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          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents



ID: 731919.0, MPI für Astronomie / Publikationen_mpia
High-precision astrometry towards ELTs
Authors:Massari, D.; Fiorentino, G.; Tolstoy, E.; McConnachie, A.; Stuik, R.; Schreiber, L.; Andersen, D.; Clénet, Y.; Davies, R.; Gratadour, D.; Kuijken, K.; Navarro, R.; Pott, J.-U.; Rodeghiero, G.; Turri, P.; Verdoes Kleijn, G.
Place of Publication:Bellingham, Wash.
Publisher:SPIE
Date of Publication (YYYY-MM-DD):2016
Audience:Not Specified
Abstract / Description:With the aim of paving the road for future accurate astrometry with MICADO at the European-ELT, we performed an astrometric study using two different but complementary approaches to investigate two critical components that contribute to the total astrometric accuracy. First, we tested the predicted improvement in the astrometric measurements with the use of an atmospheric dispersion corrector (ADC) by simulating realistic images of a crowded Galactic globular cluster. We found that the positional measurement accuracy should be improved by up to 2 mas with the ADC, making this component fundamental for high-precision astrometry. Second, we analysed observations of a globular cluster taken with the only currently available Multi-Conjugate Adaptive Optics assisted camera, GeMS/GSAOI at Gemini South. Making use of previously measured proper motions of stars in the field of view, we were able to model the distortions affecting the stellar positions. We found that they can be as large as 200 mas, and that our best model corrects them to an accuracy of 1 mas. We conclude that future astrometric studies with MICADO requires both an ADC and an accurate modelling of distortions to the field of view, either through an a-priori calibration or an a-posteriori correction.
External Publication Status:published
Document Type:Other
Communicated by:N. N.
Affiliations:MPI für Astronomie
Identifiers:URL:http://adsabs.harvard.edu/abs/2016SPIE.9909E..1GM
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