Simple Improved Reference Subtraction for H4RG, H2RG, and H1RG Near-infrared Array Detectors
arXiv:2602.02253 · doi:10.1117/1.JATIS.8.2.028002
Abstract
Teledyne's H4RG, H2RG, and H1RG near-infrared array detectors provide reference pixels embedded in their data streams. Although they do not respond to light, the reference pixels electronically mimic normal pixels and track correlated read noise. In this paper, we describe how the reference pixels can be used with linear algebra and training data to optimally reduce correlated read noise. Simple Improved Reference Subtraction (SIRS) works with common detector clocking patterns and, when applicable, relies only on post-processing existing data so long as the reference pixels are available. The resulting reference correction is optimal, in a least squares sense, when the embedded reference pixels are the only references and the reference columns on the left and right are treated as two reference streams. We demonstrate SIRS using H4RG ground test data from the Nancy Grace Roman Space Telescope Project. The Julia language SIRS software is freely available for download from the NASA GitHub. The package includes a python-3 ``backend'' that can be used to apply SIRS corrections if a SIRS calibration file has been provided by the instrument builders.
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Cited by in corpus (3)
- A Joint Roman Space Telescope and Rubin Observatory Synthetic Wide-Field Imaging Survey
- Analysis of biasing from noise from the Nancy Grace Roman Space Telescope: implications for weak lensing
- Spot-Based Measurement of the Brighter-Fatter Effect on a Roman Space Telescope H4RG Detector and Comparison with Flat-Field Data