BVI photometry of NGC 2547 (Naylor+, 2002)

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Clusters: Open, Photometry: Ubvri

Scientific paper

The catalogues have been created using the optimal photometry algorithm described in Naylor (1998MNRAS.296..339N) and Naylor et al. (2002MNRAS.335..291N, this paper). Further information is also available from Tim Naylor's optimal photometry page ( http://www.astro.ex.ac.uk/people/timn/Photometry/description.html ). The catalogues are primarily in what is called cluster format, though there are occasional variations where they are needed. There is a deep survey (Table 3), a shallower, but wider area survey (Table 4), and the combination of these (Table 5). Extracted from the deep catalogue are tables of members of the cluster derived using either the D'Antona & Mazzitelli (1997MmSAI..68..807D) isochrones (Table 6). or the Siess (2000A&A...358..593S) isochrones (Table 7). These catalogues are the result of a collaboration between teams within the Exeter Astrophysics Group led by Tim Naylor, and the Keele Astrophysics Group led by Rob Jeffries. The contributors to the currently available catalogues are Tina Devey, Monica Pozzo (now at Imperial), Simon Thompson and Ed Totten. (6 data files).

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