Answers are grounded in this paper and cite their sources.
We have developed iodine (I₂) cells for the High Dispersion Spectrograph (HDS) on the Subaru telescope and for the HIgh Dispersion Echelle Spectrograph (HIDES) on the Okayama 1.88m reflector. The cell is put into a compact vacuum vessel, which fits into a small space behind the entrance slit of the HDS. The cell assembly is designed to minimize heat losses from the cell, which is heated during observations, to keep I₂ vapor from condensation. The amount of I₂ in the cell is determined to be best suited for radial-velocity measurements of solar-type stars. We also report on some performances of the HDS and HIDES as well as their instrumental profiles based on tests of our I₂ cells. Lastly, we discuss future improvements of our instruments and data-analysis softwares for I₂ observations, and also describe the scientific goals of our project.
No takes yet. Share an insight, caveat, or question.
Kambe et al. (2002) studied this question.
Synapse has enriched 10 related papers. Consider them for comparative context: