English

On-instrument wavefront sensor design for the TMT infrared imaging spectrograph (IRIS) update

Instrumentation and Methods for Astrophysics 2015-06-22 v1

Abstract

The first light instrument on the Thirty Meter Telescope (TMT) project will be the InfraRed Imaging Spectrograph (IRIS). IRIS will be mounted on a bottom port of the facility AO instrument NFIRAOS. IRIS will report guiding information to the NFIRAOS through the On-Instrument Wavefront Sensor (OIWFS) that is part of IRIS. This will be in a self-contained compartment of IRIS and will provide three deployable wavefront sensor probe arms. This entire unit will be rotated to provide field de-rotation. Currently in our preliminary design stage our efforts have included: prototyping of the probe arm to determine the accuracy of this critical component, handling cart design and reviewing different types of glass for the atmospheric dispersion.

Keywords

Cite

@article{arxiv.1407.2999,
  title  = {On-instrument wavefront sensor design for the TMT infrared imaging spectrograph (IRIS) update},
  author = {Jennifer Dunn and Vlad Reshetov and Jenny Atwood and John Pazder and Bob Wooff and David Loop and Leslie Saddlemyer and Anna M. Moore and James E. Larkin},
  journal= {arXiv preprint arXiv:1407.2999},
  year   = {2015}
}

Comments

Proceedings of the SPIE, 9147-354

R2 v1 2026-06-22T05:01:26.702Z