Abstract: An axiconic telescope that receives a collimated input light beams and includes a first axicon and second axicon. Depending on the distance between the two axicons, the input collimated beam is converted to a diverging conical wave front by the first axicon, which is re-collimated by the second axicon having an oppositely signed cone angle. The output of the telescope is a collimated beam having an annular cross section, with the annulus having a width of dependent on the diameter of the telescope. The axiconic telescope may be used to produce an output beam having annulus size that can be optimized to illuminate a portion of a transducer in an solid immersion lens or photon tunning method device that contributes evanescent waves to increase resolution of an optical device.