Paper
13 February 2003 Observations of faint galaxies with adaptive optics
Richard I. Davies, Matthew D. Lehnert, Andrew Baker, Niranjan A. Thatte, Alvio Renzini, Domenico Bonaccini
Author Affiliations +
Abstract
Encouraged by imaging of faint galaxies around bright stars using ALFA on the 3.5-m telescope at Calar Alto, we have begun a survey to identify a large number of candidate sources near bright stars. In this contribution we report the status of this survey and show our preliminary results from deep imaging around one of these stars during the early phases of CONICA and NAOS on the 8.2-m VLT. We outline the exciting prospects for this type of work in terms of number counts, morphology, and rotation curve analyses.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Richard I. Davies, Matthew D. Lehnert, Andrew Baker, Niranjan A. Thatte, Alvio Renzini, and Domenico Bonaccini "Observations of faint galaxies with adaptive optics", Proc. SPIE 4834, Discoveries and Research Prospects from 6- to 10-Meter-Class Telescopes II, (13 February 2003); https://doi.org/10.1117/12.457689
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Stars

Galactic astronomy

Adaptive optics

Point spread functions

Telescopes

K band

Cameras

Back to Top