Paper
6 July 2018 New wavefront-sensing guiders for SOAR
Author Affiliations +
Abstract
The 4.1-m SOAR telescope needs fast tip-tilt guiding and active correction of focus and astigmatism to reach good image quality allowed by the excellent site seeing. A concept of the new guider with a 2×2 wavefront sensor is presented. It uses the X-Y positioning mechanism of the current guider, while the pick-off arm, camera, and detector are replaced by the new hardware. The pick-off arm has 2 positive lenses to collimate the beam, with an internal focus adjustment to compensate for focus offset in the science instrument and for the field curvature. The 4 spots are formed by a mirror with slightly tilted segments, located near the camera. The detector is an EM CCD; guiding on stars as faint as V=17 mag is possible using the correlation algorithm for centroiding; aberrations are measured on the averaged images. Results of the on-sky tests of the new guider prototype are presented.
© (2018) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrei Tokovinin, Nicole David, José Piracés, and Rolando Cantarutti "New wavefront-sensing guiders for SOAR", Proc. SPIE 10702, Ground-based and Airborne Instrumentation for Astronomy VII, 107022F (6 July 2018); https://doi.org/10.1117/12.2312082
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Stars

Cameras

Sensors

Telescopes

Charge-coupled devices

Vignetting

RELATED CONTENT

The Keck Cosmic Web Imager
Proceedings of SPIE (July 19 2010)
Segment Alignment For The Keck Telescope Primary Mirror
Proceedings of SPIE (August 20 1986)
OAJ: 2.6m wide field survey telescope
Proceedings of SPIE (September 17 2012)
All-spherical wide-field camera
Proceedings of SPIE (November 19 2021)

Back to Top