The Windows Design and the Restoration of Object Environments

Details The Windows Design and the Restoration of Object Environments The Windows Design and the Restoration of Object Environments

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.576..429d&link_type=abstract

"Proceedings of the Gaia Symposium "The Three-Dimensional Universe with Gaia" (ESA SP-576). Held at the Observatoire de Paris-Me

Astronomy and Astrophysics

Astrophysics

1

Gaia, Imaging, Methods Data Analysis

Scientific paper

For each object detected by Gaia, some windows are transmitted to the ground. Their design depends on the CCD rows of the astrometric fields and on the magnitude of the object. However, the limited telemetry rate limits the size of these windows. Given the selected windows for the Astro Sky Mapper (ASM) and the Astrometric Field 11 (AF11) of Gaia, it is worth investigating what kind of high angular resolution imaging will be achievable at the mission completion. We present a method to restore the environments of the detected objects and stress the astrophysical impact that can be achieved with the transmission of the data vectors issued from the two mentioned astrometric CCD rows.

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