UBV(RI)c photometry of NGC 4852 (Ahumada+, 2011)

Details UBV(RI)c photometry of NGC 4852 (Ahumada+, 2011) UBV(RI)c photometry of NGC 4852 (Ahumada+, 2011)

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012ycat..74151355a&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/415/1355. Originally published in: 2011MNRAS.415.1355A

Physics

Clusters: Open, Photometry: Ubvri

Scientific paper

The field of NGC 4852 was observed at the Cerro Tololo Inter-American Observatory (CTIO, Chile) with the 1-m (ex YALO, now operated by the SMARTS Consortium) telescope and the Y4K Camera1 (Y4KCam) of the Ohio State University. The filters provided include a Johnson-Cousins BVRI set plus a U+ CuSO4 filter. The cluster was observed on two nights (2006 April 22-23 and 23-24).
(3 data files).

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