The TACTIC (TeV Atmospheric Cherenkov Telescope with Imaging Camera) is a 4 m imaging atmospheric Cherenkov telescope designed for very high-energy (VHE) gamma-ray observations and has been operational at Mount Abu, India, for over two decades. The telescope’s light collector has recently been upgraded to a tessellated structure comprising 34 spherical mirrors fabricated from single-point diamond-turned aluminum alloy (Al 6061-T6). Each mirror has a diameter of 600 mm and a focal length of ~4000 mm. Previously, the telescope employed glass mirrors of the same diameter, which required frequent aluminization due to degradation of reflectivity under prolonged atmospheric exposure. In this work, we present qualification studies of the diamond-turned metallic mirrors to evaluate their optical performance and environmental durability for Cherenkov light collection in the 300–700 nm wavelength range. The characterization includes spot size measurements using the 2f method, surface roughness evaluation, reflectivity assessment, and water ingress testing. Additionally, ray-tracing simulations were performed using ROBAST to estimate the point-spread function (PSF) for all 34 mirrors of the TACTIC telescope. The results demonstrate that the developed mirrors satisfy the required specifications and are suitable for long-term operation under site-specific environmental conditions.


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