Simulation and Optimization of an Astrophotonic Reformatter

TL;DR

This paper simulates and optimizes an astrophotonic reformatter called the photonic dicer, demonstrating improvements in throughput and stability, which are crucial for advancing astronomical spectrograph design.

Contribution

It provides a detailed simulation and optimization of the photonic dicer, showing how to enhance throughput and reduce modal noise for better astronomical instrumentation.

Findings

Transmission of 8-20% depending on AO correction

Reduced modal noise with minimal slit barycentre variation

Throughput improved by 6.4% and slit movement reduced by 50%

Abstract

Image slicing is a powerful technique in astronomy. It allows the instrument designer to reduce the slit width of the spectrograph, increasing spectral resolving power whilst retaining throughput. Conventionally this is done using bulk optics, such as mirrors and prisms, however more recently astrophotonic components known as photonic lanterns (PLs) and photonic reformatters have also been used. These devices reformat the multi-mode (MM) input light from a telescope into single-mode (SM) outputs, which can then be re-arranged to suit the spectrograph. The photonic dicer (PD) is one such device, designed to reduce the dependence of spectrograph size on telescope aperture and eliminate modal noise. We simulate the PD, by optimising the throughput and geometrical design using Soapy and BeamProp. The simulated device shows a transmission between 8 and 20 %, depending upon the type of adaptive optics (AO) correction applied, matching the experimental results well. We also investigate our idealised model of the PD and show that the barycentre of the slit varies only slightly with time, meaning that the modal noise contribution is very low when compared to conventional fibre systems. We further optimise our model device for both higher throughput and reduced modal noise. This device improves throughput by 6.4 % and reduces the movement of the slit output by 50%, further improving stability. This shows the importance of properly simulating such devices, including atmospheric effects. Our work complements recent work in the field and is essential for optimising future photonic reformatters.