30 
Blazkov. 
Bestimmung des Azimuthes. 
Object 
Kreislage 
Ulnzeit 
Kreisablesung 
wegen des Run 
corrigiert 
Correction 
wegen 
Neigung 
Azimuth 
des Sternes 
Siidp unkt 
der 
Kreistheilung 
Azimuth 
des Objectes 
exclusive 
Correction der 
Collimation 
1891. Mai 29. a. 
m. 
a = l h 18 m 7'6; § = 4b 88 c 
43’ 24-5; ar = — l m 10 ? 3; 
Ambrozny -<> 
R 
189° 12' 3 V 8 
Polaris 
0 
22 11 46 m 43 ? 5 
61 14 16-G 
4- l v 9 
1° 14’ 21*4 
59° 59’ 57*0 
309° 12’ 6*8 
W 
22 49 21-5 
241 13 11-0 
4- 4-9 
1 13 16-7 
239 59 59-1 
5-5 
Ambrozny <>- 
L 
9 12 4-6 
Mittel = 
=309° 12' 6*15 
Äa* =4-0*027 Aa” — 0-934 A3” 
1891. Mai 29. a. 
m. 
a = l h 18 m 7 ? 6; 8 = 4- 88° 
43' 24-5; x— — l m 10'3; 
Ambrozny <>- 
L 
99° 11' 37-9 
Polaris 
W 
22 h 56 m 52 ? 0 
331 9 34*0 
4- 1*7 
1° 10’ 8*8 
329° 59' 26*9 
309° 12' 10*0 
0 
22 59 290 
151 8 22-9 
-4 4-2 
1 9 2-1 
149 59 24-9 
15-3 
Ambrozny -<> 
R 
279 11 "40-2 
Mittel = 
= 309° 12’ 13*15 
A a =4- 0-028 Aa’ —0-928 A3" 
1891. Mai 29. a. 
m. 
a = l h 18 m 7 ? 6; 8 = 4-88° 43' 24-5: 
x— — l m 10 ? 3; 
Ambrozny <>■ 
R 
234° 12' 18''0 
Polaris 
0 
23 11 8 m 1 ? 0 
106 5 27-1 
4- 1*3 
1° 5’ 20*9 
105° 0’ 7*5 
309° 12’ 10*5 
vv 
23 10 14-5 
286 4 28-7 
4- 4-7 
1 4 22-2 
285 0 112 
8-5 
Ambrozny «>- 
L 
54 12 19-7 
Mittel - 
=309° 12' 9*50 
Aa" =4-0*029 Aa" —0-866 A3” 
1891. Mai 29. a. 
m. 
a = l Jl 18 m 7 ? 6; 8 = 4- 88 c 
43' 24*5; » = — l m 10 ? 3; 
Ambrozny <>• 
L 
144° 11' 39"4 
Polaris 
W 
23 h 16 m 4 ? 5 
16 1 20-6 
4- 3*0 
1° 1’ 46*6 
14° 59’ 36*9 
309° 12' 2*5 
0 
23 18 9-0 
196 0 15-2 
4- 6-4 
1 0 50-7 
194 59 30-8 
11*4 
Ambrozny -<>■ 
R 
324 11 42-2 
Mittel = 
= 309° 12' 6*95 
Aa” = + 0-030 Aa” —0*819 A8 y