Table of Contents
ISRN Astronomy and Astrophysics
Volume 2014 (2014), Article ID 398182, 12 pages
Research Article

CCD SDSS Photometry of Poorly Studied Star Clusters in the Large Magellanic Cloud

1Observatorio Astronómico, Universidad Nacional de Córdoba, Laprida 854, 5000 Córdoba, Argentina
2Consejo Nacional de Investigaciones Científicas y Técnicas, Avenida Rivadavia 1917, C1033AAJ Buenos Aires, Argentina

Received 19 November 2013; Accepted 18 March 2014; Published 11 May 2014

Academic Editors: M. Marconi and L. Pulone

Copyright © 2014 Andrés E. Piatti. This is an open access article distributed under the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Supplementary Material

The resulting standardized photometric tables list successively a running number per star, the x and y coordinates, the averaged g magnitudes, the observational errors σ(g), the g-r colors, the observational errors σ(g-r), and the number of observations.

Only a portion of Table 2 is shown here for guidance regarding its form and content. The whole content of Tables 2–7 is provided as Supplementary Tables.

  1. Supplementary Material