795 273 B5 8.49 0.19 -0.54 BD+63deg 1794 274 K0III 10.05 1.16 0.83 275 B6 10.80 0.18 -0.7 276 F8 10.53 0.49 -0.22 blend 277 B7 11.75 0.80 0.19 278 A0 12.33 0.46 -0.07 279 M 10.51 1.65 2.24 280 B5 9.57 0.23 -0.57 281 dG 11.77 0.78 0.17 282 F8 11.46 0.64 -0.19 283 A0 12.13 0.62 0.03 284 F8 11.80 0.57 -0.16 285 A2 11.98 0.52 -0.05 286 K5I-II 11.48 1.15 0.99 287 A0 12.30 0.31 -0.01 288 B7 10.81 0.29 -0.43 289 K2 10.96 1.44 0.98 290 K0 9.00 1.55 1.41 BD+63deg 1789 291 A0 12.08 0.30 0.00 292 A2 11.74 0.29 -0.34 293 A0 11.02 0.38 -0.12 294 A7 12.07 0.46 -0.03 295 B8 11.70 0.25 -0.31 296 F8 11.51 0.46 -0.02 297 G0III 9.35 0.74 0.18 BD+63deg 1786 298 G0V 9.23 1.10 0.73 BD+63deg 1785 299 G8V 11.68 0.58 0.19 300 K0III 10.77 1.20 0.76 301 K0III-IV 9.50 1.50 1.63 BD+63deg 1787 302 A0 12.36 0.46 0.23 303 F5 10.97 1.28 1.12 304 G0 11.65 0.48 0.11 305 A0 11.50 0.12 -0.25 306 G2III 9.30 0.87 0.39 BD+63deg 1791 307 F8 11.06 0.57 -0.12 308 K0III 8.63 0.58 -0.20 BD+63deg 1792 309 G0V 11.57 0.56 -0.08 310 F8 11.97 0.48 -0.23 311 A0 11.12 0.04 -0.11 312 A0 12.19 0.34 -0.25 313 A0 12.47 0.48 -0.08 314 A0 12.77 0.43 0.03 315 A2 9.54 0.08 -0.38 BD+63deg 1793 316 F8 12.34 0.38 -0.25 317 A2 9.21 0.20 -0.14 BD+63deg 1610 318 G8V 10.75 0.90 0.39 319 A6 12.34 0.62 0.14 320 A0 12.36 0.36 0.02 321 G3V 11.15 1.26 0.29 322 F8 10.92 0.47 -0.15 323 G5III 10.85 1.07 0.54 324 F8 10.73 0.28 -0.05 325 A7 10.30 0.03 -0.02 BD+63deg 1605 326 A2 11.62 0.21 -0.04 327 K0III 10.21 0.95 0.70 328 A0 11.96 0.22 0.21 329 A0 11.57 0.32 0.05 330 A5 11.41 0.49 0.14 331 A0 12.57 0.32 0.07 332 A0 11.73 0.20 -0.26 333 F6 11.88 0.51 -0.26 334 F8 11.36 1.01 0.80 335 G8III 7.57 0.82 0.60 BD+64deg 1599 336 K0III 9.41 1.17 1.02 BD+63deg 1778 337 F8 11.05 0.32 -0.26 338 A0 11.17 0.20 0.32 339 K0III 10.21 1.00 0.67 BD+63deg 1776 340 F8 11.57 0.46 -0.01 341 F4 11.60 0.62 -0.08 342 G5V 11.37 0.66 0.10 343 F4 11.31 0.75 -0.17 344 A0 12.14 0.51 -0.01 345 A5 12.50 0.72 -0.16 346 K0III 9.79 1.13 0.85 347 G2 10.02 0.41 -0.19 348 A0 11.86 0.24 -0.03 349 F8 11.70 0.63 -0.07 350 K0IV 10.26 1.46 1.39 351 B8 11.02 0.16 -0.20 352 K0III 10.98 1.07 0.57 353 G0 10.34 0.55 -0.13 354 F8 12.06 0.67 -0.19 355 B8 11.03 0.25 -0.33 356 K0III 11.46 1.16 0.78 357 A0 12.82 0.79 0.09 358 A2 11.37 0.38 0.00 359 K2III 8.35 1.62 1.67 BD+63deg 1780 360 F2 11.97 0.55 -0.26 361 G0 11.93 0.58 -0.12 362 G 10.55 0.77 0.06 blend 363 K0V 11.09 1.09 1.03 364 F0 10.42 0.50 -0.02 BD+63deg 1781 365 A0 11.86 0.64 0.09 366 B6 10.45 0.40 -0.13 367 F8 10.86 0.55 -0.13 368 F6 11.21 0.23 0.00 369 A2 11.78 0.47 0.15 370 F2 11.72 0.49 0.07 371 F8 11.41 0.64 -0.01 372 F2 11.41 0.47 -0.16 373 A2 12.37 0.28 -0.01 374 A0 11.98 0.24 0.09 375 G8III 11.22 1.33 0.49 376 A0 11.15 0.49 0.17 377 K0III 11.22 0.93 0.72 378 K0II 10.00 1.24 1.15 379 F0 10.38 0.43 -0.03 BD+63deg 1786 380 F4 10.50 0.59 -0.16 381 B2 8.19 0.10 -0.66 BD+63deg 1779 382 F8 12.25 0.77 -0.25 383 F8 11.78 0.88 0.08 blend 384 A0 11.73 0.73 0.25 385 A0 11.61 0.39 0.11 386 A0 10.47 0.52 0.09 387 F5 12.55 0.46 -0.14 388 A0 9.64 0.40 0.03 BD+63deg 1777 389 A0 11.95 0.27 0.14 390 G2III 11.42 0.71 0.13 391 K2III 10.53 1.25 1.12 392 K0III 9.44 1.43 1.34 BD+63deg 1775 393 A0 11.46 0.32 -0.01 394 A0 12.21 0.59 0.10 395 K0III 10.02 1.03 0.76 BD+63deg 1774 396 A0 12.03 0.19 0.12 397 G5V 11.72 0.59 -0.04 398 A0 12.09 0.55 0.09 399 F6 10.54 0.49 -0.17 400 A5 11.18 0.30 0.06 401 G8III 10.85 0.88 0.78 402 F8 11.39 0.62 0.04 403 F8 11.29 0.65 -0.05 404 K0III 10.40 1.39 1.30 405 A0 12.45 0.22 0.25 406 A0 11.56 0.43 -0.06 407 A2 12.37 0.38 -0.10 408 K2III 10.66 1.52 1.29 409 A0 12.04 0.33 0.02 410 A0 11.48 0.30 0.16 411 F8 11.85 0.75 0.12 412 A2 12.08 0.25 0.18 413 A6 12.39 0.31 0.27 414 A0 12.32 0.77 0.15 415 G8V 11.36 0.70 0.18 416 A4 11.18 0.49 0.02 417 F0 12.31 0.50 0.03 418 F6 11.23 0.46 -0.21 419 F6 11.39 0.48 -0.13 420 A2 11.49 0.37 -0.21 421 G5III 10.44 1.44 1.25 422 K0V 11.38 0.95 0.69 424 A0 12.27 0.73 0.05 425 F5 10.14 0.60 -0.25 BD+63deg 1782 426 A0 12.11 0.53 0.12 427 B7 7.73 -0.03 -0.31 BD+63deg 1784 428 A0 12.39 0.38 0.07 429 F5 11.25 0.44 -0.26 430 A0 11.78 0.34 0.00 431 A2 9.57 0.12 -0.20 432 A4 10.62 0.41 0.04 433 G8 10.06 1.16 0.77 434 K0V 11.12 1.19 0.99 435 B7 10.29 0.25 -0.30 BD+62deg 2005 436 B7 9.80 0.23 -0.30 437 G2 11.22 0.24 0.36 438 A0 12.40 0.44 0.03 439 A2 11.96 0.65 0.30 440 A0 12.03 0.68 0.07 441 A7 10.95 0.68 0.13 442 A0 11.55 0.24 0.17 blend 443 M2Ib+B8Ve 4.78 1.96 0.30 BD+62deg 2007 444 A0 9.10 0.11 -0.71 BD+63deg 1788 445 K0III 10.62 1.29 1.09 446 K0III 10.50 1.13 0.58 447 F8 11.64 0.70 -0.07 448 K5III 8.78 1.55 1.44 BD+63deg 1790 449 K0III 10.78 1.33 1.17 450 A2 11.65 0.18 -0.23 451 G8V 12.15 0.71 0.00 452 G2III 9.93 0.75 0.27 453 F8 10.23 0.50 -0.16 454 A0 12.58 0.37 0.07 455 A0 12.11 0.29 -0.27 456 F2 12.75 0.50 0.21 457 B6 10.22 0.15 -0.67 458 A0 10.63 0.55 -0.21 459 B8 11.34 0.21 -0.52 460 A0 12.03 0.35 -0.10 461 A0 12.23 0.41 0.11 462 F8 10.52 0.46 -0.28 463 G8V 11.85 0.83 0.39 464 A0 11.66 0.34 0.12 465 A0 11.12 0.03 -0.38 466 K5III 10.71 1.44 1.68 467 A0 12.29 0.31 0.13 468 K0III 10.53 1.21 0.85 469 dM 10.01 1.85 2.21 470 F0 10.45 0.33 -0.01 471 A0 11.40 0.57 0.15 472 F8 10.35 0.90 -0.07 473 F5 10.49 0.40 -0.09 474 A2 8.71 0.06 -0.20 BD+62deg 2012 475 A0 13.20 0.32 0.19 476 F8 11.23 0.66 -0.09 477 F8 11.77 0.48 -0.09 478 A0 13.07 0.49 -0.03 479 A0 13.06 0.63 0.12 480 B7 9.21 0.11 -0.36 BD+62deg 2009, blend 481 F2 7.19 0.63 0.07 BD+62deg 2004 482 A0 13.07 0.52 0.18 483 F0 11.77 0.45 0.00 484 A0 12.94 0.29 0.05 485 A0 12.23 0.38 0.01 486 K2V 9.40 1.70 2.02 BD+62deg 2000 487 F6 11.34 0.43 -0.22 488 F6 11.55 0.71 0.14 489 A6 12.49 0.41 -0.12 490 A4 12.60 0.34 0.06 491 A2 10.99 0.35 0.09: 492 B5 10.05 0.15 -0.90: 493 A0 11.88 0.47 -0.28 494 F0 11.90 0.58 -0.18 495 K0I-II 9.21 1.47 1.22 496 A0 12.69 0.58 0.22 497 F0 11.47 0.57 -0.16 498 A0 12.91 0.72 0.15 499 A0 12.59 0.67 0.19 500 G5IV 10.38 1.13 0.57 501 F2 11.90 0.51 -0.26 502 A0 11.83 0.12 -0.13 503 A0 12.84 0.31 -0.15 504 F5 12.21 0.73 0.28 505 F2 10.68 0.61 -0.28 506 K0III 9.04 1.05 0.55 BD+62deg 1983 507 F0 12.85 0.44 0.13 508 A2 11.81 0.43 0.15 509 F2 10.92 0.40 -0.27: BD+62deg 1984 510 G5III 10.06 1.64 1.69 BD+62deg 1987 511 A0 12.93 0.38 0.19: 512 A0 12.31 0.56 0.02: 513 A2 11.46 0.40 0.15: 514 A2 10.54 0.76 0.17: BD+62deg 1982 515 F8 10.84 0.36 -0.18: 516 A0 11.60 0.45 0.29: 517 A2 11.35 0.18 -0.44: 518 K0III 10.15 1.36 0.71 BD+62deg 1980 519 A0 11.52 0.27 -0.17 520 A0 11.64 0.13 -0.08 521 F6 11.56 0.44 -0.19 522 A6 11.09 0.27 0.13 523 A0 11.89 0.28 0.03 524 A2 11.73 0.38 0.14 525 A4 12.09 0.69 0.08 526 F0 11.90 0.52 0.02 527 A0 11.06 0.42 0.07: 528 A0 11.69 0.08 -0.15: 529 A0 12.40 0.24 -0.03 530 A0 12.40 0.59 0.20 531 A7 11.98 0.58 0.20 blend 532 dK 10.88 1.71 2.10 533 F8 9.58 0.61 -0.13 BD+62deg 1981 534 A2 12.07 0.26 0.00 535 G0 10.17 0.07 -0.11: 536 A0 12.64 0.19 -0.07 537 A0 11.15 0.09 -0.22: 538 F0 10.83 0.42 0.11 BD+62deg 1990 539 A0 11.82 0.21 0.11 540 F8 11.08 0.61 0.11 BD+62deg 1991 541 F0 12.11 0.49 0.19: 542 A2 11.56 0.09 0.11 543 B3 7.42 0.09 -0.78 BD+62deg 1992 544 F8 10.26 0.45 -0.17 BD+62deg 1991 545 A0 11.25 0.38 0.05 546 F5 10.61 0.40 -0.20 BD+62deg 1996 547 A2 11.68 0.23 0.06 548 K0III 9.55 1.09 0.76 BD+62deg 1997 549 K0III 9.43 1.05 0.73 BD+62deg 1998 550 A7 10.34 0.30 -0.13 BD+62deg 2001 551 K2III 8.17 1.85 1.98 BD+62deg 1999 552 F8 12.43 0.74 0.32 553 A0 11.81 0.67 0.27 554 F8 11.23 0.56 0.01 555 A5 12.22 0.22 0.09 556 F8 11.39 0.55 -0.02 557 F0 12.26 0.29 0.00 558 A0 11.60 0.36 0.03 559 K0III 10.25 1.36 1.57 560 F8 11.43 0.61 -0.19 561 F0 10.37 0.26 0.17 BD+62deg 2003 562 A7 11.88 0.25 0.31 563 G0 11.81 0.49 0.04 564 A0 10.70 0.11 -0.28 565 B7 10.75 0.12 0.06 566 B3 9.85 0.03 -0.53 BD+62deg 2002 567 dM 10.88 1.79 1.77 568 B0 7.77 -0.16 -0.73 BD+62deg 2006 569 F8 11.59 0.60 0.03 570 F0 10.92 0.36 0.09 571 A7 9.86 0.17 -0.02 572 A2 11.50 0.37 0.17 573 B8 12.09 0.75 -0.15: edge of plates 574 F0 12.53 0.35 0.24 575 F4 13.40 0.92 0.27 576 A7 11.64 0.44 0.22 577 A0 12.20 0.29 0.00 578 A0 12.74 0.60 0.14 579 G2III 9.69 1.29 1.34 BD+62deg 2011 580 F4 11.19 0.97 0.39 581 A0 12.12 0.58 0.01 582 G2V 11.63 1.34 1.16 583 K0III 9.08 0.81 1.06: BD+62deg 2013 584 K0III 9.99 1.11 0.85 585 M 5.76 1.74 1.90 BD+62deg 2010 586 F8 11.40 0.57 -0.05 587 F0 10.83 0.34 0.13 588 A0 12.41 0.59 0.16 589 F8 11.82 0.57 0.06 590 A0 9.73 0.19 -0.03 BD+62deg 2008 591 F8 12.07 0.77 0.23 592 A0 12.80 0.42 0.26 593 B8 11.19 0.16 0.07 BD+61deg 2223 594 A2 11.34 0.35 0.34 595 A4 11.88 0.42 0.29 596 A2 10.17 0.29 0.49 597 A0 9.76 0.17 -0.11 BD+61deg 2222 598 F8 11.01 0.75 0.22 599 A4 11.38 0.55 0.28 600 A0 12.36 0.63 0.30 601 B7 11.44 0.19 0.00 602 A0 12.57 0.61 0.28 603 A0 12.65 0.41 0.40 604' A0 11.52 0.36 0.23 605 K0III 11.22 1.43 1.29 606' A0 12.14 0.34 0.42 607' A0 11.62 0.46 0.53 608 A0 10.97 0.11 -0.18 609' A0 12.24 0.39 0.28 610' B7 12.07 0.34 0.28 611 A2 13.02 0.41 0.31 612 F2 11.39 0.54 0.06 613' A0 12.39 0.46 0.39 614' A0 12.53 0.46 0.38 615' B1 6.69 0.24 -0.57 BD+62deg 1994 616 F8 11.73 0.20 0.00 617 G5III 10.85 1.04 0.99 618 A7 10.50 0.26 0.28 619 F8 12.03 0.63 0.36 620 A2 11.49 0.48 0.36 621 F5 9.53 0.32 -0.06 BD+62deg 1986 622 F8 9.51 0.50 0.17 BD+62deg 1985 623 K0III 11.25 1.44 1.22 624 A0 12.29 0.20 -0.09 625 F6 10.91 0.40 -0.04 626 A0 12.05 0.50 0.18 627 A0 11.91 0.37 0.36 628 F8 11.43 0.59 -0.04 629 A0 11.32 0.39 0.09 630 F8 9.10 0.41 -0.19 BD+61deg 2203 631 F2 12.21 0.75 -0.12 632 B7 12.84 0.52 -0.23 633 G8V 11.62 0.76 0.60 634 M2III 10.33 1.76 2.41 635 A7 11.96 0.42 0.25 636 F5 11.93 0.68 0.26 blend 637 A5 10.52 0.19 0.00 638 B8 10.40 1.14 1.21 639 K2III 10.57 1.44 2.23 640 A2 11.23 0.32 0.17 641 F8 11.83 0.63 0.23 642 F2 11.07 0.71 0.35: blend 643 A0 12.53 0.43 0.24 644 F8 10.86 0.57 -0.13: blend 645 F5 10.68 0.32 -0.09 646 M2V 11.32 1.43 1.22 647 F2 10.82 0.55 0.29 648 B7 10.59 0.28 -0.20 649 A0 9.74 0.14 -0.05 BD+61deg 2201 650 F0 9.29 0.32 0.11 BD+61deg 2206, blend 651 A2 11.58 0.48 0.23 652 F0 11.37 0.72 0.29 653 dM 12.15 1.80 0.64 654 A2 12.40 0.88 0.08 655 B8 9.73 0.07 -0.03 BD+61deg 2197 656 F6 10.53 0.42 -0.07 657 A4 11.89 0.78 0.34 658 F8 11.76 0.76 0.07 659 K2V 18.91 2.50 2.03 BD+62deg 1977 660 F8 12.15 0.38 0.45 661 A0 12.60 0.36 0.18 662 F8 12.13 0.56 0.12 663 A2 12.18 0.28 0.15 664 A2 12.06 0.26 0.24 665 A0 12.64 0.40 0.00 666 F2 9.27 0.26 -0.06 BD+62deg 1978 667 