OF THE ROGER N. CLARK
OF THE ROGER N. CLARK
OF THE ROGER N. CLARK
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G<br />
VISUAL ASTRONOMY <strong>OF</strong> <strong>THE</strong> DEEP SKY<br />
Table F.5 (cont. )<br />
APPENDIX F: OPTIMUM DETECTION MAGNIFICATIONS FOR DEEP-SKY OBJECTS<br />
TELEDOM examples<br />
15<br />
x = (sb-sbx(i» / (sbx( i+l ) -sbx (i» *<br />
1 (opv(i+l ) -opv(i» + opv(i)<br />
go to 500<br />
c<br />
c sb less than beginning of table<br />
c<br />
100 x = opv( l)<br />
go to 500<br />
c<br />
c sb greater than last in table<br />
c<br />
200 x = (sb-sbx(17» / (sbx(18)-sbx(17» *<br />
1 (opv( 18)-opv( 17» + opv(17)<br />
c<br />
c compute opvang from x<br />
c<br />
500 if (x.gt.37.0) x=37 .0<br />
if (x.lt. - 37 .0) x= - 37 .0<br />
c*debug<br />
c*debugSOS<br />
c*debug<br />
c*debug<br />
wr ite (6,505) i,sb, sbx(i), sbx(i+l), opv(i), opv(i+l ), x<br />
format (lx,<br />
1 sb sbx(i) sbx (i+l ) opv(i) opv(i+l ) x',<br />
2 /, lx, i2, 6(£7.3, lx) , /, lx, 72( lh - »<br />
opvang = 10 .0 ** x<br />
c<br />
c limit opvang to 360.0 arc-minutes .<br />
c<br />
if (opvang .gt. 360 .0) opvang<br />
360.0<br />
Each example shows the user input in bold .<br />
Example 1: NGC 134:<br />
***** Program Teleodm : Telescope Optimum Detection Magnification *****<br />
Enter the telescope aperture in inches<br />
8.<br />
Enter the total magnitude of the object<br />
11.4<br />
Enter the minimum and maximum sizes of the object in arc - minutes<br />
5. ,1.<br />
Telescope aperture : 8.0 inches<br />
Minimum usable magnification: 27x<br />
Faintest star : 15.2<br />
Object size : 5.00 by 1.00 arc minutes<br />
surface brightness (magnitudes / sq . arc- sec. ):<br />
object with no telescope: 21.8<br />
reduction due to ODM: 4.6<br />
object in telescope at ODM : 26.2<br />
background in telescope at ODM : 28 .8<br />
ODM :<br />
187x<br />
return<br />
end<br />
Log object contrast: 1.0<br />
Log threshold contrast : .6<br />
The object is detectable<br />
348<br />
349