Gaia Data Release 1 - The Cepheid and RR Lyrae star pipeline and its application to the south ecliptic pole region

G. Clementini; V. Ripepi; S. Leccia; N. Mowlavi; I. Lecoeur-Taibi; M. Marconi; L. Szabados; L. Eyer; L. P. Guy; L. Rimoldini; G. Jevardat de Fombelle; B. Holl; G. Busso; J. Charnas; J. Cuypers; F. De Angeli; J. De Ridder; J. Debosscher; D. W. Evans; P. Klagyivik; I. Musella; K. Nienartowicz; D. Ordóñez; S. Regibo; M. Riello; L. M. Sarro; M. Süveges

doi:10.1051/0004-6361/201629583

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Volume 595 (November 2016)

A&A, 595 (2016) A133

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Gaia Data Release 1

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Fig. 9

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G-band R₂₁ vs. period diagram for DCEPs in the Magellanic Clouds (red: F, blue: 1O DCEPs in the LMC; magenta: F, cyan: 1O DCEPs in the SMC). The figure was obtained by transforming the I-band R₂₁ values in Soszynski et al. (2008a, 2010a, 2015b,c) to the G-band using eq. (16) (see text for details).

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