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Final design and on-sky testing of the iLocater SX acquisition camera: broad-band single-mode fibre coupling
Author
Crass, JBechter, A
Sands, B
King, D
Ketterer, R
Engstrom, M
Hamper, R
Kopon, D
Smous, J
Crepp, J R
Montoya, M
Durney, O
Cavalieri, D
Reynolds, R
Vansickle, M
Onuma, E
Thomes, J
Mullin, S
Shelton, C
Wallace, K
Bechter, E
Vaz, A
Power, J
Rahmer, G
Ertel, S
Affiliation
Steward Observatory, University of ArizonaIssue Date
2020-10-30Keywords
Instrumentation: adaptive opticsInstrumentation: spectrographs
Techniques: high angular resolution
Metadata
Show full item recordPublisher
Oxford University PressCitation
Crass, J., Bechter, A., Sands, B., King, D., Ketterer, R., Engstrom, M., ... & Ertel, S. (2021). Final design and on-sky testing of the iLocater SX acquisition camera: broad-band single-mode fibre coupling. Monthly Notices of the Royal Astronomical Society, 501(2), 2250-2267.Rights
© 2020 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
Enabling efficient injection of light into single-mode fibres (SMFs) is a key requirement in realizing diffraction-limited astronomical spectroscopy on ground-based telescopes. SMF-fed spectrographs, facilitated by the use of adaptive optics (AO), offer distinct advantages over comparable seeing-limited designs, including higher spectral resolution within a compact and stable instrument volume, and a telescope independent spectrograph design. iLocater is an extremely precise radial velocity (EPRV) spectrograph being built for the Large Binocular Telescope (LBT). We have designed and built the front-end fibre injection system, or acquisition camera, for the SX (left) primary mirror of the LBT. The instrument was installed in 2019 and underwent on-sky commissioning and performance assessment. In this paper, we present the instrument requirements, acquisition camera design, as well as results from first-light measurements. Broad-band SMF coupling in excess of 35 per cent (absolute) in the near-infrared (0.97-1.31 ${\mu {\rm m}}$) was achieved across a range of target magnitudes, spectral types, and observing conditions. Successful demonstration of on-sky performance represents both a major milestone in the development of iLocater and in making efficient ground-based SMF-fed astronomical instruments a reality.ISSN
0035-8711EISSN
1365-2966Version
Final published versionSponsors
National Aeronautics and Space Administrationae974a485f413a2113503eed53cd6c53
10.1093/mnras/staa3355