Table 2: Log of spectroscopic observations.

Object		 Run PA Position Single exp. time Total exp. time Template
    [$\circ$]   [s] [h]  

(1)		 (2) (3) (4) (5) (6) (7)

NGC 1638		 2 70 MJ 3600+3000 1.8 HR 1318
  2 160 MN $2\times2700$ 1.5 HR 1318
NGC 2855 1 120 MJ $2\times3600$ 2.0 HR 2035
  1 30 MN $3\times3600$ 3.0 HR 2035
NGC 3885 1 123 MJ $4\times3600$ 4.0 HR 2429
  1 33 MN $3\times3600$ 3.0 HR 2429
NGC 4224 1 57 MJ $2\times3600$ 2.0 HR 2429
  1 147 MN $2\times3600$ 2.0 HR 2429
NGC 4235 1 48 MN $2\times3600$ 2.0 HR 2035
  1 138 MN $2\times3600$ 2.0 HR 2035
NGC 4586 1 115 MJ $4\times3600$ 4.0 HR 2701
  1 25 MN $3\times3600$ 3.0 HR 2701
NGC 4984 1 90 MJ $3\times3600+3000$ 3.8 HR 2035
  1 0 MN $3\times3600$ 3.0 HR 2035
NGC 7049 2 57 MJ 3600 1.0 HR 2113
  2 147 MN 3600 1.0 HR 2113
NGC 7213 2 124 MJ $2\times 3600 + 2700$ 2.8 HR 2113
  2 34 MN $2\times3600$ 2.0 HR 2113
NGC 7377 2 101 MJ $2\times3600$ 2.0 HR 2113
  2 21 MN $2\times3600$ 2.0 HR 2113
Notes. - Column 2: observing run. Column 3: slit position angle measured North through East. Column 4: slit position. MJ = major axis; MN = minor axis. Column 5: number and exposure time of the single exposures. Column 6: total exposure time. Column 7: giant star used as kinematical template in measuring the stellar kinematics (see Sect. 2.2).


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