Fitting isochrones to open cluster photometric data - II. Nonparametric open cluster membership likelihood estimation and its application in optical and 2MASS near-IR data

W. S. Dias; H. Monteiro; T. C. Caetano; A. F. Oliveira

doi:10.1051/0004-6361/201118206

Free Access

Issue		A&A Volume 539, March 2012


Article Number		A125
Number of page(s)		21
Section		Galactic structure, stellar clusters and populations
DOI		https://doi.org/10.1051/0004-6361/201118206
Published online		06 March 2012

Online material

	Fig. 3 Graphs for the filtering of open cluster NGC 2477. Upper graphs give all UBV data and lower ones the filtered and weighted data and the fitted isochrone and ZAMS (solid lines). The symbol size is proportional to likelihood value.
Open with DEXTER

	Fig. 4 Graphs for the filtering of open cluster NGC 2477. Upper graphs give all 2MASS data and lower ones the filtered and weighted data and the fitted isochrone and ZAMS (solid lines). The symbol size is proportional to likelihood value.
Open with DEXTER

	Fig. 5 Same as Fig. 1 for NGC 7044.
Open with DEXTER

	Fig. 6 Same as Fig. 2 for NGC 7044.
Open with DEXTER

	Fig. 7 Same as Fig. 1 for NGC 2266.
Open with DEXTER

	Fig. 8 Same as Fig. 2 for NGC 2266.
Open with DEXTER

	Fig. 9 Same as Fig. 1 for Berkeley 32.
Open with DEXTER

	Fig. 10 Same as Fig. 2 for Berkeley 32.
Open with DEXTER

	Fig. 11 Same as Fig. 1 for NGC 2682 (Ref. 31).
Open with DEXTER

	Fig. 12 Same as Fig. 1 for NGC 2682 (Ref. 54).
Open with DEXTER

	Fig. 13 Same as Fig. 1 for NGC 2682 (Ref. 335).
Open with DEXTER

	Fig. 14 Same as Fig. 2 for NGC 2682.
Open with DEXTER

	Fig. 15 Same as Fig. 1 for NGC 2506 (Ref. 284).
Open with DEXTER

	Fig. 16 Same as Fig. 1 for NGC 2506 (Ref. 163).
Open with DEXTER

	Fig. 17 Same as Fig. 2 for NGC 2506.
Open with DEXTER

	Fig. 18 Same as Fig. 1 for NGC 2355 (Ref. 44).
Open with DEXTER

	Fig. 19 Same as Fig. 1 for NGC 2355 (Ref. 217).
Open with DEXTER

	Fig. 20 Same as Fig. 2 for NGC 2355.
Open with DEXTER

	Fig. 21 Same as Fig. 1 for Melotte 105 (Ref. 289).
Open with DEXTER

	Fig. 22 Same as Fig. 1 for Melotte 105 (Ref. 32).
Open with DEXTER

	Fig. 23 Same as Fig. 2 for Melotte 105.
Open with DEXTER

	Fig. 24 Same as Fig. 1 for Trumpler 1 (Ref. 86).
Open with DEXTER

	Fig. 25 Same as Fig. 1 for Trumpler 1 (Ref. 320).
Open with DEXTER

	Fig. 26 Same as Fig. 2 for Trumpler 1.
Open with DEXTER

	Fig. 27 Same as Fig. 1 for Dias 6 observed by our group.
Open with DEXTER

	Fig. 28 Same as Fig. 2 for Dias 6.
Open with DEXTER

	Fig. 29 Comparison of our fit with that of Bica et al. (2004) for Dias 6. See the text for details.
Open with DEXTER

	Fig. 30 Comparison of our fit with that of Tadross (2008) for Dias 6. See the text for details.
Open with DEXTER

© ESO, 2012

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.