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Table 2

Photometric and morphometric selection criteria adopted.

Quantity Band NGC 3115 NGC 1399
ΔX6−12 g/i ± 0.15 ± 0.15
CLASS_STAR g ≥0.4 ≥0.4
CLASS_STAR i ≥0.7 ≥0.2
PSF FWHM g ≥3.5, ≤7.5 ≥4.5, ≤8.5
PSF FWHM i ≥3.5, ≤7.5 ≥4.5, ≤8.5
Flux radius g ≤4.5 ≤4.5
Flux radius i ≤4.0 ≤4.5
Kron radius g/i ≤5 ≤5
Petro. radius i ≥3.5, ≤7.5 ≥3.5, ≤7.5
Elongation a/b g/i ≤1.5 ≤1.5
(ui) ≥1.25, ≤3.75 ≥1.25, ≤3.75
(gi) ≥0.4, ≤1.4 ≥0.4, ≤1.4
Δ(ui) ≤0.3 ≤0.3
Δ(gi) ≤0.2 ≤0.2
Δ mag g/i ≤0.2 ≤0.2
mbright g 19.5 20.2
mbright i 18.5 19.2
Color–color ∣(gi)  − [0.380(ui)  − 0.005]∣ ≤ 0.2 ∣(gi)  − [0.362(ui)  − 0.0205]∣ ≤ 0.2

Notes. Explanation of listed parameters. ΔX6−12: interval adopted for the magnitude concentration index in g- and i-band. SExtractor output parameters: CLASS_STAR: Neural-Network-based star/galaxy classifier; PSF FWHM: point spread function full width at half maximum; Flux Radius: half light radius; Kron Radius: defined from the automatic aperture photometry, intended to give a precise estimate of total magnitude, inspired to Kron (1980) first moments algorithm; Petro. Radius: the radius at which the surface brightness of the isophote is η times the average surface brightness within the isophote; Elongation: semi-major over semi-minor axis ratio (see Bertin & Arnouts 1996, and references therein for more details). Other selection parameters. (ui) and (gi): colour intervals adopted from the comparison with empirical data and stellar population models; Δ(gi) and Δ(ui): maximum allowed error on colors; Δ mag: maximum error on magnitude; mbright : bright cut magnitude, at ~3 × σ brighter than the turn-over magnitude of the GCLF; color–color: equation of color–color region used for selecting GC candidates.

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