164 
165 
Zone o° bis -j- 20° Declination. 
165 
Grösse 
7-19 
8.o8 
7.07 
5.86 
6 .&? 
7.« 
6-57 
6.26 
7-52 
6.42 
6.84 
7-38 
6.78 
6.82 
6.51 
6.50 
7.41 
7.48 
7.48 
7-36 
7.28 
6.66 
6-59 
6-95 
7.27 
6 - 55 
6.86 
7 - 2 5 
7-36 
6.82 
7.21 
B.D. 
Sternzeit 
I 
II 
UI 
IV 
J 
z 
log sin 2 / 
corrig. 
für Ext. 
Diff. 
in log. 
l)iff. in 
Grössen 
Grösse 
io‘ 
’1818 
7 1 
*35" 
i 9°3 
1783 
1986 
1784 
18840 
4382 
8.9984 
9.0289 
9 
2239 
7 
37 
15-3 
13.6 
15.6 
14.7 
14.80 
50.1 
8.8146 
8.8631 
13 
2074 
7 
40 
18.0 
17.0 
18.7 
16.2 
1748 
43-2 
8.9553 
8.9858 
0.0516 
— 0.13 
6.82 
19 
2201 
7 
41 
10.8 
9-5 
11.2 
9.6 
10.28 
37-9 
8.5030 
8.5239 
0.4103 
4-1-03 
7.98 
18 
2182 
7 
43 
13-7 
12.4 
14-3 
I 3 - 1 
13-38 
38.6 
8.7287 
8.7508 
0.1834 
+ O.46 
7.41 
18 
2183 
7 
45 
14.7 
13.6 
16.0 
144 
14.68 
38-7 
8.8076 
8.8298 
0.1044 
+ O.26 
7.21 
G 
CO 
1 ^ 
O 
CM 
7 
46 
23-3 
19.2 
23.0 
19.0 
21.12 
39-7 
9-1134 
9- 1 3 7 3 
0.2031 
— 0.51 
6.44 
19 
2215 
7 48 
1 1-5 
10.5 
11-4 
10.2 
10.90 
37-4 
8-5534 
8.5736 
0.3606 
4- 0.90 
7.85 
9 
2239 
7 
50 
14.0 
12.8 
154 
134 
13.90 
48.8 
8.7612 
8.8058 
10 
1818 
7 
53 
18.5 
17.0 
18.1 
17.6 
17.80 
42.4 
8.9706 
8.9995 
Mittel aus den Vergleichstcrnbeobachtungen : 8.9540; 8.9460; 8.9027. 
Zur Reduction benutzt: 8.9342. 
Zone 100 
. 1887 Februar 28. 
Beobachter: Kempf. 
Photometer : 
D. Vergleichsterne: Nr. 22 und Nr. 
24. Luft: 
3 * 
9 ' 
2374 
g ll 2 2 m 
3287 
3486 
3684 
3 1 86 
33882 
4583 
9.4911 
9.5264 
11 
2372 
9 
24 
21.5 
20.5 
23-5 
21.4 
21.72 
47.6 
9.1366 
9.1778 
15 
2290 
9 
26 
1 5 -1 
13.6 
16.9 
13-5 
14.78 
41.1 
8.8134 
8.8398 
0.5275 
4 - 1.32 
7.72 
10 
2250 
9 
28 
17.0 
13-5 
16.4 
14-3 
I 5-30 
45-6 
8.8428 
8.8788 
0.4885 
4- 1.22 
7.62 
13 
2358 
9 
29 
14.0 
12.5 
13-5 
134 
13-35 
43 -o 
8.7268 
8.7569 
0.6104 
4 - i -53 
7-93 
14 
2344 
9 
30 
10.8 
10.6 
14.4 
11.1 
11.72 
42.4 
8.6156 
8.6445 
O.7228 
4- 1.81 
8.21 
14 
2345 
9 
32 
14.4 
12.6 
18.5 
15.6 
15.28 
41.9 
8.8417 
8.8696 
O.4977 
4 -1-24 
7.64 
17 
2318 
9 
33 
20.0 
21.4 
234 
20.0 
21.20 
38.8 
9-1165 
9.1389 
0.2284 
4-0.57 
6.97 
9 
2374 
9 
36 
32.1 
35 -o 
38.9 
39-6 
36.40 
44-5 
9-5467 
9.5801 
11 
2372 
9 
38 
21.5 
22.5 
22.3 
21.1 
21.85 
46-3 
9 -I 4 I 5 
9-1793 
16 
2224 
9 
40 
15.6 
13-5 
15.O 
14.0 
14.52 
39-5 
8.7984 
8.82 19 
0.5454 
4 -1-36 
7.76 
12 
2307 
9 
42 
17-5 
16.9 
18.5 
154 
17.08 
43-8 
8-9358 
8.9677 
0.3996 
4-1.00 
7.40 
15 
2301 
9 
44 
22.0 
22.9 
23.6 
25.0 
23-38 
40.8 
9.1972 
9.2230 
0.1443 
4-0.36 
6.76 
11 
2333 
9 
45 
13-4 
14-5 
16.5 
16.2 
15-15 
44-5 
8.8344 
8.8678 
0.4995 
4 -1-25 
7-65 
13 
2378 
9 
47 
21.7 
18.9 
20.9 
18.9 
20.10 
42.5 
9.0723 
9.1014 
0.2659 
4- 0.66 
7.06 
13 
2379 
9 
48 
18.5 
19.8 
19.1 
20.5 
19.48 
42.2 
9.0461 
9.0746 
0.2927 
4-0.73 
7-13 
9 
2374 
9 
50 
31-5 
34 -o 
344 
35-6 
33-88 
43-9 
9.4924 
9-5245 
11 
2372 
9 
52 
22.2 
21.8 
24.8 
22.9 
22.92 
45 -o 
9.1809 
9-2155 
Mittel aus den Vergleichsternbeobachtungen: 9.3521 ; 9.3797; 9.3700. 
