Theoretical isochrones compared to 2MASS observations: Open clusters at nearly solar metallicity

By C. Bonatto, E. Bica, L. Girardi. 2004

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In Astronomy and Astrophysics

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THE DISTANCE, MASS, AND RADIUS OF THE NEUTRON STAR IN 4U 1608−52 (2008, background): “The absolute magnitude (MK) and intrinsic color, (J − Ks)0, of the red clump giants are well established (Alves 2000; Grocholski & Sarajedini 2002; Salaris & Girardi 2002; Pietrzyński et al. 2003).”
Atmospheric circulations of terrestrial planets orbiting low-mass stars (2011, background): “(2008) with Bonatto et al. (2004) for 2MASS-specific details, and the photometric system is 2MASSJHKs with circumstellar dust turned off.”
The ACS Survey of Galactic Globular Clusters. II. Stellar Evolution Tracks, Isochrones, Luminosity Functions, and Synthetic Horizontal-Branch Models (2007, background): “…this paper, chief among these are Berbusch & Vandenberg (2001); Vandenberg et al. (2006, hereafter Victoria-Regina), Girardi et al. (2002); Bonatto et al. (2004); Girardi et al. (2004, hereafter Padova), Pietrinferni et al. (2004, 2006, hereafter BaSTI) and Cordier et al. (2007), and Yi…”
THE APOGEE RED-CLUMP CATALOG: PRECISE DISTANCES, VELOCITIES, AND HIGH-RESOLUTION ELEMENTAL ABUNDANCES OVER A LARGE AREA OF THE MILKY WAY'S DISK (2014, methodology): “We have also computed the density near the RC using the Padova (Girardi et al. 2000; Bonatto et al. 2004) and BaSTI (Pietrinferni et al. 2004) isochrone libraries using the same IMF and SFH assumptions.”
The Initial Mass Function of the Massive Star-forming Region NGC 3603 from Near-Infrared Adaptive Optics Observations (2007, methodology): “For the 8 − 19 M⊙ high-mass bin, in addition to the 2.5 Myr MS isochrone in the Geneva model (LS01), we apply an isochrone of the Padova evolutionary model computed with the 2MASS filter system (Bertelli et al. 1994; Girardi et al. 2000; Bonatto et al. 2004).”
A PHOTOMETRIC VARIABILITY SURVEY OF FIELD K AND M DWARF STARS WITH HATNet (2009, methodology): “The relation for giant stars with log g < 2.0 is taken from the 1.0 Gyr, solar metallicity Padova isochrone (Marigo et al. 2008; Bonatto et al. 2004).5 While the majority of stars lie in the expected dwarf range, a significant number of stars fall along the giant branch.”
Decay of Planetary Debris Disks (2005, unknown): “…1985; (17) Song et al. 2001; (18) Perryman et al. 1998; (19) Gerbaldi et al. 1999; (20) Paunzen 1997; (21) Barrado y Navascués et al. 1999; (22) Bonatto et al. 2004; (23) U Sco, de Zeeuw et al. 1999; (24) IC 2602, Randich et al. 2001; (25) King et al. 2003; (26) Iliev & Barzova 1995; (27)…”