A generalized ray-tracing procedure for an atmospheric Cherenkov imaging telescope and optical characteristics of the TACTIC light collector

  • A. K. Tickoo
  • , R. L. Suthar
  • , R. Koul
  • , M. L. Sapru
  • , N. Kumar
  • , C. L. Kaul
  • , K. K. Yadav
  • , S. Thoudam
  • , S. K. Kaul
  • , K. Venugopal
  • , M. Kothari
  • , H. C. Goyal
  • , P. Chandra
  • , V. K. Dhar
  • , R. C. Rannot
  • , M. K. Koul
  • , S. R. Kaul

Research output: Contribution to journalArticlepeer-review

10 Scopus citations

Abstract

A generalized ray-tracing procedure has been developed, which facilitates the design of a multimirror-based light collector used in atmospheric Cherenkov telescopes. This procedure has been employed to study the optical characteristics of the 3.5 m diameter light collector of the TACTIC Imaging telescope. Comparison of the measured point-spread function of the light collector with the simulated performance of ideal Davies-Cotton and paraboloid designs has been made to determine an optimum arrangement of the 34 spherical mirror facets used in the telescope to obtain the best possible point-spread function. A description of the ray-tracing subroutine used for processing CORSIKA-generated Cherenkov data, required for carrying out Monte-Carlo simulation studies, is also discussed in the paper.

Original languageBritish English
Pages (from-to)177-190
Number of pages14
JournalNuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume539
Issue number1-2
DOIs
StatePublished - 21 Feb 2005

Keywords

  • γ-ray astronomy
  • Ray-tracing formalism
  • TACTIC telescope

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