Zur Reduction benutzt: 9.3673. 
Zone 101. 1887 März i. 
Beobachter : Müller. 
Photometer: D. Vergleichsterne: Nr. 16 und Nr. 18. Luft: 
2. 
11° 
1588 
5 ' 
42“ 
2 o?o 
1787 
2 I?2 
1885 
19835 
4 d -7 
9.0406 
9.0769 
10 
1818 
5 
45 
154 
16.4 
18.4 
16.0 
16.55 
53 -i 
8.9093 
8.9683 
17 
1696 
5 
47 
12.7 
12.4 
13.O 
11.4 
12.38 
42.4 
8.6624 
8.6913 
0.3013 
4-0.75 
7-43 
16 
1580 
5 
48 
12.0 
11.4 
12.8 
11.4 
11.90 
43 - 1 
8.6286 
8.6589 
0.3337 
4- 0.83 
7-51 
16 
1590 
5 
50 
24.4 
24.4 
26.5 
23-3 
24.65 
43-4 
9.2405 
9-2 7 1 5 
0.2789 
— 0.70 
5-98 
18 
1778 
5 
52 
12.5 
12.3 
13-9 
12.3 
12.75 
40.8 
8.6876 
8 - 7 i 34 
0.2792 
4-0.70 
7-38 
12 
I 71 2 
5 
53 
13-5 
13-7 
15.0 
13-4 
13.90 
45-8 
8.7612 
8.7977 
0.1949 
4-0.49 
7- 1 7 
11 
1717 
5 
55 
IO.I 
8.0 
9-7 
8.8 
9- 1 5 
47-2 
8.4029 
8.4430 
0.5496 
4 - 1 -3 7 
8.05 
11 
1588 
5 
57 
17.7 
17.6 
19.7 
17.6 
18.15 
44.4 
8.9869 
9.0201 
IO 
I8l8 
5 
59 
18.5 
15.2 
154 
15.6 
16.18 
51-5 
8.8901 
8.9432 
16 
1598 
6 
1 
22.6 
21.4 
21.3 
22.6 
21.98 
41.8 
9.1464 
9- 1 741 
0.1815 
— 0.45 
6.23 
13 
l8ll 
6 
3 
20.3 
19.7 
21.6 
20.9 
20.62 
44.6 
9-0935 
9.1272 
0.1346 
— 0.34 
6-34 
19 
1896 
6 
5 
12.0 
12.7 
13-9 
12.6 
12.80 
39-4 
8.6909 
8 - 7 I 43 
0.2783 
-i-0.70 
7-38 
18 
l8l6 
6 
6 
14.0 
12.3 
13-7 
12.9 
13.22 
39-9 
8.7185 
8.7427 
0.2499 
4- 0.62 
7-30 
13 
l8l6 
6 
7 
17.6 
154 
17-5 
15-9 
16.60 
44.9 
8.9118 
8.9462 
0.0464 
—(— 0.12 
6.80 
13 
1817 
6 
9 
14.6 
14-3 
13-7 
15-6 
14-55 
44-7 
8.8001 
8.8340 
0.1586 
4-0.40 
7.08 
11 
1588 
6 
10 
19.1 
1 7-7 
18.4 
17.7 
18.22 
43-5 
8.9901 
9.0213 
IO 
I8l8 
6 
13 
16.5 
15-3 
17.0 
15.0 
15-95 
49.9 
8.8781 
8.9260 
Mittel aus den Vergleichsternbeobachtungen: 9.0226; 8.9817; 8.9736: Zur Reduction benutzt: 8.9926. 
Putì, des Astrophys. Obs. zu Potsdam. Bd. IX. 21