MODHIS is a first light instrument that will enable high resolution spectroscopy from y-K band on the TMT. It is a single-mode fiber fed spectrograph that relies on the adaptive optics correction provided by NFIRAOS. By operating at the diffraction-limit the MODHIS spectrographs, split into two near identical units with a yJ and HK channel, are extremely compact and can be in the wedge room at the bottom of the building. Injecting light from a 30-m aperture into a single-mode fiber with a core size of the order of 5 microns requires a high-performance adaptive optics correction, schemes to eliminate non-common path errors, a high-quality correction to the differential atmospheric refraction, and precise pointing and tip/tilt control. These issues are currently under investigation with the pathfinder injection unit commissioned at Keck known as the Keck Planet Imager and Characterizer. MODHIS also leverages significant developments from a near identical precursor instrument aimed to be deployed to Keck in 2026: HISPEC.
In this paper we will present a technical overview of the instrument and discuss the subtleties of the single-mode-fiber feed on an ELT. These topics encompass adaptive optics acquisition and correction, tracking, and non-common path error correction.
| Subject : | : | poster |
| Topics | : | ELT Science with AO |
| Keywords | : | Exoplanets ; Diffraction ; limited ; high resolution spectroscopy ; PRV |
| PDF version | : |  PDF version |
