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Table 1:

Distribution of the B1900.0 centers of the 1400 $2^\circ \times 2^\circ $ fields of the Sydney Observatory Astrographic Program.
$\delta_0$ n $\Delta\alpha$ $(\alpha_0)_j,1\leq j\leq n$ Epoch k m
-52$^\circ$ 120 12m 12m(j-1) 1924.14 $\pm$ 9.24 3 5
-53$^\circ$ 120 12m 6m+12m(j-1) 1902.30 $\pm$ 4.04 12 17
-54$^\circ$ 120 12m 12m(j-1) 1928.05 $\pm$ 2.12 3 10
-55$^\circ$ 120 12m 6m+12m(n-1) 1900.55 $\pm$ 3.04 12 17
-56$^\circ$ 120 12m 12m(j-1) 1928.62 $\pm$ 1.95 3 13
-57$^\circ$ 120 12m 6m+12m(j-1) 1901.27 $\pm$ 3.33 20 23
-58$^\circ$ 120 12m 12m(j-1) 1929.19 $\pm$ 1.17 6 23
-59$^\circ$ 120 12m 6m+12m(j-1) 1901.47 $\pm$ 3.23 28 37
-60$^\circ$ 90 16m 16m(j-1) 1928.82 $\pm$ 2.67 11 17
-61$^\circ$ 90 16m 8m+16m(j-1) 1902.67 $\pm$ 4.53 24 25
-62$^\circ$ 90 16m 16m(n-1) 1929.63 $\pm$ 0.83 11 22
-63$^\circ$ 90 16m 8m+16m(j-1) 1902.51 $\pm$ 3.97 24 25
-64$^\circ$ 80 18m 18m(j-1) 1929.90 $\pm$ 0.54 8 7

Source LaTeX | All tables | In the text

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