F2 11.07 0.54 0.14 668 A0 12.16 0.30 -0.20 669 F6 11.00 0.46 -0.02 670 A0 12.01 0.18 0.06 671 F8 11.72 0.75 0.07 672 F6 12.15 0.68 0.00 673 F5 11.54 0.39 -0.02 674 F8 11.13 0.84 0.41 675 G2V 10.81 1.06 0.37 676 A0 12.49 0.50 -0.10 677 A0 13.28 0.42 0.26 678 A0 12.16 0.34 0.23 679 A2 11.80 0.60 0.28 680 A0 12.81 0.45 0.22 681 B8 11.89 0.12 0.07 682 A4 11.51 0.23 -0.29 683 F8 11.78 0.75 0.24 684 K0V 11.17 1.29 1.26 685 dG 13.04 0.60 0.19 686 F5 11.33 0.45 -0.10 687 F8 12.08 0.44 -0.13 688 F4 11.98 0.52 0.02 689 F8 11.19 0.91 0.28 690 dM 10.19 1.81 1.95 691 F0 11.86 0.43 -0.01 692 G8III 11.23 1.18 0.77 693 K0V 10.44 1.14 1.21 694 A0 12.32 0.26 0.07 695 F2 11.38 0.65 0.20 696 G0 11.03 0.34 0.03 697 F8 9.82 0.34 -0.20 BD+63deg 1773 698 G8III 11.31 0.97 0.77 699 F8 11.50 0.48 -0.07 700 F8 10.66 0.38 -0.18 701 A2 11.32 0.28 0.04 702 F5 11.51 0.92 0.14 703 A0 12.14 0.34 0.17 704 A2 9.16 0.20 0.14 BD+63deg 1769 705 A4 12.04 0.32 0.01 706 A2 9.77 0.10 -0.24 BD+63deg 1765 707 K2III 8.91 1.36 1.50 BD+63deg 1763 708 A7 10.33 0.31 0.17 BD+63deg 1762 709 F0 11.63 0.49 -0.13 710 K0III 8.54 1.50 1.44 BD+63deg 1761 711 A7 10.41 0.22 0.24 BD+63deg 1760, blend 712 A0 11.76 0.50 0.17 713 F5 10.94 0.70 0.07 714 K0III 11.11 1.15 1.08 715 F5 11.74 0.39 -0.06 716 F0 12.31 0.49 -0.34 717 F6 11.90 0.40 -0.13 718 K0V 11.25 0.83 0.65 719 F2 8.31 0.21 -0.11 BD+63deg 1768 720 K2III 9.85 1.08 1.01 BD+63deg 1767 721 F0 11.05 0.56 -0.07 722 A0 11.37 0.05 -0.39 723 K2III 9.97 1.36 1.24 724 F0 11.37 0.50 -0.05 725 A0 12.21 0.43 0.11 726 A0 11.05 0.20 0.14 727 F6 11.08 0.37 -0.01 728 dK 11.89 1.39 0.92 729 G0 11.91 0.68 0.08 730 G2 10.18 0.58 0.07 731 F8 11.41 0.56 0.09 732 K2 10.31 1.43 1.92 733 B5 10.61 0.16 0.04 734 A4 9.19 0.13 0.04 BD+63deg 1755 735 K0III 11.22 1.12 1.49 736 A5 10.78 0.29 0.15 737 A0 10.02 0.11 -0.61 BD+63deg 1757 738 B3 12.40 0.73 0.05 739 F6 10.85 0.03 -0.47 740 F6 11.77 0.46 -0.04 741 G8V 11.77 0.61 -0.06 742 F8 11.56 0.44 -0.13 743 K0III 10.81 1.46 1.22 744 K0III 11.10 1.03 0.80 745 A2 11.51 0.41 0.35 746 F5 6.95 0.45 -0.23 BD+63deg 1764 747 A2 12.12 0.52 0.00 748 A2 11.87 0.30 0.19 749 F5 8.16 0.30 -0.02 BD+62deg 1975 750 B8 11.55 0.23 -0.17 751 G5 11.26 1.19 0.87 752 A2 12.20 0.52 0.20 753 F5 11.03 0.61 0.25 754 F8 11.47 0.54 0.07 755 A5 12.65 0.68 0.25 756 F5 11.46 0.61 0.29 757 G5V 11.10 0.72 0.30 758 A0 11.58 0.33 0.24 759 F2 11.99 0.56 0.27 760 G0V 11.15 0.76 0.02 761 gK 11.11 1.34 1.43 762 A0 12.83 0.71 0.31 763 F8 11.68 0.56 0.00 764 G2 10.56 0.72 0.42: 765 K5III 10.23 1.76 1.93 766 F8 10.46 0.60 0.04 767 A0 11.43 0.24 0.18 768 K0III 9.94 1.18 1.09 BD+62deg 1960 769 B7 11.21 0.17 -0.03 770 G0 10.76 0.82 0.24 771 K2V 10.63 1.45 1.25 772 A0 12.70 0.17 0.28 773 B2 8.09 0.06 0.01 BD+63deg 1753 774 A0 12.02 0.68 0.29 775 A0 12.75 0.56 0.43 776 A0 13.23 0.49 0.32 777 G8III 10.54 0.62 -0.08 778 F0 12.12 0.77 0.38 779 K2III 10.32 1.65 1.68 780 A2 12.00 0.44 0.18 781 F6 9.14 0.31 0.09 BD+62deg 1959 782 F5 11.07 0.60 -0.04 783 F2 11.24 0.65 0.26 784 A0 12.71 0.38 0.23 785 dK 12.59 0.89 0.27 786 K2III 8.57 1.82 2.49 787 A0 11.96 0.44 -0.28 788 G0 9.81 0.52 0.13 BD+62deg 1962 789 F8 10.78 0.60 0.22 790 K2 8.95 0.95 0.79 BD+62deg 1963 791 A0 11.25 0.30 -0.17 792 G0 10.33 0.68 0.10 793 A2 11.03 0.43 0.20 794 G0 11.29 0.65 -0.03 795 G8 10.73 1.18 1.07 796 G 12.31 0.63 0.10 797 A4 9.91 0.14 -0.42 BD+62deg 1968 798 F6 8.96 0.34 -0.07 BD+62deg 1969 799 K5III 9.59 1.84 2.04 BD+62deg 1972 800 G8III 11.39 0.81 0.39 801 K2III 10.63 1.37 1.18 802 K0 9.46 0.90 0.93 BD+62deg 1971 803 A0 12.12 0.31 0.06 804 F8 11.58 0.60 0.20 805 F4 11.35 0.40 -0.13 806 K2III 11.29 1.32 0.86 807 A2 12.42 0.35 0.22 808 B6 9.36 0.04 -0.20 BD+62deg 1967, blend 809 A2 9.62 0.36 0.21 BD+62deg 1964 810 A2 12.01 0.27 0.06 811 A0 12.55 0.50 0.24 812 F0 10.15 0.28 -0.09 BD+62deg 1966 813 F8 11.22 0.52 0.07 814 F0 12.30 0.58 0.12 815 A0 12.43 0.30 0.09 816 A0 12.30 0.37 0.31 817 A0 11.66 0.18 -0.31 818 G0 11.77 0.70 0.23 819 gK 10.20 1.82 2.15 820 A0 10.82 0.21 -0.21 821 F5 11.11 0.57 0.08 822 F6 11.03 0.54 0.01 823 A0 12.98 0.44 0.14 824 A0 11.97 0.39 0.18 825 F2 10.78 0.73 0.34 826 A2 11.07 0.50 0.53 827 A5 12.57 0.86 0.53 828 F0 12.15 0.61 0.42 829 A2 11.61 0.46 0.02 830 F0 9.27 0.35 0.03: BD+62deg 1957 831 A0 12.09 0.57 0.57 832 A0 12.37 0.14 0.21 833 G5V 11.13 0.62 0.35 834 K2III 8.88 1.56 1.95 BD+61deg 2157 835 A0 12.10 0.37 0.43 836 A0 11.45 0.48 0.42 837 B5 10.42 0.09 -0.46 BD+61deg 2161 838 F5 9.86 0.51 0.07 BD+61deg 2162 839 A2 12.45 0.42 0.42 840 F8 13.43 0.86 0.31 841 F6 10.65 0.51 0.04 842 F6 12.00 0.55 -0.04 843 B5 10.50 0.24 -0.46 BD+61deg 2170 844 F8 10.64 0.37 0.12 BD+61deg 2173 845 K2III 9.96 1.07 1.19 BD+61deg 2174 846 A0 13.09 0.33 -0.31 847 A0 12.60 0.30 0.18 848 A2 11.12 0.32 -0.15 849 F8 11.83 0.78 0.12 850 F4 11.17 0.43 -0.05 851 F2 11.43 0.74 0.30 852 dM 10.33 1.60 0.93 853 B8 10.19 0.26 -0.25 854 A2 11.48 0.51 0.26 855 A0 12.55 0.85 0.15 856 F6 11.46 0.60 0.09 857 A2 11.62 0.28 0.13 858 F0 10.48 0.38 0.04 859 G8V 11.78 0.59 0.22 860 K2III 10.97 1.31 1.28 861 B5 10.97 0.48 -0.03 862 A2 10.97 0.23 -0.12 863 G2 11.62 0.66 0.04 864 A0 12.24 0.46 -0.02 865 B5 8.76 0.10 -0.70 BD+62deg 1973 