The magnification of the telescope is given by formula
"m=\\frac {f_o}{f_e}= (1)"
where fo is objective focal distance, fe is the eye-piece focal distance
Mirror formula
"\\frac {1}{f}= \\frac {1}{v} + \\frac {1}{u} (2)"
We can rewrite formula (1) as
"m=\\frac {v}{u}=\\frac {f}{f+u} (3)"
Image distance is equal to
"u=-(f_o+f_e) (4)"
Using (2),(3),(4) we got
"m=\\frac {L}{I}"
Answer
"\\frac {L}{I}"
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