All Tables

• Table 1: Summary of the XMM-Newton observation of UU Col.
• Table 2: Spectral parameters as derived from simultaneously fitting the EPIC PN and MOS phase-averaged spectra for the two best fit models discussed in the text. Quoted errors refer to the 90confidence level for the parameter of interest.
• Table 3: Spectral parameters as derived from fitting the EPIC PN spectrum at maximum and minimum of spin pulsation using Model A in Table 2.