Table 2: Observed and emitted fluxes of SN 2002ap on 2002 February 2, for three different spectral models consistent with the observed X-ray count rates in the EPIC pn and MOS bands (Table 1). A distance of 7.3 Mpc has been assumed. Fluxes are in units of 10-15 erg cm-2 s-1.

Instrument		 Flux Flux Flux Flux
  (0.3-12.0) keV (0.3-1) keV (1-2) keV (2-12) keV
  model: $n_{\rm H} = 5 \times 10^{21}$ cm-2; $kT_{\rm {rs}} = 0.50$ keV; $Z=Z_{\odot}$

pn observed flux		 $4.9\pm0.6$ $2.8\pm0.4$ $1.9\pm0.4$ $0.2\pm1.2$
MOS1 observed flux $4.0\pm1.0$      
MOS2 observed flux $4.1\pm1.0$      
pn emitted flux $25.7\pm3.1$ $21.5\pm2.9$ $3.9\pm0.8$ $0.2\pm1.2$
MOS1 emitted flux $21.1\pm5.1$      
MOS2 emitted flux $21.4\pm5.2$      
  model: $n_{\rm H} = 3 \times 10^{21}$ cm-2; $kT_{\rm {rs}} = 0.75$ keV; $Z=Z_{\odot}$

pn observed flux		 $5.2\pm0.6$ $2.9\pm0.4$ $2.0\pm0.4$ $0.2\pm1.2$
MOS1 observed flux $4.1\pm1.1$      
MOS2 observed flux $4.2\pm1.1$      
pn emitted flux $12.4\pm1.5$ $9.2\pm1.2$ $3.1\pm0.7$ $0.2\pm1.2$
MOS1 emitted flux $9.9\pm2.4$      
MOS2 emitted flux $10.0\pm2.4$      
  model: $n_{\rm H} = 0.5 \times 10^{21}$ cm-2; $kT_{\rm {rs}} = 0.85$ keV; $Z=Z_{\odot}$

pn observed flux		 $5.0\pm0.6$ $2.8\pm0.4$ $2.0\pm0.4$ $0.2\pm1.2$
MOS1 observed flux $4.1\pm1.1$      
MOS2 observed flux $4.2\pm1.1$      
pn emitted flux $5.9\pm0.7$ $3.6\pm0.5$ $2.0\pm0.4$ $0.2\pm1.2$
MOS1 emitted flux $4.9\pm1.3$      
MOS2 emitted flux $5.0\pm1.3$      


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