2014
DOI: 10.1002/asna.201312003
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The Subaru Telescope High Dispersion Spectrograph (HDS)

Abstract: The High Dispersion Spectrograph (HDS) is the échelle spectrograph for an open‐use instrument of the Subaru Telescope. The current status of the instrument is reviewed. The new image slicers that significantly improve the efficiency of observations with very high resolving power have been installed in the past three years. Brief overview of recent science results is given on studies of early generations of stars and extra‐solar planets. An upgrade plan and future prospects of this instrument are discussed. (© … Show more

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Cited by 22 publications
(1 citation statement)
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“…This will lead to a quasi-static correction to the computed velocity aberration point-ahead of the downlink from the observed OBT position, but also variation in the respective deflections due to turbulence that will be more difficult to compensate. The static dispersion of ∼ 4µrad displacement between the upgoing 532nm and downcoming 800nm beams is greatest at low elevations [89]. A correction can be included with the point-ahead compensation [14] .…”
Section: Atmospheric Scattering Absorption and Distortionmentioning
confidence: 99%
“…This will lead to a quasi-static correction to the computed velocity aberration point-ahead of the downlink from the observed OBT position, but also variation in the respective deflections due to turbulence that will be more difficult to compensate. The static dispersion of ∼ 4µrad displacement between the upgoing 532nm and downcoming 800nm beams is greatest at low elevations [89]. A correction can be included with the point-ahead compensation [14] .…”
Section: Atmospheric Scattering Absorption and Distortionmentioning
confidence: 99%