866 F0 8.41 0.14 -0.06 BD+62deg 1976 867 G0 12.14 0.82 0.06 868 A5 10.43 0.47 -0.04 869 F5 8.32 0.34 -0.26 BD+61deg 2188 870 B8 11.79 0.14 -0.02 871 K2III 8.94 1.77 2.15 BD+61deg 2120 872 A5 11.39 0.55 0.10 873 B2 5.87 0.32 -0.60 BD+61deg 2193, blend 874 gK 11.84 1.53 0.99 875 F8 12.00 0.58 -0.12 876 F5 11.11 0.75 0.51 877 F4 11.86 0.73 0.18 878 F6 9.20 0.45 0.00 879 F6 10.86 0.49 -0.10 880 A0 12.26 0.57 0.25 881 F8 11.76 0.29 0.09 882 K0III-IV 9.89 1.00 0.60 BD+61deg 2189 883 F2 11.03 0.43 0.02 884 A2 12.03 0.55 0.08 885 G8 10.58 1.19 0.95 886 A2 11.27 0.14 0.09: 887 A2 10.87 0.29 0.12 888 K2III 9.84 1.21 1.21 BD+61deg 2191 889 A0 12.45 0.39 0.21 890 F0 12.17 0.64 0.22 891 A2 12.08 0.48 0.26 892 F6 9.56 0.40 -0.02 BD+61deg 2187 893 A2 8.35 0.02 0.00 BD+61deg 2185 894 A0 11.79 0.39 0.00 895 K2II-III 8.45 1.45 1.41: BD+61deg 2186 896 A2 12.56 0.50 0.10 897 A0 12.72 0.56 0.28 898 A0 12.53 0.40 0.19 899 A2 12.46 0.45 0.16 900 A0 11.63 0.42 0.22 901 A0 12.02 0.48 0.23 902 gK 11.80 1.71 1.46 903 A0 11.86 0.78 0.38 904 A0 12.20 0.40 0.32 905 A0 12.44 0.62 0.33 906 A0 9.66 0.10 -0.05 BD+61deg 2182 907 K0V 11.72 0.65 0.45 908 A2 12.42 0.38 0.16 909 A0 12.25 0.50 0.23 910 F5 10.76 0.67 0.19 911 A0 10.60 0.20 -0.36 912 A0 11.92 0.20 -0.04 913 B5 10.59 0.18 -0.55 BD+61deg 2178 914 F0 12.94 0.42 0.17 915 F8 12.30 0.67 0.23 916 A0 12.47 0.62 0.51: 917 F5 11.27 0.68 0.31 918 G2III 7.11 0.91 0.71 BD+61deg 2166 919 A0 13.52 0.39 0.49 920 dK 10.43 1.39 1.48 921 A2 10.07 0.33 0.24 922 A0 12.75 0.56 0.52 923 A0 11.39 0.37 0.27 924 A7 9.33 0.51 -0.36 BD+61deg 2163 925 G2 11.54 0.34 -0.04 926 F8 10.53 0.46 0.08 BD+61deg 2164 927 A0 12.56 0.55 0.65 928 A0 12.18 0.84 0.38 929 F5 10.08 0.32 0.05 930 A0 12.52 0.60 0.39 931 A0 12.82 0.63 0.13 932 A0 12.44 0.38 0.14 933 F0 9.92 0.19 0.16 BD+61deg 2165 934 A2 12.20 0.10 0.08 935 F5 8.98 0.30 0.03 BD+61deg 2274 936 F5 11.72 0.52 -0.16 937 A0 9.87 0.12 0.00 BD+60deg 2273 938 G8III 11.32 0.92 0.57 939 B7 11.38 0.27 0.10 940 A0 12.43 0.87 0.06 941 A0 12.49 0.52 0.02 942 F8 10.64 0.48 -0.34 943 A0 12.05 0.16 -0.21 944 A0 11.81 0.36 0.16 945 A0 11.33 0.44 -0.05 946 F0 10.53 0.37 -0.30 947 A0 11.45 0.53 -0.01 948 A7 8.81 0.05 -0.57 BD+60deg 2276 949 F8 10.95 0.59 -0.34 950 A0 12.40 0.45 -0.01 951 A0 12.81 0.43 0.18 952 gK 11.49 1.93 2.08 953 A0 13.45 0.69 0.05: 954 A0 12.60 0.73 0.48 955 K0III 9.25 1.15 0.94 BD+61deg 2177 956 F8 11.11 0.60 0.07 957 K2II 8.83 1.28 1.56 BD+61deg 2175 958 A2 11.98 0.35 0.23 959 B8 10.14 0.32 -0.16: 960 F2 11.76 0.51 0.11 961 F2 11.73 1.01 0.26: blend 962 A4 11.50 0.41 0.25 963 F6 9.84 0.41 0.06 BD+61deg 2167 964 B6 10.53 0.12 -0.45 BD+61deg 2168 965 O9II 5.96 0.31 -0.64 BD+61deg 2172 966 A7 11.11 0.37 0.31 967 F2 11.52 0.56 0.13 968 F8 11.31 0.46 0.05 969 A0 12.35 0.62 0.43 970 A0 12.34 0.61 0.42 971 F2 11.68 0.49 0.00 972 dK 11.29 2.26 2.19 973 A2 10.69 0.20 0.10 BD+61deg 2179 974 G2V 11.51 1.02 0.69 975 A0 13.10 0.48 0.26 976 B5 9.79 0.25 -0.32 BD+61deg 2180 977 A0 12.24 0.44 0.44 978 A0 12.26 0.62 0.23 979 F8 10.92 0.72 0.21 980 F0 11.73 0.75 0.18 981 A0 12.36 0.35 0.17 982 A2 11.91 0.26 0.02 983 G8III 9.71 1.12 0.77 BD+61deg 2181 984 F8 11.59 0.60 0.28 985 A5 11.26 0.52 0.40 986 A7 11.32 0.70 0.42 987 F0 12.05 0.73 0.45 988 G0V 10.84 0.42 0.48 989 A2 10.29 0.07 0.19 BD+61deg 2183 990 F5 11.30 0.61 0.16 991 K0III 10.31 1.30 1.08 992 F2 11.71 0.59 0.24 993 G5V 11.86 0.87 0.16 994 A2 10.07 0.16 0.14 BD+61deg 2184 995 G8III 10.96 1.01 0.61 996 F8 11.43 0.45 -0.02 997 A0 11.51 0.46 0.38 998 F8 11.17 0.63 0.09 999 G0 8.65 0.48 -0.07 BD+61deg 2195 1000 B8 9.17 0.73 0.29 BD+61deg 2198 1001 B8 11.33 0.29 -0.17 1002 A0 10.07 0.21 -0.31: BD+61deg 2196 1003 F5 11.48 0.50 -0.07 1004 K3III 9.23 1.67 2.09 BD+60deg 2287 1005 A2 10.19 0.39 0.26 BD+60deg 2286 1006 A5 11.03 0.56 0.33 1007 A0 12.50 0.58 0.17 1008 A2 11.75 0.54 0.40 1009 G5V 11.98 0.74 0.11 1010 A0 12.03 0.56 0.29 1011 A2 12.11 0.45 0.15 1012 A7 12.53 0.39 0.50 1013 F0 11.94 0.63 0.37 1014 F2 10.33 0.67 0.43 blend 1015 F0 12.14 0.61 0.26 1016 A2 10.83 0.40 0.13: 1017 K2III 11.06 1.61 1.44 1018 F8 11.77 0.58 0.25 1019 A5 8.71 0.22 0.18 BD+60deg 2278 1020 A2 10.70 0.34 0.28 1021 A2 11.49 0.49 0.25 1022 A2 12.44 0.59 0.38 1023 A0 12.60 0.56 0.25 1024 A0 12.80 0.47 0.41 1025 A5 11.92 0.75 0.63 1026 A2 11.90 0.40 0.51 1027 A2 10.97 0.52 0.21 1028 A0 11.32 0.57 0.07 1029 G0 11.12 0.59 0.29 1030 A0 11.67 0.60 0.25 1031 A2 10.48 0.49 -0.01 BD+60deg 2280 1032 G0 10.92 0.75 0.43 1033 A7 10.36 0.45 0.08 BD+60deg 2282 1034 A0 12.77 0.70 0.59 1035 A0 12.84 0.73 -0.05 1036 G0V 10.22 0.69 -0.05 BD+60deg 2281 1037 A2 10.79 0.46 0.52 1038 F8 10.17 0.47 0.13 BD+60deg 2284 1039 F8 11.15 0.75 0.27 1040 F5 11.37 0.52 0.27 1041 A0 12.13 0.62 0.43 1042 A2 12.09 0.60 0.14 1043 F5 10.84 0.54 0.30 1044 A2 12.41 0.81 0.40 1045 A0 12.20 0.49 0.29 1046 G0III 7.31 0.76 0.34 BD+60deg 2285 1047 A7 11.56 0.76 0.69 1048 K0V 11.92 0.82 0.27 1049 F8 12.11 0.74 0.21 1050 A0 11.44 0.64 0.32 1051 A2 10.94 0.73 0.72 1052 A0 11.92 0.49 0.12 1053 A0 11.63 0.54 0.45 1054' A2Ia 4.29 0.52 0.14 BD+60deg 2288 1055 A0 11.63 0.45 -0.01 1056 A0 12.02 0.49 0.36 1057 G0 8.59 0.41 0.14 BD+60deg 2290 1058 A0 12.29 