- Table 1:
Best-fits to the 0.5-10 keV XMM-Newton PN persistent
emission spectra of X1254-690 using a disk-blackbody model with an inner
and normalization k given by
in the inner radius in km and d the
distance in units of 10 kpc and a power-law with a photon index,
together with an emission and two absorption lines.
- Table 2:
Properties of the Fe XXVI K
feature in three segments of the persistent emission during the 2001
observation. The time reference used for phase 0 is 19.25 h of 2001 January 22 and the period is 3.88 h.