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Attaining m s⁻¹ level intrinsic Doppler precision with RHEA, a low-cost single-mode spectrograph

Feger, Tobias; Ireland, Michael; Schwab, Christian; Bento, Joao; Bacigalupo, Carlos; Coutts, David W.

Description

We present RHEA, a compact and inexpensive single-mode spectrograph which is built to exploit the capabilities of modest-sized telescopes in an economic way. The instrument is fed by up to seven optical waveguides with the aim of achieving an efficient and modal-noise-free unit, suitable for attaining extreme Doppler precision. The cross-dispersed layout features a wavelength coverage from 430-650 nm, with spectral resolution of R∼75,000. When coupled to small telescopes using fast tip/tilt...[Show more]

dc.contributor.authorFeger, Tobias
dc.contributor.authorIreland, Michael
dc.contributor.authorSchwab, Christian
dc.contributor.authorBento, Joao
dc.contributor.authorBacigalupo, Carlos
dc.contributor.authorCoutts, David W.
dc.date.accessioned2019-01-03T00:25:56Z
dc.identifier.issn0922-6435
dc.identifier.urihttp://hdl.handle.net/1885/154844
dc.description.abstractWe present RHEA, a compact and inexpensive single-mode spectrograph which is built to exploit the capabilities of modest-sized telescopes in an economic way. The instrument is fed by up to seven optical waveguides with the aim of achieving an efficient and modal-noise-free unit, suitable for attaining extreme Doppler precision. The cross-dispersed layout features a wavelength coverage from 430-650 nm, with spectral resolution of R∼75,000. When coupled to small telescopes using fast tip/tilt control, our instrument is well-suited to sensitive spectroscopy. Example science cases are accurate radial velocity studies of low to intermediate-mass giant stars with the purpose of searching for giant plants and using asteroseismology to simultaneously measure the host star parameters. In this paper we describe the final instrument design and present first results from testing the internal stability.
dc.description.sponsorshipThis research was partially funded by the Australian Research Council (ARC) Discovery Project DP120103751.
dc.format.mimetypeapplication/pdf
dc.publisherSpringer Verlag
dc.rights© Springer Science+Business Media Dordrecht 2016
dc.sourceExperimental Astronomy
dc.subjectInstrumentation
dc.subjectSingle-mode spectrograph
dc.subjectHigh-resolution
dc.subjectRadial velocity
dc.subjectTube lens
dc.subjectExtrasolar planets
dc.subjectAsteroseismology
dc.titleAttaining m s⁻¹ level intrinsic Doppler precision with RHEA, a low-cost single-mode spectrograph
dc.typeJournal article
local.identifier.citationvolume42
dc.date.issued2016
local.type.statusPublished Version
local.type.statusPublished Version
local.contributor.affiliationIreland, M., Research School of Astronomy & Astrophysics, The Australian National University
local.description.embargo2037-12-31
dc.relationhttp://purl.org/au-research/grants/arc/DP120103751
local.bibliographicCitation.issue3
local.bibliographicCitation.startpage285
local.bibliographicCitation.lastpage300
local.identifier.doi10.1007/s10686-016-9510-5
CollectionsANU Research Publications

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