Pre-main-sequence isochrones – I. The Pleiades benchmark
Version of Record online: 25 JUL 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 424, Issue 4, pages 3178–3191, 21 August 2012
How to Cite
Bell, C. P. M., Naylor, T., Mayne, N. J., Jeffries, R. D. and Littlefair, S. P. (2012), Pre-main-sequence isochrones – I. The Pleiades benchmark. Monthly Notices of the Royal Astronomical Society, 424: 3178–3191. doi: 10.1111/j.1365-2966.2012.21496.x
- Issue online: 8 AUG 2012
- Version of Record online: 25 JUL 2012
- Manuscript Accepted: 11 JUN 2012
- Manuscript Received: 8 JUN 2012
- UK Science and Technology Facilities Council (STFC) studentship
- RCUK fellowship
- National Aeronautics and Space Administration (NASA)
- National Science Foundation
Disclaimer: Supplementary materials have been peer-reviewed but not copyedited.
Table 2. The full Pleiades photometric catalogue with colours and magnitudes in the natural INT-WFC photometric system.
Table 3. The calculated transformations between the SDSS and INT-WFC photometric systems for unreddened MS stars where Δ represents (INT-WFC − SDSS).
Table 4. The transformed Stripe 82 standard star catalogue with colours and magnitudes in the natural INT-WFC photometric system.
Table 5. The catalogue of colours and magnitudes in the natural INT-WFC photometric system for Pleiades members.
Table 6. The Pleiades single-star sequence in the INT-WFC and 2MASS bandpasses.
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