0.46 0.30 1059 B7 9.57 0.53 -0.22 BD+60deg 2289 1060 A7 10.29 0.32 0.18 1061 F6 11.65 0.51 0.06 1062 F5 11.12 0.40 -0.01: 1063 F6 10.93 0.49 0.13: 1064 A0 12.29 0.59 0.24 1065 A0 11.97 0.25 0.20 1066 F6 11.13 0.56 0.13 1067 K2III 9.09 1.18 1.38 BD+60deg 2296 1068 F8 10.14 0.63 0.15 1069 A5 11.54 0.53 0.41 1070 F4 9.31 1.00 0.85 BD+60deg 2297 1071 B0n 11.90 0.37 -0.53 1072 A5 11.75 0.41 0.37 1073 K0III 9.04 1.09 0.90 BD+60deg 2295 1074 F0 9.03 0.33 0.11 BD+60deg 2291 1075 A2 11.14 0.45 0.30 1076 G0 10.17 0.69 0.30 1077 F5 11.59 0.57 0.13 1078 M 5.31 1.61 2.06 BD+60deg 2294 1079 G8V 11.09 0.56 0.24 1080 A0 12.90 0.68 0.39 1081 A0 13.53 0.64 0.34 1082 K5III 9.10 2.03 2.31 BD+60deg 2302 1083 A2 11.20 0.58 0.62 1084 K2III 10.37 1.79 1.36 1085 A0 11.69 0.71 0.15 1086 A0 12.47 0.65 0.38 1087 A0 11.87 0.80 0.22 1088 A0 11.94 0.62 0.55 1089 A5 11.42 0.84 0.73 1090 A0 11.90 0.52 0.35 1091 A0 13.22 0.47 0.43 1092 A0 12.66 0.88 0.27 1093 F8 11.18 0.63 0.32 1094 K0II 10.24 1.46 1.60 1095 K0III 9.01 1.11 1.13 BD+59deg 2425 1096 F8 11.59 0.77 0.69: 1097 G5III 7.59 0.60 1.44 BD+59deg 2428 1098 F0 12.01 0.62 0.47 1099 A2 9.51 0.07 0.42: BD+59deg 2431, blend 1100 F6 10.90 0.92 0.26 1101 K0V 10.90 0.93 0.97 1102 A7 11.15 0.45 0.16 1103 A0 12.36 0.31 0.49 1104 G8III 9.77 1.35 1.78 BD+59deg 2426 1105 A0 12.84 0.68 0.39 1106 A0 12.18 0.62 0.41 1107 A0 13.76 0.75 0.68 1108 A0 12.66 0.73 0.40 1109 A2 12.22 0.92 0.31 1110 F8 11.66 0.55 0.06 1111 A0 11.83 0.70 0.46 1112 F0 11.06 0.95 0.67 1113 G5III 10.67 0.88 0.93 1114 G0III 10.19 0.85 0.85 1115 F8 10.42 0.63 0.21 BD+60deg 2305 1116 G0V 11.56 0.61 0.29 1117 K0III 10.97 1.15 1.46 1118 F8 11.64 0.49 0.13 1119 F8 11.74 0.68 0.27 1120 B1 8.07 0.36 -0.57 BD+59deg 2430 1121 A5 10.76 0.26 0.33 1122 A0 11.69 0.61 0.50 1123 B7 11.02 0.34 -0.01 1124 A0 12.47 0.68 0.54 1125 A0 12.18 0.81 0.88 1126 A0 11.83 0.29 0.34 1127 F0 11.56 0.55 0.15 1128 A0 11.57 0.45 0.02 1129 A0 12.60 0.56 0.42 1130 K2III 9.56 1.77 2.37 BD+59deg 2433 1131 F0 12.08 1.05 0.39 1132 A0 11.46 0.73 0.49 1133 A7 10.18 0.52 0.39 1134 A0 12.02 0.51 0.26 blend 1135 B6 10.73 0.33 -0.05 1136 B8 10.80 0.33 0.23 1137 A2 12.41 0.63 0.51 1138 dK 10.97 1.27 1.30 1139 F8 11.43 0.62 0.10 1140 A7 10.65 0.54 0.95 1141 A4 8.45 0.15 0.35 1142 K2II-III 10.28 1.41 1.56 1143 A2 10.20 0.32 -0.06 1144 A0 12.49 0.22 0.17 1145 B5 11.23 0.33 -0.39 1146 A0 10.24 0.27 -0.06 1147 A0 12.66 0.34 0.05 1148 F2 11.85 0.62 0.25 1149 A2 11.57 0.46 0.36 1150 G0 10.42 0.56 0.38 BD+60deg 2317 1151 F4 10.23 0.48 0.24 BD+60deg 2316 1152 F8 9.56 0.64 0.15 BD+60deg 2315 1153 A2 10.81 0.42 0.33 1154 B5 9.99 0.38 -0.28 1155 A4 11.89 0.38 0.29 1156 F8 11.88 0.55 0.12 1157 A0 13.04 0.47 0.57 1158 A0 12.86 0.53 0.30 1159 A0 12.68 0.37 0.36 1160 A0 9.09 0.12 0.03 BD+60deg 2306 1161 A0 12.01 0.28 0.17 1162 A0 13.05 0.39 0.32 1163 F0 9.52 0.39 0.23 BD+60deg 2308 1164 K5III 8.78 1.75 2.35 BD+60deg 2313 1165 A2 11.62 0.35 0.32 1166 A2 11.64 0.37 0.34 1167 A0 11.60 0.25 0.36 1168 K2III 9.81 1.54 1.80 1169 A0 11.86 0.34 0.34 1170 G5V 11.32 0.70 0.41 1171 A0 12.13 0.19 0.18 1172 F8 11.50 0.61 0.22 1173 A5 11.79 0.53 0.41 1174 K0III 10.95 1.26 1.26 1175 A0 11.99 0.76 0.59 1176 A0 11.82 0.23 0.07 1177 F5 10.48 0.36 0.12: BD+60deg 2319 1178 A0 11.58 0.36 0.00 1179 F8 7.72 1.02 0.27: BD+60deg 2321 1180 F6 11.01 0.67 0.19 1181 A2 11.86 0.58 0.21 1182 F8 10.83 0.50 -0.13 1183 F8 11.48 0.72 0.17 1184 G0III: 10.88 0.75 0.65 1185 A0 8.97 0.17 0.28 BD+60deg 2324 1186 F8 11.68 0.67 0.16 1187 G0V 11.94 0.67 -0.12 1188 G8III 10.75 1.14 0.89 1189 A0 11.75 0.52 -0.17 1190 dK 10.67 1.89 2.53 1191 A0 12.76 0.48 0.14 1192 F2 11.12 0.45 -0.02 1193 A0 12.89 0.38 0.19 1194 A0 10.89 0.38 -0.05 1195 A0 7.03 0.07 -0.31 BD+60deg 2320 1196 A0 12.69 0.26 0.31 1197 F8 12.62 0.37 0.22 1198 G8V 11.40 0.78 0.50 1199 G0 11.79 0.73 0.31 1200 F8 10.56 0.57 0.09 1201 A2 12.19 0.59 0.41 1202 F8 12.00 0.66 -0.10 1203 F2 11.82 0.67 0.33 1204 G0III 9.85 0.70 0.39 BD+60deg 2307 1205 K5III 9.77 1.69 1.99 1206 A0 12.29 0.44 0.36 1207 A0 12.22 0.82 0.45 1208 A2 11.38 0.21 0.20 1209 A0 10.17 2.03 2.45 1210 F8 10.84 0.52 0.00 1211 F8 12.21 0.59 0.40 1212 A0 13.05 1.21 1.13 1213 A0 12.17 0.54 0.59 1214 A2 11.39 1.03 0.37 1215 K0V 10.32 0.53 0.18 BD+60deg 2299 1216 A2 13.35 1.61 0.46 1217 dG 12.35 0.75 0.22 1218 A0 12.80 0.33 0.44 1219 M 5.93 1.97 2.18 BD+60deg 2300 1220 F8 11.30 0.64 0.24 1221 A0 12.52 0.72 0.45 1222 A0 12.34 0.18 0.23 1223 A2 12.65 0.46 -0.05 1224 K0III-IV 8.37 1.02 0.79: BD+60deg 2293 1225 K0IV 9.10 1.56 1.46: BD+60deg 2292 1226 F5 12.25 0.61 0.02: 1227 A0 12.28 0.26 0.09: blend 1228 A0 12.56 0.30 -0.06: 1229 F5 9.03 1.03 0.46: BD+60deg 2298, blend 1230 A0 12.94 0.51 0.12 1231 A2 12.78 0.53 0.30 1232 A2 12.10 0.38 0.17 1233 G5V 11.42 0.88 0.17 1234 F8 11.84 0.76 1.81 1235 F8 11.74 0.94 0.41 1236 A0 12.61 0.48 0.09: 1237 A2 11.28 0.35 0.08: 1238 A0 12.72 0.60 0.07: 1239 A0 12.27 0.31 -0.17: 1240 A2 11.11 0.46 0.17: 1241 F5 10.60 0.56 -0.21: BD+60deg 2304 1242 A0 12.40 0.39 0.02: 1243 B6 11.38 0.28 -0.29: 1244 B8 10.71 0.26 -0.07: 1245 A2 10.67 0.33 0.04: 1246 A0 12.24 0.31 -0.09: 1247 A0 13.08 0.65 0.09: 1248 B5 7.21 0.24 0.05: BD+60deg 2303 1249 A0 11.80 