Distance to the Large Magellanic Cloud: The RR Lyrae Stars

By Gisella Clementini, R. Gratton, A. Bragaglia, E. Carretta, L. Di Fabrizio, M. Maio. 2003

192 citations recorded by the source corpus.

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In Astronomy and Astrophysics

Citations in the corpus

The Great disk of Milky Way satellites and cosmological sub-structures (2004, methodology): “The data are from Mateo (1998, Table 2), except that for the LMC D and eD are taken from Salaris et al. (2003) and Clementini et al. (2003), and likewise for the SMC from Dolphin et al. (2001).”
The Adequacy of Stellar Evolution Models for the Interpretation of the Color-Magnitude Diagrams of Resolved Stellar Populations (2005, methodology): “…Yoshii 1998; filled squares), trigonometric parallaxes (Gratton 1998; dotted line), MS fitting (Carretta et al. 2000; solid line), Baade Wesselink (Clementini et al. 2003; short-dashed-longdashed), RR Lyrae in ω Cen (Olech et al. 2003; dashed line), GCs in M31 (R.M. Rich, C.E. Corsi, C. Cacciari,…”
The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations (2018, background): “The references in the last column are as follows: (1) de Vaucouleurs et al. (1991); (2) Clementini et al. (2003); (3) van der Marel et al. (2002); (4) Udalski et al. (1999); (5) Harris & Zaritsky (2006); (6) Monaco et al. (2004); (7) Mateo, Olszewski & Morrison (1998); (8) Frinchaboy et al. (2012);…”
THE AGES OF 55 GLOBULAR CLUSTERS AS DETERMINED USING AN IMPROVED METHOD ALONG WITH COLOR–MAGNITUDE DIAGRAM CONSTRAINTS, AND THEIR IMPLICATIONS FOR BROADER ISSUES (2013, methodology): “Insofar as the slope of the variation of MV (RR) with [Fe/H] is concerned, we (and Benedict et al. 2011) are inclined to favor the value derived by Clementini et al. (2003) because it is based on so many variable stars.”
CLUSTERING OF LOCAL GROUP DISTANCES: PUBLICATION BIAS OR CORRELATED MEASUREMENTS? III. THE SMALL MAGELLANIC CLOUD (2014, methodology): “…& Kovács 1996) to derive metallicities (e.g., Deb & Singh 2010; Kapakos et al. 2010, 2011; Kapakos & Hatzidimitriou 2012), followed by absolutemagnitude calibration based on either theoretical models (e.g., Weldrake et al. 2004) or robust observational analysis (e.g., Clementini et al. 2003).”
Distances and ages of NGC 6397, NGC 6752 and 47 Tuc (2003, methodology): “A quite accurate and robust estimate for the slope has been recently obtained by Clementini et al. (2003), based on observations of a hundred RR Lyrae stars in the LMC.”