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Depth-Of-Field Tables for the CINE-SERVO 50-1000mm T5.0-8.9 EF/PL lens.
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... 0.01 mm f = 50 f = 75 f = 100 f = 200 f = 500 f = 1000 ... 0.01 mm f = 50 x ... ... 89 1120. 28 35.07 ... f = 75 x ... f = 100 x ... ... 66 109. 28 1201.12 ... f = 200 x ... f = 500 x ... ... 78 202. 28 196.87 ... f = 1000 x ... ... 0.01 mm f = 50 ... 7.69 4.5 ... 5.45 3.5 3.33 ... f = 75
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Depth-Of-Field Tables for the CINE-SERVO 17-120mm T2.95-3.9 EF/PL
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... 0.01 mm f = 17 mm T 4 T5 .6 ... 25.61 4.5 ... 9.49 3.5 f = 25 mm T 4 T5 .6 ... 8.02 4.5 ... 5.50 3.5 f = 35 mm T 4 T5 .6 ... 6.16 4.5 ... 4.63 3.5 f = 50 mm T 4 T5 .6 ... 5.50 4.5 ... 4.29 3.5 f = 90 mm T 4
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CINEMA EOS LENSES
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The curves shown in Figures 4 and 5 yield the anticipated MTF characteristics at one specific spatial frequency – namely, 40 line pairs per millimeter (LP/ mm ). Given that the optical Nyquist frequency for a 4K lens is twice that – at80LP/mm– the question might be asked: why look at half that defining boundary spatial frequency? Many years of accumulated experiences in cinematography have shown that the most important region of an MTF curve lies in its central region.
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Depth-Of-Field Tables for the COMPACT-SERVO 18-80mm T4.4 EF/PL
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CN-E18-80 mm T4.4 L IS KAS S ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6 ... T4. 4 T5 .6
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CINEMA EOS LENSES
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3 Figure 5 Showing a typical Relative Light Distribution characteristic for a Super 35 mm cine zoom lens
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