0.29 0.01: 1250 B6 11.06 0.25 -0.23: 1251 A0 11.64 0.38 -0.15 1252 F8 11.83 0.66 -0.08 1253 F8 11.55 0.58 -0.12 1254 A5 10.88 0.52 0.28: 1255 K0III 11.18 1.36 1.09 1256 A2 12.70 0.31 0.07 1257 B7 9.75 0.23 -0.44 BD+60deg 2310 1258 A0 12.89 0.71 -0.21: 1259 A0 12.42 0.32 -0.17 1260 A4 10.44 0.20 -0.40: 1261 A2 12.19 0.38 -0.09 1262 K0III 9.74 1.22 1.02: BD+60deg 2312 1263 A0 12.09 0.34 -0.22 1264 K0III 8.49 0.95 0.57: BD+60deg 2311 1265' G8Ib 6.13 1.60 1.60 BD+60deg 2318 1266 A7 11.27 0.58 0.25 1267 A0 12.09 0.44 0.14 1268 A0 12.57 0.44 -0.11 1269 A2 11.46 0.42 0.23 1270 A2 11.27 0.89 0.26 1271 F2 12.00 0.59 0.10 1272 A2 11.21 0.42 0.36 1273 K0IV 9.90 1.43 1.59 1274 K0 12.76 0.51 0.02 1275 A0 11.82 0.48 0.03 1276 F2 10.83 0.57 0.31 1277 A4 10.42 0.30 -0.34 BD+60deg 2322 1278 AS 7.12 0.30 -0.20 BD+60deg 2323 1279 A0 11.79 0.60 0.15 1280 A0 12.12 0.44 0.16 1281 A0 12.43 0.42 0.05 1282 A7 11.38 0.46 0.23 1283 F5 12.02 0.91 -0.22 1284 A4 12.23 0.53 0.11 1285 A2 12.04 0.51 -0.17 1286 A2 12.04 0.51 0.12 1287 F5 11.56 0.67 -0.01 1288 B7 11.74 0.34 -0.40 1289 A2 9.68 0.34 -0.23 BD+61deg 2225 1290 A2 11.85 0.39 -0.05 1291 dM 11.10 1.56 1.54: 1292 F6 8.37 0.46 -0.26: BD+61deg 2224 1293 F8 10.66 0.48 -0.22 1294 A0 12.69 0.66 0.09 1295 F2 12.08 0.78 0.03 1296 A0 12.31 0.22 -0.12 1297 K0III 10.22 1.35 1.36 1298 F0 12.65 0.51 0.13 1299 A4 11.92 0.63 0.05 1300 B7 11.43 0.22 -0.55 1301 A0 12.59 0.32 -0.01 1302 B8 11.40 0.24 -0.20: 1303 K2III 10.38 1.27 0.81 1304 G8III-IV 9.69 0.95 0.28 BD+61deg 2221 1305 G8III 7.10 1.01 0.53: 1306 A0 11.78 0.41 0.11 1307 A0 11.97 0.50 0.22 1308 F8 11.77 0.88 0.20 1309' B3V 7.56 0.13 -0.52 BD+61deg 2209 1310 G8III 10.89 1.22 0.81 1311' B2V 8.18 0.14 -0.57 BD+61deg 2208 1312 F2 10.66 0.40 -0.05: 1313 K3II 8.16 1.49 1.65: BD+61deg 2207 1314 K2III 9.80 1.73 1.90: BD+61deg 2205 1315 G5III 9.96 0.79 0.30: BD+61deg 2206 1316 F8 11.25 0.57 -0.18: 1317 F5 10.78 0.51 0.02: 1318 A0 12.13 0.65 0.00: 1319 K3I-II 10.63 1.49 1.32 1320 F0 12.20 0.49 0.21: 1321 A7 10.74 0.58 0.34 1322 G5III 10.76 1.34 0.74 1323 A0 12.36 0.60 0.15 1324 A3 8.36 0.30 0.14: BD+61deg 2199 1325 F6 10.42 0.58 0.02 1326 A0 13.54 0.49 0.09 1327 F2 11.59 0.75 0.05 1328 A0 12.26 0.58 0.24 1329 A0 12.19 0.41 0.10 1330 F5 10.15 1.00 0.21: blend 1331 B6 11.08 0.31 -0.49 1332 B0 7.53 0.31 -0.85 BD+61deg 2194 1333 F0 10.65 0.64 0.27 1334 dK 11.77 1.56 0.90 1335 A2 11.51 0.53 0.15 1336 A0 12.58 0.40 0.07 1337 F0 10.39 0.57 0.21 BD+61deg 2202 1338 A2 11.44 0.91 0.04 1339 F8 12.48 0.38 0.04 1340 F0 11.69 0.73 0.26: blend 1341 A0 12.20 0.62 0.15 1342 A0 12.09 0.50 -0.02 1343 A6 11.69 0.63 0.11 1344 F8 11.43 0.93 0.19 1345 A2 11.45 0.61 -0.05 1346 A0 12.18 0.62 0.74 1347 K2IV 9.63 0.87 0.24 BD+61deg 2204 1348 gK 11.21 1.42 1.24 1349 A2 10.93 0.41 0.01 1350 A0 12.53 0.55 0.09 1351 A0 12.67 0.74 0.04 1352 AD 12.03 0.30 0.12 1353 A0 11.78 0.78 0.06 1354 A0 12.79 0.38 0.03 1355 A0 12.23 0.77 0.14 1356 A0 11.46 0.46 0.17 1357 A0 11.75 0.44 0.06 1358 A0 11.60 0.22 0.14 1359 B5 9.16 0.15 -0.41 BD+61deg 2211 1360 F8 11.59 0.59 0.09 1361 gK 10.51 1.96 2.33 1362' F4 10.50 0.44 0.02 1363' A0 11.13 0.30 0.13 1364 A0 11.92 0.45 0.06 1365 A0 11.62 0.41 0.06 1366 B7 10.88 0.42 -0.20 1367 A0 12.95 0.47 0.21 1368 A0 11.90 0.25 -0.02 1369 A0 11.75 0.42 0.01 1370 A0 11.93 0.51 0.12 1371 A0 12.56 0.38 0.09 1372 A4 10.87 0.43 0.18 1373 B8 11.30 0.33 -0.30 1374 F8 12.01 0.65 0.17 1375 G8III 10.79 1.15 0.89 1376 F0 10.23 0.43 -0.17 BD+61deg 2212 1377 G8II 10.79 1.25 1.01 1378 A0 11.21 0.29 -0.09 1379 A0 11.35 0.46 0.01 1380 F8 8.92 0.51 -0.13 BD+61deg 2210, blend 1381 F2 12.06 0.85 -0.05 1382 A0 12.80 0.49 0.10 1383 F2 12.09 1.33 1.27 1384 F8 10.36 0.38 -0.11: 1385 F8 10.87 0.51 -0.29: 1386 A0 12.49 0.23 -0.05 1387 F8 11.35 0.58 -0.12 1388 A0 12.54 0.45 0.38 1389 F0 12.29 0.55 0.14 1390 F8 11.29 0.45 0.06 1391 K0III 10.03 1.59 1.66 1392 K0III 10.52 1.15 1.25 BD+61deg 2219 1393 F8 11.79 0.75 -0.01 1394 B8 11.28 0.26 -0.21 1395 F2 11.97 0.38 0.25 1396 A0 12.82 0.56 0.20 1397 K0V 10.66 0.88 0.44 1398 A0 13.04 0.38 0.30 1399 A0 12.54 0.23 0.43 1400 B6 10.15 0.22 -0.31 1401 F8 8.89 0.47 -0.01: BD+61deg 2223 1402 K0III 10.50 1.06 1.18: 1403 A0 12.35 0.42 0.23: 1404 A7 13.32 0.86 0.48: 1405 K2III 11.15 1.48 1.49: 1406 A0 12.36 0.59 0.14 1407 A2 11.02 0.31 -0.21: 1408 F6 12.62 0.63 0.24 1409 A0 12.64 0.25 0.40 1410 F8 12.17 0.49 0.31 1411 gK 11.33 1.36 1.37 1412 B8 11.54 0.28 0.12: 1413 A2 11.18 0.29 -0.19 1414 F8 10.15 0.20 0.28 BD+61deg 2228, blend 1415 A0 12.07 0.40 0.36 1416 F8 11.16 0.53 0.09 1417 G5 11.57 0.92 0.51: 1418 F8 10.10 0.86 0.75 1419 F0 11.65 0.55 0.14 1420 A4 10.54 0.40 0.32 BD+61deg 2230 1421 A2 9.91 0.10 0.08 BD+61deg 2231 1422 K0III 9.64 1.28 1.20 BD+61deg 2229 1423 F5 10.55 0.68 0.05 1424 K0III 9.55 0.97 0.92 1425 F0 10.74 0.34 -0.04 1426 F5 8.79 0.43 -0.05 BD+61deg 2226 1427 F5 10.44 0.39 -0.10 1428 K0V 10.01 1.00 0.77 BD+61deg 2227 1429 F8 10.95 0.78 0.45 1430 B1 6.68 0.09 -0.76 BD+61deg 2233 1431 K2III 11.64 0.58 0.04 1432 A2 11.37 0.27 -0.29 1433 F0 11.08 0.51 -0.03 1434 G0 11.90 0.65 -0.16 1435 G 12.41 0.93 0.12 1436 K0 9.94 1.58 1.09 BD+61deg 2239 1437 F2 11.31 0.77 0.06 1438 A0 12.82 0.53 0.30 