AnnualReport-1881 — Page 120

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Probable error of clise

tion -On he assituation

' pute

tre ahve Tabe umishes

3

be the severaly

observation is the same for every pair of stars, a comparison of the "estuts all means for determining its mean value from all the pairs, thus. Let differences for any pair between the several results for latitude from that pair (of which there have been n observations) and the mean result from that pair; and let such differences or residuals be similarly taken out for all of the pairs which have been observed more than once; and let V be the sum of the squares of all these residuals, N the total number of determinations, M the total number of 'pairs observed more than once, and Q (.6745) the factor for reduction of mean to probable errors. Then e,

the probable error of observation, is found by the formula,

1

V

Q2

N-M

.455

N-M

..(6)

Table III, below, exhibits the steps of the process for determining V.

TABLE III.

TO FIND THE PROBABLE ERROR OF OBSERVATION.

No. of pair

Stars of the pair; B. A. C. Nos.

Seconds of latitude

Means

V

#

#!

Г

9.55

0.68

.4624

9.54

0.69

.4761.

745-786

10.48

10,23

0.25

.0625

11.18

0.95

.9025

10.41

0.13

.0324

13.59

0.54

.2916

872-901

12.26

13.05

0.79

.6241

13.31

0.26

.0676

3

502-518

13.97

13.39

0.65

.4225

1

999-1052

14.55

14.05

0.50

.2500

14.20

0.15

.0225

10.66

0.28

.0781

10

5

1097-1138

9.27

10.38

1.11

1.2321

11.22

0.84

.7056

12.27

0.70

.4900

6

574-628

11.57

10.87

0.70

.4900

12.56

0.03

.0009

1045-1052

11.82

12.53

0.71.

