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Cited article:

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The Chandra Deep Field–North Survey. XVII. Evolution of Magnetic Activity in Old Late‐Type Stars

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The Astrophysical Journal 611 (2) 1107 (2004)
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Dependence of coronal X-ray emission on spot-induced brightness variations in cool main sequence stars

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Time evolution of X-ray coronal activity in PMS stars; a possible relation with the evolution of accretion disks

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Evidence for coronal activity cycles on 61 Cygni A and B

A. Hempelmann, J. H. M. M. Schmitt, S. L. Baliunas and R. A. Donahue
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XMM-Newtonand the Pleiades - I. Bright coronal sources and the X-ray emission from intermediate-type stars

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