Design and development of Cassegrain module for PARAS-2 spectrograph (CAMPAS)

We present here the design and development of the Cassegrain Module for the PARAS-2 spectrograph (CAMPAS). PARAS-2 is a high-resolution fiber-fed echelle spectrograph developed for the PRL 2.5 m telescope. The CAMPAS acts as a coupler between two optical systems, the PRL 2.5 m telescope and the PARAS-2 spectrograph. It has primarily been developed for the precise injection of the light beam into the optical fibers of the PARAS-2 spectrograph. The CAMPAS consists of a focal reducer, beam-guiding optics, an atmospheric dispersion corrector, optical fiber mounts, a calibration unit incorporating calibration lamps and beam-guiding optics, and other auxiliary subsystems. It was developed in-house at PRL, Ahmedabad, between the years 2020 and 2022 and was installed at one of the two side ports of the PRL 2.5 m telescope in March 2022. It is one of the first light instruments for the PRL 2.5 m telescope. The CAMPAS serves critical purposes of precise fiber feed, point spread function estimation, and atmospheric dispersion correction.

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Publication Details

Journal
Journal of Astronomical Telescopes Instruments and Systems
Published
2025-10-15
DOI
https://doi.org/10.1117/1.jatis.11.4.045003
Primary Topic
Geophysics and Gravity Measurements
Type
article
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article

Design and development of Cassegrain module for PARAS-2 spectrograph (CAMPAS)

Kevikumar A. Lad, Abhijit Chakraborty, Rishikesh Sharma, Neelam J. S. S. V. Prasad et al.
Journal of Astronomical Telescopes Instruments and Systems
Geophysics and Gravity Measurements
article

Design and development of Cassegrain module for PARAS-2 spectrograph (CAMPAS)

Kevikumar A. Lad, Abhijit Chakraborty, Rishikesh Sharma, Neelam J. S. S. V. Prasad, Ashirbad Nayak, Kapil K. Bharadwaj, Nikitha Jithendran, Vishal Joshi
article en

Abstract

We present here the design and development of the Cassegrain Module for the PARAS-2 spectrograph (CAMPAS). PARAS-2 is a high-resolution fiber-fed echelle spectrograph developed for the PRL 2.5 m telescope. The CAMPAS acts as a coupler between two optical systems, the PRL 2.5 m telescope and the PARAS-2 spectrograph. It has primarily been developed for the precise injection of the light beam into the optical fibers of the PARAS-2 spectrograph. The CAMPAS consists of a focal reducer, beam-guiding optics, an atmospheric dispersion corrector, optical fiber mounts, a calibration unit incorporating calibration lamps and beam-guiding optics, and other auxiliary subsystems. It was developed in-house at PRL, Ahmedabad, between the years 2020 and 2022 and was installed at one of the two side ports of the PRL 2.5 m telescope in March 2022. It is one of the first light instruments for the PRL 2.5 m telescope. The CAMPAS serves critical purposes of precise fiber feed, point spread function estimation, and atmospheric dispersion correction.

Journal of Astronomical Telescopes Instruments and SystemsVol. 11(04)
Physical Research Laboratory (IN)
Openalex Percentile: Top 71%
Geophysics and Gravity Measurements
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Design and development of Cassegrain module for PARAS-2 spectrograph (CAMPAS) — Kevikumar A. Lad, Abhijit Chakraborty, et al. · Journal of Astronomical Telescopes Instruments and Systems (2025) | TGRS Research Map | TGRS