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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

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