Clusters and candidate clusters.
|Name||α||δ||g||r||V||FWHM r||FWHMr/⟨FWHMr,stars ⟩||notes|
|SexA-C1||10:10:51.7||−04:41:33.5||20.15||19.69||19.87||2.92″||3.9||cand. − extended?|
|SexB-C1||10:00:04.7||+05:20:07.5||18.16||17.87||17.98||1.04″||1.3||Sharina et al. (2007) cluster|
|SexB-C2||10:00:07.3||+05:18:00.8||18.37||17.32||17.75||1.19″||1.5||cand. – E0 galaxy?|
|SexB-C3||09:59:39.7||+05:16:36.0||19.65||19.55||19.59||2.77″||3.1||cand. – extended?|
Notes. Integrated magnitudes are computed within apertures of radius = 15 px (corresponding to 3.4″); typical uncertainties are ≃0.05 mag.
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