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  5. Optimal Differential Astrometry for Multiconjugate Adaptive Optics. I. Astrometric Distortion Mapping using On-sky GeMS Observations of NGC 6723
 

Optimal Differential Astrometry for Multiconjugate Adaptive Optics. I. Astrometric Distortion Mapping using On-sky GeMS Observations of NGC 6723

Journal
THE ASTRONOMICAL JOURNAL  
Date Issued
2022
Author(s)
Taheri, Mojtaba
•
McConnachie, Alan W.
•
Turri, Paolo
•
MASSARI, DAVIDE  
•
Andersen, David
•
BONO, Giuseppe  
•
FIORENTINO, Giuliana  
•
Venn, Kim
•
Véran, Jean-Pierre
•
Stetson, Peter B.
DOI
10.3847/1538-3881/ac5747
Abstract
The Extremely Large Telescope and the Thirty Meter Telescope will use state of the art multiconjugate adaptive optics (MCAO) systems to obtain the full D 4 advantage that their apertures can provide. However, to reach the full astrometric potential of these facilities for on-sky science requires understanding any residual astrometric distortions from these systems and find ways to measure and eliminate them. In this work, we use Gemini multiconjugate adaptive optic system (GeMS) observations of the core of NGC 6723 to better understand the on-sky astrometric performance of MCAO. We develop new methods to measure the astrometric distortion fields of the observing system, which probe the distortion at the highest possible spatial resolution. We also describe methods for examining the time-variable and static components of the astrometric distortion. When applied to the GeMS Gemini South Adaptive Optics Imager (GSAOI) data, we are able to see the effect of the field rotator at the subpixel level, and we are able to empirically derive the distortion due to the optical design of GeMS/GSAOI. We argue that the resulting distortion maps are a valuable tool to measure and monitor the on-sky astrometric performance of future instrumentation. Our overall astrometry pipeline produces high-quality proper motions with an uncertainty floor of ~45 μas yr-1. We measure the proper motion dispersion profile of NGC 6723 from a radius of ~10″ out to ~1' based on ~12,000 stars. We also produce a high-quality optical-near infrared color-magnitude diagram, which clearly shows the extreme horizontal branch and main-sequence knee of this cluster.
Volume
163
Issue
4
Start page
187
Uri
http://hdl.handle.net/20.500.12386/35532
Url
https://iopscience.iop.org/article/10.3847/1538-3881/ac5747
https://api.elsevier.com/content/abstract/scopus_id/85128931432
Issn Identifier
0004-6256
Ads BibCode
2022AJ....163..187T
Rights
open.access
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