The Infrared Imaging Spectrograph (IRIS) for TMT: Volume phase holographic grating performance testing and discussion
Shaojie Chen, Elliot Meyer, Shelley A. Wright, Anna M. Moore, James E., Larkin, Jerome Maire, Etsuko Mieda, and Luc Simard

TL;DR
This paper evaluates the performance of volume phase holographic gratings for the IRIS instrument on TMT, demonstrating high efficiency in the near-infrared with detailed lab measurements and analysis of angular dependence.
Contribution
It provides the first detailed efficiency testing of near-infrared VPH gratings for IRIS, showing their suitability for high-throughput spectrograph applications.
Findings
Peak efficiencies of ~88% at H-band and 90.23% at J-band in lab tests.
Efficiency drops of 20-28% when deviating from the Bragg angle.
VPH gratings are promising dispersing elements for IRIS.
Abstract
Maximizing the grating efficiency is a key goal for the first light instrument IRIS (Infrared Imaging Spectrograph) currently being designed to sample the diffraction limit of the TMT (Thirty Meter Telescope). Volume Phase Holographic (VPH) gratings have been shown to offer extremely high efficiencies that approach 100% for high line frequencies (i.e., 600 to 6000l/mm), which has been applicable for astronomical optical spectrographs. However, VPH gratings have been less exploited in the near-infrared, particularly for gratings that have lower line frequencies. Given their potential to offer high throughputs and low scattered light, VPH gratings are being explored for IRIS as a potential dispersing element in the spectrograph. Our team has procured near-infrared gratings from two separate vendors. We have two gratings with the specifications needed for IRIS current design:…
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