1439 A0 12.39 0.29 0.07 1440 A2 10.90 0.17 -0.04 1441 A0 10.52 0.29 -0.01 1442 A0 11.89 0.64 0.28 1443 G5 12.68 0.90 0.26 1444 gK 9.58 1.64 1.38: 1445 B6 10.65 0.21 -0.51 1446 F0 11.44 0.49 0.20 1447 K0III 9.83 1.23 0.93 1448 A0 8.42 0.14 -0.03 BD+61deg 2243 1449 B7 11.05 0.10 -0.27 1450 A3 10.87 1.14 0.74 BD+61deg 2248 1451 A2 10.86 0.08 -0.15 1452 A0 12.49 0.42 0.37 1453 G0 8.92 0.50 0.11 BD+61deg 2250 1454 F0 10.06 0.40 0.29 BD+61deg 2252 1455 G5IV 9.35 0.85 0.51 BD+61deg 2253 1456 F8 8.63 0.36 0.05 BD+61deg 2258 1457 K2III 8.61 1.03 1.27 BD+61deg 2259 1458 A0 12.08 0.57 -0.01 1459 A0 11.79 0.42 0.14 1460 F8 11.66 0.51 0.05 1461 A2 11.82 0.13 0.10 1462 K2II-III 10.51 1.36 1.55 1463 F0 11.07 0.52 0.13 1464 K2I-II 9.96 1.37 1.51 1465 F2 11.48 0.73 0.23 1466 A0 8.73 0.04 0.01 BD+61deg 2260 1467 A0 12.19 0.43 0.19 1468 A0 11.79 0.56 0.13 1469 F6 11.26 0.70 -0.13 1470 F2 10.34 0.72 0.08 1471 K0III 9.26 1.14 0.80 BD+61deg 2264 1472 A2 11.26 0.37 0.13 1473 K0III 9.49 1.58 1.75 BD+61deg 2265 1474 A2 11.55 0.48 0.36 1475 F8 11.01 0.56 -0.14 1476 F8 10.90 0.56 0.07 1477 G0 11.21 0.59 0.23 1478 A0 9.02 0.01 0.05 1479 A0 11.96 0.21 -0.14 1480 A2 11.23 0.50 0.38 1481 K0III 9.44 1.49 1.46 1482 F8 11.83 0.68 0.09 1483 A0 11.76 0.39 -0.03 1484 G5 11.78 0.51 0.01 1485 K3II 8.77 1.05 1.11 BD+61deg 2257 1486 F6 9.82 0.41 -0.18 1487 K3II 8.82 1.02 0.93 BD+61deg 2255 1488 F2 12.00 0.54 0.20 1489 K2II 8.51 1.07 1.02 BD+61deg 2251 1490 K0III 9.82 1.07 0.89 1491 F6 10.95 0.74 0.08 1492 A2 11.07 0.32 -0.10 1493 A0 11.67 0.30 -0.09 1494 A0 11.67 0.31 -0.03 1495 K3III 11.05 1.08 0.99 1496 A2 11.45 0.47 0.08 1497 A0 11.84 0.51 0.09 1498 A0 12.10 0.34 -0.24 1499 K2III 11.19 1.35 0.85 1500 B7 10.31 0.10 -0.40 BD+61deg 2247 1501 O5e 8.86 -0.03 -0.73 BD+61deg 2248 1502 A0 12.33 0.65 0.06: 1503 A2 10.58 0.25 0.48 1504 A0 11.91 0.55 0.18 1505 A2 10.68 0.44 0.07 1506 A2 11.41 0.42 0.18 1507' O9.5Ib 5.10 0.09 -0.84 BD+61deg 2246 1508 A0 10.95 0.28 0.15 1509 B7 10.71 0.33 -0.31 1510 A0 11.39 0.39 0.16 1511 F0 11.24 0.64 0.28 1512 A0 11.67 0.35 -0.09 1513 A0 9.91 0.19 -0.38 BD+61deg 2242 1514 B3e 10.92 0.19 -0.43 1515 A0 11.45 0.49 0.03 1516 K0V 10.07 1.07 0.56 BD+61deg 2244 1517 A0 9.95 0.35 -0.26 BD+61deg 2241 1518 A0 11.52 0.41 0.05 1519 A5 9.39 0.28 0.13 BD+61deg 2240 1520 A0 11.59 0.44 0.15 1521 F5 11.26 0.57 0.03 1522 G5III 9.31 1.04 0.61 1523 K0III 8.90 1.22 1.21 BD+61deg 2336 1524 M 8.98 1.85 2.26 BD+61deg 2227 1525 A0 10.78 0.62 0.30 1526 F6 11.37 0.67 0.04 1527 F6 12.66 0.35 0.22 blend 1528 F6 11.16 0.72 0.11 1529 A7 11.61 0.58 0.34 1530 F5 11.65 0.65 -0.02 1531 K0 9.34 1.54 1.57 1532 A3 10.51 0.36 0.22 1533 A2 10.59 0.24 0.13 1534 K0III 6.95 1.17 1.18 BD+61deg 2334 1535 F0 11.76 0.98 0.04 1536 A0 12.95 0.56 0.21 1537 A0 12.13 0.84 0.24 1538 K2 11.34 1.15 0.05 blend 1539 F8 10.86 0.79 0.22 1540 A0 9.18 0.21 -0.04 BD+61deg 2245 1541 A0 11.82 0.50 0.16 1542 K0V 10.60 0.98 0.55 1543 A2 11.70 0.53 -0.04 1544 A0 11.96 0.43 0.19 1545 A4 10.94 0.59 -0.46 1546 G8 12.01 0.72 0.29 1547 F8 12.00 0.69 0.15 1548 B8 12.83 0.86 0.43 1549 A0 11.45 0.28 -0.01 1550 A2 11.00 0.26 -0.04 1551 K0III 11.13 1.60 1.09 1552 K0V 11.76 1.02 0.62: 1553 F8 11.76 0.49 0.15 1554 A2 12.00 0.37 0.30 1555 K2II-III 9.69 1.30 1.61 1556 F8 11.39 0.47 0.23 1557 G2 11.29 0.65 0.09 1558 B6 9.27 0.14 -0.30 BD+60deg 2359 1559 B8 11.58 0.12 -0.07 1560 A2 11.76 0.41 0.31 1561 A0 11.14 0.32 0.18 1562 G0 10.79 0.59 0.46 1563 A0 11.40 0.25 -0.18 1564 F8 11.55 0.95 0.38 1565 A0 11.62 0.21 0.25 1566 A0 12.35 0.33 0.18 1567 B2III 10.19 0.06 -0.25 BD+60deg 2355 1568 F8 10.18 0.47 0.06 1569 K0III 8.18 0.99 0.94 BD+60deg 2353 1570 A4 12.00 0.34 0.28 1571 B7 11.12 0.15 -0.16 1572 B8 10.86 0.19 0.16 1573 A0 12.27 0.57 0.29 1574 A0 12.33 0.37 0.04 1575 A0 12.70 0.35 -0.47 1576 A2 10.04 0.29 0.23 1577 F4 11.81 0.62 -0.04 1578 A0 12.91 0.39 0.11 1579 F2 10.71 0.52 0.13 1580 A2 10.00 0.18 -0.20 1581 A2 11.48 0.57 0.16 1582 A0 12.46 0.32 0.08 1583 A4 11.93 0.37 0.18 1584 F8 11.94 0.70 0.19 1585 G0 10.50 1.16 0.69 1586 F6 11.24 0.75 0.05 1587 B8 10.56 0.29 -0.09 1588 A0 11.92 0.38 -0.35 1589 B5 10.80 0.31 -0.01 BD+61deg 2232 1590 A5 10.79 0.53 0.13 1591 F8 10.76 0.68 -0.07 1592 A2 11.35 0.31 0.02 1593 A0 11.51 0.33 0.19 1594 B6 11.47 0.38 -0.37 1595 A0 11.54 0.21 0.17 1596 F8 11.63 0.48 -0.11 1597 A0 12.50 0.19 0.15 1598 A2 11.93 0.51 0.19 1599 A5 10.90 0.22 -0.02 1600 A7 11.17 0.61 0.24 1601 K0III 11.12 1.28 0.91 1602 A2 10.74 0.42 0.02 1603 F8 12.04 0.62 0.05 1604 G5III 10.87 1.29 0.97 1605 G0 11.99 0.68 0.17 1607 K0III 8.36 1.74 2.30 BD+60deg 2333 1608 A2 7.29 0.08 0.06: BD+60deg 2334 1609 A0 11.60 1.35 1.30 1610 A0 11.35 0.26 -0.11 1611 A0 12.90 0.36 0.19 1612 A0 12.87 0.69 0.28 1613 A0 11.71 0.44 0.14 1614 A0 12.77 0.38 0.03 1615 K0V 11.76 0.67 0.11 1616 A0 12.50 0.46 0.22 1617 A2 11.52 0.35 0.19 1618 F8 11.52 0.48 0.05 1619 A2 11.77 0.33 0.21 1620 A0 12.03 0.32 0.12 1621 F0 9.96 0.42 0.27 1622 A0 12.32 0.04 0.22 1623 G 10.46 0.57 0.47 1624 K 7.68 0.93 1.28 BD+60deg 2357 1625 A0 10.21 0.11 -0.42 BD+60deg 2356 1626 B2 8.15 0.03 -0.65 BD+60deg 2352 1627 A0 10.81 0.18 -0.19 1628 A0 11.81 0.14 0.08 1629 A0 11.76 0.39 0.11 1630 A0 13.06 0.36 