A. Nebot Gómez-Morán

SEGUE: A SPECTROSCOPIC SURVEY OF 240,000 STARS WITH<i>g</i>= 14-20

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The XMM-Newton serendipitous survey. VII. The third XMM-Newton serendipitous source catalogue

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Post-common-envelope binaries from SDSS. IX: Constraining the common-envelope efficiency

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