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Table 2

Best-fit temperature, relative abundance of heavy elements, X-ray luminosity, and signal-to-noise ratio using a redshift of 0.0501.

Region kT Z L0.5−2 S/N
keV Z 1043 erg s-1

Full Comet

Head* 10
Main tail* 11
Full comet* 14

Outside* 0.05 fixed 5

Notes. The


marks fits, where the cluster emission in (4–7) was simultaneously fitted and accounted for (the S/N could only in these cases be calculated properly, since the cluster emission is accounted for in the noise).

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