Abstract
Major atmospheric Cherenkov experiment (MACE) is a ground-based imaging atmospheric Cherenkov telescope installed at Hanle (~4.3 km above sea level), Ladakh in the northern region of India. With a large parabolic reflector of 21 m diameter and 25 m focal length, MACE telescope is expected to explore the γ-ray Universe above 20 GeV. The tesselated light collector of MACE telescope employs 356 mirror panels each of size ~1m × 1m. The individual panel comprises of 4 metallic mirror facets each of size ~0.5m × 0.5m with a similar focal length. All 1424 mirror facets (356 × 4) are aligned in such a way that the whole reflector functions approximately as a single quasi-parabolic mirror of area ~339 m2 with a focal length varying from 25 m in the central region to 26.16 m on the periphery. Here, we describe the methodology for developing the metallic mirrors using the diamond turning technique. We also present the results from the testing and characterization of ~1500 mirror facets, which qualify all the optical requirements of the MACE reflector. The testing of mirrors includes dimensionality, water ingress and environmental tests. The optical characterization of individual mirror facets is based on the measurements of focal length, spot size and reflectance.
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Acknowledgments
The authors are thankful to the anonymous reviewer for his/her suggestions in improving the manuscript. They also thank their colleagues from the Astrophysical Sciences Division, Center for Design & Manufacturing, and Atomic & Molecular Physics Division at Bhabha Atomic Research Centre for their contributions at different stages in the development of metallic mirror facets for the MACE telescope. Help rendered by Dr S. K. Ghosh from the Materials Processing & Corrosion Engineering Division for surface roughness measurements is duly acknowledged. The authors are also thankful to the Electronics Corporation of India Limited (ECIL) and Paras Defence & Space Technologies, Mumbai (earlier Mechvac India Limited) for providing the mirror facet development facilities. They dedicate this study to the memory of their colleague Dr A. K. Tickoo who passed away in February 2021.
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This article is part of the Special Issue on "Astrophysical Jets and Observational Facilities: A National Perspective".
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DHAR, V.K., SINGH, K.K., VENUGOPAL, K. et al. Development of a new type of metallic mirrors for 21m MACE γ-ray telescope. J Astrophys Astron 43, 17 (2022). https://doi.org/10.1007/s12036-022-09799-7
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DOI: https://doi.org/10.1007/s12036-022-09799-7