.5041

13.22

0.69

.4761

11.97

0.22

.0484***

.1326-1346

12.19

12.41

0.22

.0484

13.37

0.08

.0064

9

1391-1408

13.29

13.22

0.07

.0019

10

1408-1437

11.70

10.57

0.28

.0784

11

1726-1778

9.74

10.29

0.55

.3025

10.56

0.27

.0729

9.21

0.63

.3969

12

1937-1876

9.17

9.84

0.67

.4489

11.14

1.30

1.6900

13.75

0.59

.3481

13

510- 574

13.16

12.57

0.59

.3481

11.12

0.04

.0016-

14

1377-1444

11.16

11.20

0.04

.0016

13.15

0.03

.0009

15

1420-1444

13.12

13.09

0 03

.0009

13.24

0.12

.0144,

16

1602-1687

14.90

13.36

1.54

2.3716

11.93

1.43

2.0449

9.83

0.03

17

1958-2001

9.86

9.89

0.03

.0009

00094€

18

1408-1432

11.70

1

12.72

0.23

.0529

19

1893-1900

12.49

12.26

0.23

.0529***

20

1990-2082

13.47

Page 120

Page 121

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Probable error of clise tion -On he assituation ' pute tre ahve Tabe umishes 3 be the severaly observation is the same for every pair of stars, a comparison of the "estuts all means for determining its mean value from all the pairs, thus. Let differences for any pair between the several results for latitude from that pair (of which there have been n observations) and the mean result from that pair; and let such differences or residuals be similarly taken out for all of the pairs which have been observed more than once; and let V be the sum of the squares of all these residuals, N the total number of determinations, M the total number of 'pairs observed more than once, and Q (.6745) the factor for reduction of mean to probable errors. Then e, the probable error of observation, is found by the formula, 1 V Q2 N-M .455 N-M ..(6) Table III, below, exhibits the steps of the process for determining V. TABLE III. TO FIND THE PROBABLE ERROR OF OBSERVATION. No. of pair Stars of the pair; B. A. C. Nos. Seconds of latitude Means V # #! Г 9.55 0.68 .4624 9.54 0.69 .4761. 745-786 10.48 10,23 0.25 .0625 11.18 0.95 .9025 10.41 0.13 .0324 13.59 0.54 .2916 872-901 12.26 13.05 0.79 .6241 13.31 0.26 .0676 3 502-518 13.97 13.39 0.65 .4225 1 999-1052 14.55 14.05 0.50 .2500 14.20 0.15 .0225 10.66 0.28 .0781 10 5 1097-1138 9.27 10.38 1.11 1.2321 11.22 0.84 .7056 12.27 0.70 .4900 6 574-628 11.57 10.87 0.70 .4900 12.56 0.03 .0009 1045-1052 11.82 12.53 0.71. .5041 13.22 0.69 .4761 11.97 0.22 .0484*** .1326-1346 12.19 12.41 0.22 .0484 13.37 0.08 .0064 9 1391-1408 13.29 13.22 0.07 .0019 10 1408-1437 11.70 10.57 0.28 .0784 11 1726-1778 9.74 10.29 0.55 .3025 10.56 0.27 .0729 9.21 0.63 .3969 12 1937-1876 9.17 9.84 0.67 .4489 11.14 1.30 1.6900 13.75 0.59 .3481 13 510- 574 13.16 12.57 0.59 .3481 11.12 0.04 .0016- 14 1377-1444 11.16 11.20 0.04 .0016 13.15 0.03 .0009 15 1420-1444 13.12 13.09 0 03 .0009 13.24 0.12 .0144, 16 1602-1687 14.90 13.36 1.54 2.3716 11.93 1.43 2.0449 9.83 0.03 17 1958-2001 9.86 9.89 0.03 .0009 00094€ 18 1408-1432 11.70 1 12.72 0.23 .0529 19 1893-1900 12.49 12.26 0.23 .0529*** 20 1990-2082 13.47 Page 120 Page 121
Baseline (Original)
Probable error of clise tion -On he assituation ' pute tre ahve Tabe umishes 3 be the severaly observation is the same for every pair of stars, a comparison of the "estuts all means for determining its inean value from all the pairs, thus. Let differences for any pair between the several results for latitude from that pair (of which there have been n observations) and the mean result from that pair; and let such differences or residuals be similarly taken out for all of the pairs which have been observed more than once; and let V be the sun of the squares of all these residuals, N the total number of determinations, M the total number of 'pairs observed more than once, and Q (.6745) the factor for reduction of mean to probable errors. Then e, the probable error of observation, is found by the formula, 1 حمد V Q2 N-M .455 N-M ..(6) Table III, below, exhibits the steps of the process for determining V. TABLE III. TO FIND THE PROBABLE ERROR OF OBSERVATION. No. of pair Stars of the pair; B. A. C. Nos. Seconds of latitude Means V # #! Г 9.55 0.68 .4624 9.54 0.69 .4761. 745-786 10.48 10,23 0.25 .0625 11.18 0.95 .9025 10.41 0.13 .0324 13.59 0.54 .2916 872-901 12.26 13.05 0.79 .6241 13.31 0.26 .0676 3 502-518 13.97 13.39 0.65 4225 1 999-1052 14.55 14.05 0.50 .2500 14.20 0.15 .0225 10.66 0.28 .0781 10 5 1097-1138 9.27 10.38 1.11 1.2321 11.22 0.84 .7056 12.27 0.70 .4900 6 574-628 11.57 10.87 0.70 .4900 12.56 0.03 .0009 1045-1052 11.82 12.53 0.71. .5041 13.22 0.69 .4761 11.97 0.22 .0484*** .1326-1346 12.19 12.41 0.22 .0484 13.37 0.08 .0064 9 1391-1408 13.29 13.22 0.07 .0019 10 1408-1437 11.70 10.57 0.28 .0784 11 1726-1778 9.74 10.29 0.55 .3025 10.56 0.27 .0729 9.21 0.63 .3969 12 1937-1876 9.17 9.84 0.67 .4489 11.14 1.30 1.6900 13.75 0.59 .3481 13 510- 574 13.16 12.57 0.59 .3481 11.12 0.04 .0016- 14 1377-1444 11.16 11.20 0.04 .0016 13.15 0.03 .0009 15 1420-1444 13.12 13.09 0 03 .0009 13.24 0.12 0144, 16 1602-1687 14.90 13.36 1.54 2.3716 11.93 1.43 2.0449 9.83 0.03 17 1958-2001 9.86 9.89 0.03 .0009 00094€ 18 1408-1432 11.70 1 12.72 0.23 تشير .0529 19 1893-1900 12.49 12.26 0.23 .0529*** 20 1990-2082 13.47 Page 120Page 121
2026-05-05 19:15:12 · Baseline
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Probable error of clise

tion -On he assituation

' pute

tre ahve Tabe umishes

3

be the severaly

observation is the same for every pair of stars, a comparison of the "estuts all means for determining its inean value from all the pairs, thus. Let differences for any pair between the several results for latitude from that pair (of which there have been n observations) and the mean result from that pair; and let such differences or residuals be similarly taken out for all of the pairs which have been observed more than once; and let V be the sun of the squares of all these residuals, N the total number of determinations, M the total number of 'pairs observed more than once, and Q (.6745) the factor for reduction of mean to probable errors. Then e,

the probable error of observation, is found by the formula,

1

حمد

V

Q2

N-M

.455

N-M

..(6)

Table III, below, exhibits the steps of the process for determining V.

TABLE III.

TO FIND THE PROBABLE ERROR OF OBSERVATION.

No. of pair

Stars of the pair; B. A. C. Nos.

Seconds of latitude

Means

V

#

#!

Г

9.55

0.68

.4624

9.54

0.69

.4761.

745-786

10.48

10,23

0.25

.0625

11.18

0.95

.9025

10.41

0.13

.0324

13.59

0.54

.2916

872-901

12.26

13.05

0.79

.6241

13.31

0.26

.0676

3

502-518

13.97

13.39

0.65

4225

1

999-1052

14.55

14.05

0.50

.2500

14.20

0.15

.0225

10.66

0.28

.0781

10

5

1097-1138

9.27

10.38

1.11

1.2321

11.22

0.84

.7056

12.27

0.70

.4900

6

574-628

11.57

10.87

0.70

.4900

12.56

0.03

.0009

1045-1052

11.82

12.53

0.71.

.5041

13.22

0.69

.4761

11.97

0.22

.0484***

.1326-1346

12.19

12.41

0.22

.0484

13.37

0.08

.0064

9

1391-1408

13.29

13.22

0.07

.0019

10

1408-1437

11.70

10.57

0.28

.0784

11

1726-1778

9.74

10.29

0.55

.3025

10.56

0.27

.0729

9.21

0.63

.3969

12

1937-1876

9.17

9.84

0.67

.4489

11.14

1.30

1.6900

13.75

0.59

.3481

13

510- 574

13.16

12.57

0.59

.3481

11.12

0.04

.0016-

14

1377-1444

11.16

11.20

0.04

.0016

13.15

0.03

.0009

15

1420-1444

13.12

13.09

0 03

.0009

13.24

0.12

0144,

16

1602-1687

14.90

13.36

1.54

2.3716

11.93

1.43

2.0449

9.83

0.03

17

1958-2001

9.86

9.89

0.03

.0009

00094€

18

1408-1432

11.70

1

12.72

0.23

تشير

.0529

19

1893-1900

12.49

12.26

0.23

.0529***

20

1990-2082

13.47

Page 120Page 121

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