Table 1: The log of all the observations analysed in this paper.
Name z 1 $\hbox{$^{\prime\prime}$ }$a Chandra HST ${F}_{\rm0.5{-}2~keV}$ f ${F}_{\rm [{O~\tiny\textsc{iii}}]}$ g [O III]/
    (pc) Date Instr.b Exp.c Prog. ID I/Fd Exp.e (10-13 cgs) (10-13 cgs) soft X
NGC 1386 0.0029 60 2003-11-19 A-S 20 6419 W2/F5 800 1.8 5.1 2.8
Mrk 3 0.0135 275 2000-03-18 A-S/H 100 5140 F/F5 750 4.7 20.5 4.4
NGC 3393 0.0125 255 2004-02-28 A-S 29 3981 W/F5 8000 2.2 10.5 4.8
NGC 4388 0.0084 170 2001-06-08 A-S 20 6332 W2/FR 280 3.4 13.4 3.9
NGC 4507 0.0118 240 2001-03-15 A-S/H 140 8259 W2/FR 520 3.3 11.0 3.3
NGC 5347 0.0078 160 2004-06-05 A-S 37 8598 W2/FR 800 0.27 0.8 3.0
NGC 5643 0.0040 80 2004-12-26 A-S 8 5411 W2/F5 700 1.4 5.1 3.6
NGC 7212 0.0266 530 2003-07-22 A-S 20 6332 W2/FR 600 0.8 8.8 11.0
a Radial extent of 1 arcsec at the distance of the source, assuming the cosmology reported in the text.
b Chandra instrument (A-S: ACIS-S; A-S/H: ACIS-S/HETG).
c Chandra exposure time in ks.
d HST instrument/filter configuration (W: WFPC; W2: WFPC2; F: FOC; F5: F502N; FR: FR533N).
e HST exposure time in s.
f All values taken from this paper, except for NGC 4388 (Iwasawa et al. 2003).
g All values taken from Schmitt et al. (2003a), except for NGC 5643 (this paper).

Source LaTeX | All tables | In the text