0.25 1631 A0 11.68 0.67 0.27 1632 A0 11.25 0.36 0.13 1633 A7 10.27 0.32 -0.04 BD+60deg 2336 1634 A0 12.54 0.72 0.27 1635 dG 12.18 0.69 0.24 1636 G0 11.40 0.59 0.12 1637 F8 11.43 0.50 -0.02 1638 A2 9.10 0.61 0.58 BD+60deg 2332 1639 A0 12.34 0.58 0.30 1640 K 11.79 1.47 1.08 1641 F8 11.04 0.91 0.24 1642 B8 10.30 0.43 -0.02 1643 F5 11.61 0.61 0.19 1644 A0 12.72 0.54 0.06 1645 F8 12.04 0.67 0.14 1646 A2 11.75 0.45 0.28 1647 G0 11.23 0.70 0.33 1648 B2 7.88 0.18 -0.70 BD+60deg 2329 1649 K2III 9.67 1.79 1.93 1650 B6 11.94 0.36 -0.18 1651 A0 12.85 0.48 0.46: 1652 A0 11.73 0.53 0.45 1653 gK 11.08 1.51 1.41 1654 G2 10.56 0.60 0.00 1655 A2 11.13 0.33 -0.05 1656 F8 11.51 0.88 0.42 1657 K2III 8.99 2.04 2.48 BD+60deg 2325 1658 gK 11.52 1.27 1.04 1659 F8 10.62 0.55 0.06 1660 A0 12.44 0.53 0.30 1661 F8 11.50 0.61 0.02 1662 F5 11.56 0.55 0.11 1663 A0 7.97 0.01 -0.12 BD+60deg 2330 1664 A0 11.88 0.32 0.05 1665 A0 11.92 0.33 0.19 1666 A0 12.35 0.81 0.72 1667 A0 12.43 0.41 0.39 1668 F6 8.15 0.66 0.43 BD+60deg 2335 1669 B6 11.11 0.29 0.13 1670 F8 11.27 0.29 0.24 1671 A4 10.00 0.49 0.57 BD+60deg 2339 1672 B6 10.96 0.35 -0.07 1673 A0 11.57 1.10 0.86 1674 F8 11.00 0.63 0.26 1675 K0 7.30 1.60 0.77: BD+60deg 2331 1676 A2 11.09 0.26 -0.08 1677 A2 12.61 0.34 0.27 1678 K 10.28 1.42 1.14 1679 A5 11.10 1.24 0.77 1680 A0 12.47 0.36 0.36 1681 F8 12.28 0.23 0.14 1682 A0 12.26 0.24 0.43 1683 A0 12.45 0.85 0.35 1684 K3III 9.13 1.67 2.21 BD+60deg 2326 1685 F8 10.17 0.64 -0.03 1686 A2 10.83 0.85 0.64 1687 F6 11.43 0.78 0.13 1688 B6 11.46 0.33 -0.28 1689 A0 12.80 0.26 0.15 1690 A0 12.58 0.37 0.03 1691 A0 10.05 0.67 0.26 1692 F8 11.70 0.82 0.33 1693 F5 11.10 0.57 0.15 1694 A5 8.39 0.27 0.35 1695 A0 10.29 1.46 1.53 1696 K2III 9.53 1.42 1.44 1697 B5 11.20 0.28 -0.27 1698 B5 11.31 0.27 -0.36 1699 F5 11.46 0.71 0.12 1700 K0III 10.75 1.21 0.89 1701 A0 11.96 0.31 0.19 1702 A0 12.72 0.58 0.08 1703 B6 11.90 0.18 -0.19 1704 A0 12.66 0.49 0.39 1705 A0 14.08 0.75 0.65 1706 B8 12.68 0.46 0.02 1707 A0 13.00 0.67 0.47 1708 A0 12.74 0.48 0.20 1709 A0 11.88 0.54 0.08 1710 A0 12.18 0.87 0.36 1711 A0 13.24 0.20 0.80 1712 A0 12.57 0.18 0.18 1713 A0 13.15 0.50 0.20 1714 A0 12.46 0.57 0.07 1715 A0 11.91 0.35 0.18 1716 A0 12.57 0.43 0.08 1717 A0 12.37 0.38 0.04 1718 A0 12.73 0.54 0.18 1719 F0 11.63 0.71 -0.17 1720 A0 12.25 1.23 0.17 1721 A0 12.44 0.69 0.00 1722 A0 12.36 0.91 0.11 1723 A0 12.59 0.46 0.72 1724 F2 12.15 0.61 0.00 1725 A0 12.48 1.32 0.33 1726 A0 13.09 0.93 0.19 1727 A0 12.44 0.61 0.29 1728 A0 12.97 0.79 0.40 1729 A0 12.67 0.56 0.07 1730 A0 13.67 1.03 0.72 1731 A0 12.00 0.83 0.07 1732 F8 11.30 1.46 0:91 1733 G0 12.55 0.55 0.08 1734 A0 12.06 0.98 0.22 1735 A7 13.67 0.93 0.25 1736 B8 10.73 1.64 1.41 1737 F0 11.82 0.52 0.01 1738 F2 12.57 0.49 0.14 1739 A5 12.95 1.02 0.20 1740 F8 12.24 0.84 0.28 1741 K0 11.25 1.16 0.51 1742 A0 13.09 1.08 0.16 1743 A0 12.88 0.70 0.09 1744 A0 12.14 0.71 0.15 1745 A0 12.50 0.51 0.10 1746 A0 12.24 0.49 0.19 1747 A0 12.57 0.67 0.34 1748 A0 11.21 0.52 0.09 1749 A0 13.00 0.61 0.22 1750 A0 12.56 0.63 0.20 1751 A0 12.35 0.64 0.23 1752 A0 12.70 0.60 0.17 1753 A0 12.19 0.98 0.41 1754 A5 12.98 0.95 0.15 1755 A0 12.75 0.75 0.20 1756 A0 13.12 0.89 0.26 1757 A0 12.59 0.68 0.16 1758 A0 13.02 1.76 - 1759 A0 13.00 0.75 0.11 1760 A0 12.79 0.62 0.06 1761 A0 12.88 0.69 0.04 1762 K0III 11.23 1.26 0.86 1763 F0 11.88 0.69 0.13 1764 A0 12.68 1.05 0.01 1765 F0 13.09 0.51 - 1766 A2 12.25 0.49 0.05 1767 A0 12.68 0.65 0.22 1768 A2 12.72 0.75 1.11 1769 F2 12.27 0.72 0.33 1770 A0 12.05 1.68 1.60 1771 A0 12.96 0.81 0.28 1772 A2 12.73 0:89 0.19 1773 A0 12.93 0.87 0.20 1774 K2III 10.92 1.61 1.25 1775 A0 12.95 0.92 0.28 1776 A0 12.88 0.65 0.37 1777 A0 12.81 0.80 0.41 1778 F5 11.73 0.59 0.11 1779 A0 12.76 0.63 0.06 1780 A0 13.09 0.92 0.14 1781 A0 11.95 1.13 0.27 1782 A4 12.04 1.03 0.23 1783 A0 12.65 0.90 0.58 1784 K2III 10.16 1.71 2.03 1785 A0 12.75 0.81 0.52 1786 A5 12.58 1.18 0.56 1787 A0 12.81 0.76 0.04 1788 A2 12.95 0.75 0.27 1789 A0 12.83 0.75 0.15 1790 gK 10.86 1.70 1.53 1791 A2 12.75 0.76 0.06 1792 A0 12.66 0.44 0.08 1793 A0 12.90 0.69 0.04 1794 A0 13.31 0.78 0.26 1795 A0 12.86 0.74 0.18 1796 A0 13.01 0.71 0.23 1797 A0 13.28 0.61 0.09 1798 A0 13.16 0.68 0.23 1799 A0 12.73 0.38 0.09 1800 A0 13.18 0.19 0.81 1801 A5 13.22 0.75 0.24 1802 Me 11.34 2.20 2.00 1803 Me 10.98 2.24 2.43 1804' B1 6.69 0.24 -0.57 BD+61deg 2216 1805' B1 7.02 0.26 -0.56 BD+61deg 2217 1806' B1 7.90 0.08 -0.73 BD+62deg 2006 1807' B3 8.92 0.17 -0.46 BD+61deg 2215 1808' B3 9.34 0.18 -0.40 BD+61deg 2214 1809' B3 9.83 0.23 -0.33 BD+61deg 2213 1810' B3 10.01 0.15 -0.49 NOTES TO THE CATALOGUE A point* at the right upper side of the running number denotes photoelectrically measured magnitudes. Blend is remarked if the photographic image of the measured star is distorted by a neighbouring star. A colon beside the U-B colour denotes that the ultraviolet magnitude of the star is uncertain because of the field error of the ultraviolet filter. Star No. 1501: The HD type of this star is A3. On our plates it shows an O-type spectrum, with HeII 468.6 in emission. Star No. 1514: HeI 4026 can be seen in emission. * ' in the electronic text and HTML versions