A Two-Colour CCD Survey of the North Celestial Cap: I. The Method
| Autor: | Cristina Afonso, Evgeny Gorbikov, Noah Brosch |
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| Rok vydání: | 2009 |
| Předmět: |
Physics
Ccd camera Pixel Astronomy FOS: Physical sciences Astronomy and Astrophysics Astrometry Limiting Astrophysics - Astrophysics of Galaxies Galaxy Photometry (optics) Stars Space and Planetary Science Observatory Astrophysics of Galaxies (astro-ph.GA) Astrophysics - Instrumentation and Methods for Astrophysics Instrumentation and Methods for Astrophysics (astro-ph.IM) |
| DOI: | 10.48550/arxiv.0912.2355 |
| Popis: | We describe technical aspects of an astrometric and photometric survey of the North Celestial Cap (NCC), from the Pole (DEC=90 deg) to DEC=80 deg, in support of the TAUVEX mission. This region, at galactic latitudes from ~ 17 deg to ~ 37 deg, has poor coverage in modern CCD-based surveys. The observations are performed with the Wise Observatory one-meter reflector and with a new mosaic CCD camera (LAIWO) that images in the Johnson-Cousins R and I bands a one-square-degree field with subarcsec pixels. The images are treated using IRAF and SExtractor to produce a final catalogue of sources. The astrometry, based on the USNO-A2.0 catalogue, is good to ~ 1 arcsec and the photometry is good to ~ 0.1 mag for point sources brighter than R=20.0 or I=19.1 mag. The limiting magnitudes of the survey, defined at photometric errors smaller than 0.15 mag, are 20.6 mag (R) and 19.6 (I). We separate stars from non-stellar objects based on the object shapes in the R and I bands, attempting to reproduce the SDSS star/galaxy dichotomy. The completeness test indicates that the catalogue is complete to the limiting magnitudes. Comment: 31 pages, 15 figures, Accepted for publication in Astrophysics & Space Science |
| Databáze: | OpenAIRE |
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