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Table 3

Star pile velocity dispersion measurements from FORS2 and GMOS longslits.

Instrument/Grism Radial range [kpc] PA [degrees] S/N Δ3 [km s-1] σ[km s-1]

FORS2/1200R 5–12 33.2 13 −111 ± 40 299  ±  55
Major axis 12–31 33.2 15 −141 ± 37 255  ±  47
6–12 213.2 18 −312 ± 40 308  ±  35
12–29 213.2 14 −308 ± 42 265  ±  32

FORS2/1200R 5.5–15 43.0 13 −27 ± 23 188  ±  31
Interm. axis 2–7 223.0 16 −90 ± 39 129  ±  20

GMOS/600B 5.6–10.4 29.3 9 −91 ± 56 248  ±  26
Major axis 10.4–17.6 29.3 10 −135 ± 57 307  ±  34
17.6–26.4 29.3 8 −161 ± 57 330  ±  44
5.6–8.0 209.3 12 −212 ± 41 358  ±  45
8.0–15.2 209.3 15 −223 ± 31 276  ±  29
15.2–22.4 209.3 11 −243 ± 134 264  ±  36

GMOS/600B 5.6–9.6 151.6 11 −144 ± 55 120  ±  21
Interm. Axis 9.6–17.6 151.6 10 −133 ± 27 176  ±  15
4.0–8.8 331.6 14 −252 ± 88 298 ± 21
8.8–20.8 331.6 12 −343 ± 134 349 ± 25

Notes. Column 1 indicates the instrument/grism combination. Column 2 indicates the radial range in which the spatial binning has been done, with respect to the position of the nucleus the long slit crosses. Column 3 is the position angle of the slit, measured East from North (see Fig. 1 for the exact slit positioning). Column 4 indicates the signal-to-noise ratio of each spectra at the central wavelength of the range used for the pPXF fit. Column 5 is the velocity difference with the system velocity of the cluster. Column 6 indicates the velocity dispersion and its error.

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