2014
DOI: 10.1088/0004-6256/147/6/139
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OPEN CLUSTERS IN THEKEPLERFIELD. II. NGC 6866

Abstract: We have developed a maximum-likelihood procedure to fit theoretical isochrones to the observed cluster color-magnitude diagrams of NGC 6866, an open cluster in the Kepler Spacecraft field of view. The Markov-Chain Monte Carlo algorithm permits exploration of the entire parameter space of a set of isochrones to find both the best solution and the statistical uncertainties. For clusters in the age range of NGC 6866, with few if any red giant members, a purely photometric determination of the cluster properties i… Show more

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Cited by 49 publications
(63 citation statements)
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References 22 publications
(23 reference statements)
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“…Figure 14. Differences between the BV I C photometry of Janes et al (2013) and the present paper in the sense of (ours -theirs).…”
Section: Discussionmentioning
confidence: 49%
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“…Figure 14. Differences between the BV I C photometry of Janes et al (2013) and the present paper in the sense of (ours -theirs).…”
Section: Discussionmentioning
confidence: 49%
“…G99: Glushkova et al (1999). J13: Janes et al (2013). Hectoechelle, we find mean offsets of less than 0.1 km s −1 .…”
Section: Spectroscopy Of Kic 9777062mentioning
confidence: 62%
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“…Accordingly, it can be stated that the minimum age for subextensivity falls within the range of the probable ages of NCG2516, namely between 60 and 270 Myr. On the other hand, if we consider the age of 1 Gyr for NGC6811, as determined by Janes et al [34], instead of 575 Myr, the age for the extensivity of rotation period distributions changes to only 560 Myr. Figure 2 shows how the inverse of the median rotation period changes over cluster ages, as well as the nonextensive model proposed by de Freitas & De Medeiros [15].…”
mentioning
confidence: 98%