Table A.6: Same as Table A.3 for RSCVn systems in our sample.
    O VII Ne IX
Star Instr. log $V_{\rm cor}^a$ log $V_{\rm av}^b$ fc log $V_{\rm cor}^a$ log $V_{\rm av}^b$ fc
    [cm3] [cm3] % [cm3] [cm3] %
ARLac RGS1 31.3 33.0 1.78 - - -
  MEG - - - 30.3 33.2 0.13
  HEG - - - 29.1 32.5 0.04
Capella LETG 32.8 35.0 0.64 - - -
  MEG 32.3 34.9 0.26 29.3 32.9 0.02
  HEG - - - 29.2 32.8 0.02
HR1099 RGS1 31.3 34.1 0.19 - - -
  LETG 31.2 34.2 0.08 - - -
  MEG 32.0 32.7 18.8 31.4 33.8 0.40
  HEG - - - 30.4 33.2 0.17
IIPeg MEG 30.6 34.3 0.02 31.1 33.6 0.32
  HEG - - - 30.3 33.2 0.10
IMPeg MEG 29.0 33.5 0.00 30.2 33.8 0.02
  HEG - - - 29.6 33.4 0.01
$\lambda$And RGS1 30.7 33.9 0.06 - - -
  LETG 31.2 34.5 0.04 - - -
  MEG 30.4 34.4 0.01 29.9 33.0 0.08
  HEG - - - 28.9 32.5 0.02
$\sigma^2$CrB RGS1 31.7 34.1 0.37 - - -
  MEG 30.8 33.4 0.23 29.5 32.5 0.08
  HEG - - - 29.0 32.1 0.08
TYPyx MEG 30.3 33.5 0.07 29.8 32.9 0.08
  HEG - - - 28.7 32.5 0.01
UXAri RGS1 31.1 34.1 0.08 - - -
  LETG 32.2 34.8 0.25 - - -
  MEG 30.7 33.4 0.17 30.2 33.1 0.13
  HEG - - - 29.0 32.5 0.03
V824Ara MEG 30.2 33.7 0.03 29.5 32.6 0.08
  HEG - - - 29.9 32.7 0.15
VYAri RGS1 31.8 34.3 0.34 - - -
aEmitting coronal volumes from Eq. (4). bAvailable volumes from Eq. (7).
cFilling factor $f=V_{\rm cor}/V_{\rm avail}$.

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