Physics
Scientific paper
Jun 2009
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73861625c&link_type=abstract
VizieR On-line Data Catalog: J/MNRAS/386/1625. Originally published in: 2008MNRAS.386.1625C
Physics
Clusters: Open, Photometry: Ubvri, Radial Velocities, Proper Motions
Scientific paper
U, B, V and I images centred on NGC 2112 were obtained at the Cerro Tololo Inter-American Observatory 1.0-m telescope, which is operated by the SMARTS1 consortium. The telescope is equipped with a new 4000x4000 CCD camera having a pixel scale of 0.289arcsec/pixel, which allows one to cover a field of 20x20arcmin2. This allows us to cover the entire cluster, which has an estimated diameter of 18 arcmin (Dias et al., 2002, Cat.
Medium-resolution spectroscopic observations were carried out on the night of 2006 February 15 (Julian Date 2453783.57006) with the Hydra spectrograph onboard the Wisconsin Indiana Yale NOAO (WIYN) telescope at Kitt Peak National Observatory
Echelle spectrograms of stars 535, 261, 717, 304 and 836 were obtained on 2007 October 29 with the Magellan Inamori Kyocera Echelle (MIKE) spectrograph mounted on the Nasmyth focus of Landon Clay 6.5-m telescope at the Magellan Observatory. Data were obtained with both the blue and red arms.
(1 data file).
Bidin Christian Moni
Carraro Giovanni
Demarque Pierre
McSwain Virgina M.
Villanova Sandro
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