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Table 2.

Observing log of HST/STIS data.

ID Other name Filename Proposal PA Extr. window Obs. date Exp. time Im. filter
(_sx2 /_x2d) ID (°) pix (pc) (yy-mm-dd) (s)
(1) (2) (3) (4) (5) (6) (7) (8) (9)
NGC 2685 ( * ) IRAS 08517+5855 o63n01020 8607 54 3 (21) 2001-05-06 3097 F814W
NGC 3245 IRAS 10245+2845 o57205030 7403 203 5 (23) 1999-02-02 2715 F547M
NGC 4374 M 84 o3wn01010/2010 7124 104 5 (17) 1997-04-14 1993/2223 F814W
NGC 4486 M 87 o67z01010/2010 8666 164 5 (21) 2001-03-25/27 1360 F606W
NGC 4552 M 89 o5l203020 8472 78 5 (4) 2000-06-19 1440 F555W
NGC 4594 M 104 o4d303030 7354 250 5 (15) 1999-02-05 280 F814W
NGC 4676B ( * ) IC 820 o67q09030 8669 195 3 (144) 2002-02-20 740 F814W
NGC 4698 IRAS 12458+0845 o4e022010/20/30 7361 259 5 (16) 1997-11-24 900/933/840 F606W
NGC 4736 M 94 o67110030 8591 50 5 (6) 2002-07-15 1440 F555W

Notes. Columns indicate: (1) galaxy name; (2) other name; (3) file name of the analyzed spectra as indicated in the archive; (4) proposal ID of the observations; (5) position angle of the slit (north-eastward); (6) extraction window and its corresponding scale in parsecs; (7) date of the observation; (8) exposure time of the spectra; (9) filter used for the sharp-divided image (Márquez & Moles 1996) obtained also from the HST archive. The latter are shown in Appendix B.

( * )Spectrum obtained with a slit width whose plate scale was 0.102″ pixel−1. It is 0.051″ pixel−1 for the rest of the objects.

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