All Tables

Table 1: Log of Suzaku observations of RX J1347.5-1145.
Table 2: Single-temperature APEC model parameters fit to the XIS spectra taken by four sensors (XIS-0, XIS-1, XIS-2, XIS-3), and the result from the simultaneous fit to all of the sensors (XIS-0, 1, 2, 3).
Table 3: The instrumental calibration parameters from the APEC model fit simultaneously to the XIS-0, 1, 2, and 3.
Table 4: Two-temperature APEC model parameters fit to the XIS spectra in the 0.5-10 keV and 4.0-5.5 keV bands.
Table 5: PIN count rates measured in the 12-40 keV and 40-60 keV bands. The quoted errors are 1 $\sigma$ statistical errors.
Table 6: Single-temperature APEC model parameters fit to the PIN data in the 12-60 keV band. The systematic error in the NXB model is included in the error estimate.
Table 7: Parameters of the ``6APEC model'', including estimates of the deprojected temperature profile from the Chandra ACIS-I data at the six annular bins in the NW region, which excludes the SE quadrant.
Table 8: Spectral parameters for the SE excess component obtained from the 6APEC $\times$ PLABS + APEC model fit to the XIS+PIN data and the XIS data.
Table 9: Spectral parameters for the SE excess component obtained from the 6APEC $\times$ PLABS+non-thermal power-law (PL) model fit to the XIS+PIN data.
Table 10: Limits on the amplitude (normalization) of a non-thermal power-law (PL) component with $\Gamma =1.5$ as the explanation of the excess hard X-ray emission in the SE quadrant.