A CCD Modulation Detector for a Second Hipparcos Mission

Author:

Høg E.,Lindegren L.

Abstract

A CCD modulation detector for a possible Hipparcos-2 mission is described. It is at least 1000 times more light efficient than the image dissector tube system used in the current Hipparcos mission. A beam combiner telescope with 29 cm aperture diameter could measure all 15 million stars brighter than 14th magnitude, providing accurate multi-colour photometry in addition to the astrometric parameters. Using two telescopes with different basic angles will further improve the rigidity of the resulting system of positions and proper motions. An accuracy of 0.5 milli-arcsec up to 10th magnitude is expected for a 2.5 year mission. The modulating grid is imaged on a CCD performing a ‘cophased integration’ of nine separate images of the whole field of view, each image representing a different part of the modulation period.

Publisher

Cambridge University Press (CUP)

Reference6 articles.

1. Makarov V. , 1991, ‘Periodical errors of the Hipparcos star abscissae’, private comm., 6 pp.

2. UBVRI passbands

3. Determination of Division Corrections

4. H⊘g E. & Chubey M.S. , 1991, Proposal for a Second Hipparcos, in: Proceedings of the “Etalon-91” International Symposium, Moscow 1–5 June 1991, ed. Pochucayev V.N.

Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Astrometry and Photometry of 400 Million Stars Brighter than 18 Mag;Symposium - International Astronomical Union;1993

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