Arriola, AGross, SAms, MGretzinger, TLe Coq, DWang, R. PEbendorff-Heidepriem, HSanghera, JBayya, SShaw, L. BIreland, MichaelTuthill, PWithford, M. J2017-03-28http://hdl.handle.net/1885/114003The mid-infrared wavelength regime 3:5 􀀀 4:1 m, known as the astronomical L’ band is of special interest for exoplanet hunting. Mid-IR compatible photonic technologies are an enabling platform for a range of critical observational science using compact instruments on the next generation of Extremely Large Telescopes. Pupil remapping interferometry is a technique in which subapertures of the telescope pupil (2D) are reformatted into a 1D linear array. This can be done efficiently using 3D photonics. One of the most important techniques to fabricate 3D photonic devices in glass is ultrafast laser inscription. However, common silicate glasses are opaque above 2-2.2 m and therefore not useful for the fabrication of waveguides at mid-infrared wavelengths. Here we present a study of mid-infrared transparent materials that are compatible with the ultrafast laser inscription technique. This study will inform the development of mid-infrared photonic devices for future exoplanetary discovery.This research was supported by the Australian Research Council Centre of Excellence for Ultrahigh bandwidth Devices for Optical Systems (project number CE110001018) and was performed in part at the Optofab node of the Australian National Fabrication Facility using Commonwealth and NSW and SA State Government funding. S. Gross acknowledges funding by a Macquarie University Research Fellowship.14 pagesapplication/pdf© 2017 Optical Society of AmericaGlass waveguidesInfraredLaser materials processingMicrostructure fabricationAstronomical opticsAstronomy and astrophysics2017-03-0110.1364/OME.7.000698