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New Astronomical Reduction of Old Observations (the NAROO project)

Published online by Cambridge University Press:  07 March 2018

Jean-Eudes Arlot
Affiliation:
IMCCE, Observatoire de Paris, UMR 8028 CNRS, PSL, 77 avenue Denfert-Rochereau, F-75014 Paris, France email: [email protected]
Vincent Robert
Affiliation:
IMCCE, Observatoire de Paris, UMR 8028 CNRS, PSL, 77 avenue Denfert-Rochereau, F-75014 Paris, France email: [email protected] IPSA, Institut Polytechnique des Sciences Avancees, 63 boulevard de Brandebourg, F-94200 Ivry sur Seine, France email: [email protected]
Valery Lainey
Affiliation:
IMCCE, Observatoire de Paris, UMR 8028 CNRS, PSL, 77 avenue Denfert-Rochereau, F-75014 Paris, France email: [email protected]
Coralie Neiner
Affiliation:
LESIA, Observatoire de Paris, UMR 8109 CNRS, PSL, email: [email protected]
Nicolas Thouvenin
Affiliation:
IMCCE, Observatoire de Paris, UMR 8028 CNRS, PSL, 77 avenue Denfert-Rochereau, F-75014 Paris, France email: [email protected]
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Abstract

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The Gaia astrometric reference catalogue will provide star proper motions with an accuracy of one mas one century ago for stars of magnitude 14 or brighter. Our project is to re-reduced the old observations with the new catalogue allowing to have an astrometric accuracy only limited by the observational biases and not by reference stars. Then, we plan to get an accuracy of 50 mas where the old reductions were not better than 500 mas!

For our purpose, we will digitize old photographic plates with a sub-micrometric scanner. Tests were made using the UCAC catalogue showing that old photographic plates have an intrinsect accuracy of 30 to 60 mas.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2018 

References

Robert, V., Pascu, D., Lainey, V., Arlot, J.-E., De Cuyper, J.-P., Dehant, V., & Thuillot, W., 2016, Astron. Astrophys., 596, A37 CrossRefGoogle Scholar