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The Ultra-High-Resolution Facility at the Anglo-Australian Telescope

DIEGO, F; FISH, AC; BARLOW, MJ; CRAWFORD, IA; SPYROMILIO, J; DRYBURGH, M; BROOKS, D; ... WALKER, DD; + view all (1995) The Ultra-High-Resolution Facility at the Anglo-Australian Telescope. Monthly Notices of the Royal Astronomical Society , 272 (2) pp. 323-332. 10.1093/mnras/272.2.323. Green open access

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Abstract

The Ultra-High-Resolution Facility (UHRF) has been commissioned at the coudé focus of the Anglo-Australian Telescope (AAT), and provides a resolving power of R≈106. This is the highest spectral resolution ever obtained by an optical astronomical spectrograph, and is intended mainly for astrophysical studies of cool interstellar clouds. This paper describes the development of this ambitious project, which includes diffraction-limited optical components, very tight specification for the optical configuration, and a new type of image slicer which allows ultra-high-resolution work towards faint stars. Astrophysical results from the first observing runs are presented to demonstrate the performance in terms of both resolution and throughput.

Type: Article
Title: The Ultra-High-Resolution Facility at the Anglo-Australian Telescope
Open access status: An open access version is available from UCL Discovery
DOI: 10.1093/mnras/272.2.323
Publisher version: https://doi.org/10.1093/mnras/272.2.323
Language: English
Additional information: This version is the version of record. For information on re-use, please refer to the publisher’s terms and conditions.
Keywords: line: profiles, instrumentation: spectrographs, ISM: atoms, ISM: clouds
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/10096158
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