Transforming observational data and theoretical isochrones into the ACS/WFC Vega-mag system
Open Access
- 1 March 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 357 (3) , 1038-1048
- https://doi.org/10.1111/j.1365-2966.2005.08735.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 31 references indexed in Scilit:
- How Accurately Can We Calculate the Depth of the Solar Convective Zone?The Astrophysical Journal, 2004
- A compilation of charged-particle induced thermonuclear reaction ratesPublished by Elsevier ,2003
- Evidence of a Significant Intermediate-Age Population in the M31 Halo from Main-Sequence PhotometryThe Astrophysical Journal, 2003
- Color-Magnitude Diagram and Luminosity Function of M4 near the Hydrogen-burning LimitThe Astrophysical Journal, 2001
- Toward High‐Precision Astrometry with WFPC2. I. Deriving an Accurate Point‐Spread FunctionPublications of the Astronomical Society of the Pacific, 2000
- Distances, Ages, and Epoch of Formation of Globular ClustersThe Astrophysical Journal, 2000
- A critical investigation on the discrepancy between the observational and the theoretical red giant luminosity function 'bump'Monthly Notices of the Royal Astronomical Society, 1997
- Abundances for globular cluster giants. I. Homogeneous metallicities for 24 clustersAstronomy and Astrophysics Supplement Series, 1997
- Low-temperature Rosseland opacitiesThe Astrophysical Journal, 1994
- UBVRI passbandsPublications of the Astronomical Society of the Pacific, 1990