Temperature-compensating package for OH line filters for astronomy: II. manufacture, assembly, and performance study

TL;DR

This paper introduces a self-compensating enclosure for fiber Bragg grating filters used in astronomy, achieving high wavelength stability over temperature variations, suitable for ground-based near-infrared observations.

Contribution

It presents a novel self-compensating enclosure design that significantly reduces wavelength drift in FBG filters without temperature control.

Findings

Maximum wavelength deviation of 12 pm over thermal cycles

Wavelength drift of only 0.37 pm/°C

Athermalization factor of 1/22

Abstract

Multi-channel aperiodic fiber Bragg grating (FBG) based hydroxyl (OH) line filters have attracted significant interest in ground-based near-infrared (NIR) astronomical observations. In this paper, we present the performance of a new self-compensating enclosure for the filters, that can be used in non-temperature-controlled environments. Our prototype encloses a 110 mm long single-mode photosensitive optical fiber with three 10 mm filter gratings. A fourth grating was used as a reference outside the package to measure the uncompensated wavelength shift. The prototype was tested over three thermal cycles, and showed a maximum wavelength deviation of 12 pm, a wavelength drift of only 0.37 pm/$^{\circ}$C, over the temperature range of -17$^{\circ}$C to 15$^{\circ}$C. The athermalization factor, i.e., the ratio of the maximum wavelength shift of the compensated grating to the uncompensated reference filter grating was $\frac{1}{22}$. The results demonstrate the capability of the prototype for stabilizing multi-channel long-length FBGs or chirped FBGs, particularly for astronomical applications that require sub-picometer stability.