All Tables

Table 1: XMM-Newton count rates for SN 2002ap on 2002 February 2, in units of 10^-4 cts s^-1. The rates have been corrected for the telescope vignetting and the finite size of the extraction region. The values listed here are the averages of the results obtained with the three measurements described in Sect. 2.2.
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.
Table 3: XSPEC best-fit parameters for the X-ray spectrum of XMMU J013636.5+155036 in 2002 February, from the combined XMM-Newton EPIC dataset. The foreground line-of-sight absorption column density $n_{\rm {H,~Gal}}$ has been fixed at $0.5 \times 10^{21}$ cm ^-2. See http://heasarc.gsfc.nasa.gov/docs/xanadu/xspec for a full description of the XSPEC spectral models.
Table 4: XSPEC best-fit parameters for CXOU J13651.1+154547 in 2003 January, from the combined XMM-Newton EPIC dataset. $n_{\rm {H,~Gal}} \equiv 0.5 \times 10^{21}$ cm^-2 as in Table 3.
Table A.1: Source ID and average count rates (total and in three narrow bands) of the discrete X-ray sources detected by Chandra ACIS-S in the combined 2001 June-October observation. The count rates are in units of 10^-4 cts s^-1. Errors are $1\sigma$ , with $3\sigma$ upper limits for sources not detected in a certain band.