English

DOTIFS: fore-optics and calibration unit design

Instrumentation and Methods for Astrophysics 2018-10-10 v1

Abstract

We present fore-optics and calibration unit design of Devasthal Optical Telescope Integral Field Spectrograph (DOTIFS). DOTIFS fore-optics is designed to modify the focal ratio of the light and to match its plate scale to the physical size of Integral Field Units (IFUs). The fore-optics also delivers a telecentric beam to the IFUs on the telescope focal plane. There is a calibration unit part of which is combined with the fore-optics to have a light and compact system. We use Xenon-arc lamp as a continuum source and Krypton/Mercury-Neon lamps as wavelength calibration sources. Fore-optics and calibration unit shares two optical lenses to maintain compactness of the overall subsystem. Here we present optical and opto-mechanical design of the calibration unit and fore-optics as well as calibration scheme of DOTIFS.

Keywords

Cite

@article{arxiv.1810.03627,
  title  = {DOTIFS: fore-optics and calibration unit design},
  author = {Haeun Chung and A. N. Ramaprakash and Pravin Khodade and Chaitanya V. Rajarshi and Sabyasachi Chattopadhyay and Pravin A. Chordia and Amitesh Omar and Changbom Park},
  journal= {arXiv preprint arXiv:1810.03627},
  year   = {2018}
}

Comments

7 pages, 8 figures, Conference poster at SPIE Astronomical Telescopes + Instrumentation, 2018, Austin, Texas, United States

R2 v1 2026-06-23T04:32:33.590Z