NGC 1399 and NGC 4486 globular clusters (Forte+, 2007)

Details NGC 1399 and NGC 4486 globular clusters (Forte+, 2007) NGC 1399 and NGC 4486 globular clusters (Forte+, 2007)

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008ycat..83821947f&link_type=abstract

VizieR On-line Data Catalog: J/MNRAS/382/1947. Originally published in: 2007MNRAS.382.1947F

Computer Science

Galaxies: Photometry, Clusters: Globular, Photometry: Cmt1T2V

Scientific paper

Photometric observations were carried out with the Mayall and Blanco 4-m telescopes at KPNO and CTIO, respectively, and 2048-pixels-on-a-side CCDs, with a pixel scale of 0.43". The C filter from the Washington System and the RKC filter of the Kron-Cousins system were used at both telescopes. As noted by Geisler (1996AJ....111..480G) this last filter is comparable to the T1 filter in the Washington system although much more efficient in terms of transmission. In what follows, we keep the T1 denomination for our red magnitudes.
(2 data files).

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