No. 6.| DETERMINATION OF AZIMUTH. 63 
1894. Object Oc.| Watch Horizontal Circle Level A Rem. 
i 
hms 0 ‘ a ‘ a“ 0 ‘ 4“ 
Feb, 13 Cc 392 54 11.5| 54 13 [Ass.2220] 
Feb. 22 ¢ S 265 3496 | 34 45 
a Cass N | 0 25 39 96 24 90.5|95 6.5) Went out on || 289 13 
” S | 034 5 | 98 18 54 | 19 22.5 turning 991 8 
¢ N 265 31.2 |31 85 
Mar. 5] | om : 40 95 | 7.0 
i t L 16 39 48 | 168595 | 55.5 199 2 9 
Sun PB: L. 17 36 33.5 ? 
mas 38 130 | 184 54.0 | 49.5 206 4 56 
a W095 | 7.0 
Mor.20) 3 eee 4218 |949 
un P. L. 3 2 
DRE ie 30 | 204 32.0 | 82.0 164 16.5 | 2) 
Mar. 22 Gh - |130 39 95/39 35.5 
a Persei 93 58 40 |309 18 75/19 185|/S 430 N 31,0 || 262 8 33 | 2) 
Mar. 23 - 013 16 |312 56 405/57 43 |N 41.6 S 324 || 265 49 57 
é 130 3755 | 38 15.5 
Mar30) 3 eh ds 3995 |325 
un . 5 ZI 
it F = i r 348 33.3 | 35.5 27 96 38 
un . L. 20 9 
ier 16 96.5 349 504 [53.5 8 43 55 
Son! Bel ate ge | 1195.0 | 985 270 33.27 
m 3993 | 394 
Apr.i5] | om | rete 112 61.7 |594 ; 
un P. L. = 6 P r 
Tee Te oe gy | 85528 | 51.2 M. r. MoT 18) 2 ce 
Suna 0 3% | 97454 ane M. t. 246 51 31 | font. 
Sun P. L. 91 356 ; Sun 
cea é 5 982 53.7 | 55.0 M. r. 261 54 29 | Sum 
Sun P. L. 91 20 G 
me 334, (288 938 = | 94.7 M. t. %6 3 32] Do. 
- 112 62.0 1598 
Apr.20] | om a eeee 113 20 | 00 
un Fy 5 
ee F ors| 87465 | 45.0 M. r. WS 82 58] oi 
Sete 20 BAe \rao4o0y | 1170 M. t. 7 13 97 | front. 
” 
Sun P. L. 21 37 13 : Sun 
:: Ea 3 20 292 40.5 | 42.5 M. r. 968 59 5 | pun 
un. PL: 1 
me He eyes ee WMO M. t. 270 49 43] Do. 
in 113 35 | 05 
Apr. 25 m 114 48.8 | 46.0 4) 
San Fe 20 13 10 | 93 320 © | 298 We 250 44 93 | Sun in 
Sun P. L. 21 10 20 ar Sun 
as 19 33 |286 19.5 | 20.0 M. x. 963 21 56 | pur 
Sun Feb. aL 16 50 |a80 175 | 185 M. t. 264 58 11| Do. 
Sun P. L. 21 MW 18 ! 
. 289 46.5 ( M. r. 26 97| Do. 
arRe Ts 26 30 46 48.0 r 6 49 97 0. 
1) W43h5m Hw—W=-—0™7s.7; March 21 W13h4m Hw—-W=+0™5s5. 2) Star ass. 
to be 6 Persei. The corrections applied to the altitudes of the same star in List A (p. 7) are 
erroneous; the altitudes have been computed on the supposition that the star was 0 Persei and 
with a correction of + 10‘ to the circle-readings Oc. N. 
4) Taken nearly 5 hours before the first obs. of the Sun and 8 hours before the last obs, 
of m. 
8) W 13h 19m Hw—W =-+ 
4m 195.5, 
