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Table 3

Summary of the observations.

(1)  (2)  (3)  (4)  (5)  (6)  (7)  (8)  (9)  (10)  (11)  (12)  (13)

Galaxy date total effective seeing (″) photometric aperture A K A g A z R blend N blend N
exposure time (s) airmass correction correction (ACSpix)

NGC 3377 18, 21 and 22/03/2008 12 000 1.334  ~1.2  −0.060 ± 0.007 0.286 ± 0.012 0.013 0.123 0.050 30 10 75
NGC 4278 22 and 24/03/2008 12 000 1.586  ~1.2 0.524 ± 0.023 0.010 0.105 0.043 30 6 67
NGC 4365 27 and 28/02/2007 2700 1.203  ~0.9 0.083 ± 0.005 0.008 0.076 0.0312 25 12 99
NGC 4374 18 and 19/03/2008 12 000 1.223  ~1.5 0.348 ± 0.015 0.015 0.145 0.059 35 11 93
NGC 4382 13 and 15/03/2009 12 900 1.080  ~1.0  −0.18 ± 0.03 0.341 ± 0.018 0.011 0.113 0.046 25 5 59
NGC 4406 28/02/2007 11 700 1.206  ~0.9 0.148 ± 0.006 0.011 0.109 0.044 25 8 76
NGC 4473 13, 14, and 15/03/2009 12 600 1.436  ~1.2  −0.23 ± 0.02 0.351 ± 0.016 0.010 0.102 0.041 30 2 55
NGC 4486 27 and 28/02/2007 12 000 1.195  ~1.1 0.190 ± 0.008 0.008 0.080 0.033 30 76 301
NGC 4526 18 and 19/03/2008 12 600 1.434  ~1.4  −0.050 ± 0.007 0.448 ± 0.187 0.008 0.080 0.033 35 6 55
NGC 4552 18 and 21/03/2008 12 600 1.253  ~1.3  −0.090 ± 0.006 0.233 ± 0.009 0.015 0.149 0.061 30 6 107
NGC 4570 15 and 16/03/2009 11 400 1.242  ~1.0  −0.20 ± 0.01 0.273 ± 0.013 0.080 0.080 0.033 25 1 19
NGC 4621 18 and 21/03/2008 12 000 1.249  ~1.3  −0.020 ± 0.001 0.270 ± 0.011 0.012 0.120 0.049 30 10 80
NGC 4649 27 and 28/02/2007 11 700 1.284  ~0.9 0.161 ± 0.007 0.010 0.094 0.039 25 21 164
NGC 4660 15 and 16/03/2009 12 300 1.258  ~1.2 0.466 ± 0.020 0.012 0.120 0.049 30 6 51

Notes. LIRIS K-band imaging and relevant calibration parameters for LIRIS and ACS: (1) galaxy; (2) dates the data were taken; (3) total exposure time in seconds; (4) effective airmass; (5) seeing; (6) value of photometric correction; (7) value of aperture correction; (8)–(10) galactic extinction in K(AK), g(Ag) and z(Az) respectively; (11) blending radius (Rblend); (12) number of blended sources; and (13) final number of clusters that satisfy the criteria summarised in Sect. 5.

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