PRAXIS: a low background NIR spectrograph for fibre Bragg grating OH suppression

TL;DR

PRAXIS is a specially designed low-background near-infrared spectrograph optimized for fibre Bragg grating OH suppression, aiming to significantly improve sky background reduction in astronomical observations.

Contribution

It introduces a cryogenic, fibre-fed spectrograph optimized for OH suppression, with modular design for adaptability and enhanced sensitivity in the J and H bands.

Findings

Simulations show existing spectrographs cannot fully exploit OH suppression benefits.

PRAXIS's design minimizes thermal and instrumental backgrounds.

Expected to improve sky noise limited observations in NIR astronomy.

Abstract

Fibre Bragg grating (FBG) OH suppression is capable of greatly reducing the bright sky background seen by near infrared spectrographs. By filtering out the airglow emission lines at high resolution before the light enters the spectrograph this technique prevents scattering from the emission lines into interline regions, thereby reducing the background at all wavelengths. In order to take full advantage of this sky background reduction the spectrograph must have very low instrumental backgrounds so that it remains sky noise limited. Both simulations and real world experience with the prototype GNOSIS system show that existing spectrographs, designed for higher sky background levels, will be unable to fully exploit the sky background reduction. We therefore propose PRAXIS, a spectrograph optimised specifically for this purpose. The PRAXIS concept is a fibre fed, fully cryogenic, fixed format spectrograph for the J and H-bands. Dark current will be minimised by using the best of the latest generation of NIR detectors while thermal backgrounds will be reduced by the use of a cryogenic fibre slit. Optimised spectral formats and the use of high throughput volume phase holographic gratings will further enhance sensitivity. Our proposal is for a modular system, incorporating exchangeable fore-optics units, integral field units and OH suppression units, to allow PRAXIS to operate as a visitor instrument on any large telescope and enable new developments in FBG OH suppression to be incorporated as they become available. As a high performance fibre fed spectrograph PRAXIS could also serve as a testbed for other astrophotonic technologies.