VIc photometry of M50 (NGC 2323) low-mass stars (Irwin+, 2009)

Details VIc photometry of M50 (NGC 2323) low-mass stars (Irwin+, 2009) VIc photometry of M50 (NGC 2323) low-mass stars (Irwin+, 2009)

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009ycat..73921456i&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/392/1456. Originally published in: 2009MNRAS.392.1456I

Physics

Clusters: Open, Stars: Pre-Main Sequence, Photometry: Ccd

Scientific paper

Photometric monitoring observations were obtained as part of the Monitor project, using the 4-m Blanco telescope at Cerro Tololo Inter-American Observatory (CTIO), with the Mosaic-II imager. A total of ~95h of photometric monitoring was conducted, spread over three distinct observing runs: 6xfull-nights in two three-night segments spanning 2005 February 04-06 and 2005 February 14-16, 8x1/2 nights between 2005 December 24 and 2006 January 06 and 4xfull-nights between 2006 January 28 and 2006 February 01. M50 was observed in a single telescope pointing centred on the cluster, for ~8h per night (~4h per 1/2 night).
(1 data file).

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