Hector: performance of the new integral field spectrograph instrument for the Anglo-Australian Telescope

Le résumé fourni par la source

Hector is a new optical integral field spectrograph (IFS) instrument built by Astralis - Australia’s Astronomical Instrumentation Consortium. Hector was commissioned on the Anglo-Australian Telescope (AAT) in 2022. In 2023 it began a 15,000-galaxy IFS survey of nearby z< 0.1 galaxies. The high fill-factor imaging fibre bundles ‘hexabundles’ of the type used on the SAMI instrument, have been improved and enlarged to cover up to 27-arcsec diameter. The aim is to reach 2 effective radii on most galaxies. Hector has a unique and novel robotic positioner that compensates for varying telecentricity over the 2-degree-field of the AAT to recoup the light loss and correct the focus across the field. Hector has 21 hexabundles over that 2-degree field feeding both the new Hector spectrograph (Spector) and existing AAOmega spectrograph. The new dual-arm Spector spectrograph has the highest spectral resolution of any large IFS nearby galaxy survey of 1.3 Angstrom. This is key to enable higher order stellar kinematics to be measured on a larger fraction of galaxies and to link those galaxies to the large-scale environments in which they form. A data reduction pipeline has been developed and is producing science-quality galaxy cubes and the first internal data release is now being used for science.

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.