A measurement of the systematic astrometric error in GeMS and the short-term astrometric precision in ShaneAO

From National Research Council Canada

DOI	Resolve DOI: https://doi.org/10.1117/12.2057233
Author	Search for: Ammons, S. Mark; Search for: Neichel, Benoit; Search for: Lu, Jessica; Search for: Gavel, Donald T.; Search for: Srinath, Srikar; Search for: McGurk, Rosalie; Search for: Rudy, Alex; Search for: Rockosi, Connie; Search for: Marois, Christian¹ ; Search for: MacIntosh, Bruce; Search for: Savransky, Dmitry; Search for: Galicher, Raphael; Search for: Bendek, Eduardo; Search for: Guyon, Olivier; Search for: Marin, Eduardo; Search for: Garrel, Vincent; Search for: Sivo, Gaetano
Name affiliation	National Research Council Canada. National Science Infrastructure
Format	Text
Type	Article
Proceedings title	SPIE - International Society for Optical Engineering. Proceedings
Conference	Adaptive Optics Systems IV, 22 June 2014 through 27 June 2014
ISSN	0277-786X
ISBN	9780819496164
Volume	9148
Article number	91481J
Subject	Degrees of freedom (mechanics); Linear transformations; Mathematical transformations; Stars; Systematic errors; Tomography; astrometry; Brown dwarfs; M92; multi-conjugate; NGC 1851; Adaptive optics
Abstract	We measure the long-term systematic component of the astrometric error in the GeMS MCAO system as a function of field radius and Ks magnitude. The experiment uses two epochs of observations of NGC 1851 separated by one month. The systematic component is estimated for each of three field of view cases (15'' radius, 30'' radius, and full field) and each of three distortion correction schemes: 8 DOF/chip + local distortion correction (LDC), 8 DOF/chip with no LDC, and 4 DOF/chip with no LDC. For bright, unsaturated stars with 13 < Ks < 16, the systematic component is < 0.2, 0.3, and 0.4 mas, respectively, for the 15'' radius, 30'' radius, and full field cases, provided that an 8 DOF/chip distortion correction with LDC (for the full-field case) is used to correct distortions. An 8 DOF/chip distortion-correction model always outperforms a 4 DOF/chip model, at all field positions and magnitudes and for all field-of-view cases, indicating the presence of high-order distortion changes. Given the order of the models needed to correct these distortions (∼8 DOF/chip or 32 degrees of freedom total), it is expected that at least 25 stars per square arcminute would be needed to keep systematic errors at less than 0.3 milliarcseconds for multi-year programs. We also estimate the short-term astrometric precision of the newly upgraded Shane AO system with undithered M92 observations. Using a 6-parameter linear transformation to register images, the system delivers ∼0.3 mas astrometric error over short-term observations of 2-3 minutes.
Publication date	2014-08-07
Publisher	SPIE
Terms of use	Permission is granted to temporarily download one copy of the materials for personal, noncommercial transitory viewing only. NRC Publications Archive - Copyright and terms of use
Language	English
Peer reviewed	Yes
NPARC number	21275455
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Record identifier	49343b15-02eb-4388-8011-69dbdbc37ba4
Record created	2015-07-14
Record modified	2017-04-24

Date modified:: 2019-03-24

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