High-order wavefront correction is not only beneficial for high-contrast imaging, but also spectroscopy. The size of a spectrograph can be decoupled from the size of the telescope aperture by moving to the diffraction limit which has strong implications for ELT based instrument design. Here we present the construction and characterization of an extremely efficient single-mode fiber feed behind an extreme adaptive optics system (SCExAO). We show that this feed can indeed be utilized to great success by photonic-based spectrographs. We present metrics to quantify the system performance and some preliminary spectra delivered by the compact spectrograph.
| Identifer | oai:union.ndltd.org:arizona.edu/oai:arizona.openrepository.com:10150/622807 |
| Date | 03 August 2016 |
| Creators | Jovanovic, N., Cvetojevic, N., Schwab, C., Norris, B., Lozi, J., Gross, S., Betters, C., Singh, G., Guyon, O., Martinache, F., Doughty, D., Tuthill, P. |
| Contributors | Univ Arizona, Steward Observ, Univ Arizona, Ctr Opt Sci, Subaru Telescope, National Astronomical Observatory of Japan (United States), Australian Astronomical Observatory (Australia), Macquarie Univ. (Australia), The Univ. of Sydney (Australia), Subaru Telescope, National Astronomical Observatory of Japan (United States), Macquarie Univ. (Australia), The Univ. of Sydney (Australia), Jet Propulsion Lab. (United States), Subaru Telescope, National Astronomical Observatory of Japan (United States), Observatoire de la Côte d’Azur (France), Subaru Telescope, National Astronomical Observatory of Japan (United States), The Univ. of Sydney (Australia) |
| Publisher | SPIE-INT SOC OPTICAL ENGINEERING |
| Source Sets | University of Arizona |
| Language | English |
| Detected Language | English |
| Type | Article |
| Rights | © 2016 SPIE |
| Relation | http://proceedings.spiedigitallibrary.org/proceeding.aspx?doi=10.1117/12.2234299 |
Page generated in 0.0022 seconds