CTAO NectarCAM Collaboration

arXiv2026

Towards the Deployment of the First NectarCAM, a Medium-Sized-Telescope Camera for the Cherenkov Telescope Array Observatory

NectarCAM is a Cherenkov camera designed to detect gamma rays with energies between 80 GeV and 50 TeV. It will equip nine medium-sized telescopes (MSTs) of the Cherenkov Telescope Array Observatory. NectarCAM consists of 1855 pixels distributed over 265 modules. Each pixel consists of a photomultiplier tube that is connected to a NECTAr3 chip. This NECTAr3 chip contains a 12-bit digitizer with a GHz sampling rate, and has a typical readout deadtime of ${\sim}0.7$ $\mu$s. In these proceedings, we highlight the performance of the NectarCAM in terms of time resolution and charge resolution. We also present the latest calibration techniques that were recently implemented for the camera. Finally, we briefly present the current status and plans of the NectarCAM production; the first production-line NectarCAM will be ready for shipment by Summer 2026, and it is planned to equip one of the MST pathfinders of CTAO.

astro-ph.IM↗

arXiv2025

Design and characterization of the Flat-Field Calibration of the NectarCAM Camera

The NectarCAM flat-field flasher is a calibration device designed for the camera that will equip the Medium-Sized Telescopes (MSTs) of the northern site of the Cherenkov Telescope Array Observatory (CTAO). Positioned in the centre of the MST dish, 16 meters in front of the camera, the flasher emits short (FWHM $\approx$ 5 ns), uniform (2$-$4%) light pulses to illuminate the entire focal plane. Accurate calibration is crucial for the optimal operation of the NectarCAM, ensuring precise gain computation and mitigating differences in light-collection efficiency of the pixels of the camera. Using the flat-field flasher, two informations are obtained : the pixel gain and the relative efficiency between pixels. In addition, the flasher is used to probe the dynamic range over which the camera operates effectively. In this study, we report on the performance characterisation of the flat-field flasher using a dedicated test bench. We report on the results of tests conducted on several flasher units, evaluating their reliability. Furthermore, we describe how the flat-field coefficients are applied within the camera to ensure uniformity of response of few percent level across all 1855 pixels. As the deployment of the first MST at the CTAO northern site is scheduled for 2027, this work represents a significant contribution to the collaboration`s efforts to finalize camera calibration systems.

astro-ph.IM↗