Characterisation, performance, and operational aspects of the H4RG-15 near infrared detectors for the MOONS instrument
Derek Ives, Domingo Alvarez, Naidu Bezawada, Elizabeth George, and, Beno\^it Serra

TL;DR
This paper thoroughly characterizes the H4RG-15 near-infrared detectors used in the MOONS spectrograph, focusing on performance, operational temperature effects, and novel electronics development for optimal operation.
Contribution
It presents new insights into the performance of H4RG-15 detectors at various temperatures, introduces a novel cryogenic preamplifier, and details calibration techniques for improved data quality.
Findings
Lower operational temperatures improve detector performance.
The novel cryogenic preamplifier minimizes optical footprint and enhances signal quality.
Effective correction models for persistence and programming issues are developed.
Abstract
MOONS is a multi-object spectrograph for the ESO VLT covering a simultaneous wavelength range of 0.6-1.8 microns using approximately 1000 fibres. It uses four Teledyne Imaging Systems H4RG-15 4K x 4K detectors with 2.5 m cut-off material for the two longer wavebands (YJ and H). Since the spectrographs utilize an extremely fast modified Schmidt camera design, then the detectors are situated in the optical beam and hence required the development of a novel 64- channel cryogenic differential cryogenic preamplifier, minimized for optical footprint which will be reported on. We have operated the Engineering Grade H4RG detector at a range of temperatures from 90K to 40K and we will report on the advantages of the lower operational temperature. We have completed a full persistence analysis and are able to model it reasonably well and will offer a correction for it in our data pipeline. We…
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