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An optical-UV survey of the North Celestial Cap

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Abstract

We present preliminary results of an optical-UV survey of the North Celestial Cap (NCCS) based on ∼5% areal coverage. The NCCS will provide good photometric and astrometric data for the North Celestial Cap region (80°≤δ≤90°). This region, at galactic latitudes from 17°≲b≲37°, is poorly covered by modern CCD-based surveys. The expected number of detected objects in NCCS is ∼1,500,000. We discuss issues of galactic structure, extinction, and the galaxy clustering in the colour-colour diagrams.

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Correspondence to Evgeny Gorbikov.

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Gorbikov, E., Brosch, N. An optical-UV survey of the North Celestial Cap. Astrophys Space Sci 335, 217–222 (2011). https://doi.org/10.1007/s10509-011-0603-3

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  • DOI: https://doi.org/10.1007/s10509-011-0603-3

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