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We report the results of two Chandra observations of the recurrent nova CIAql at 14 and 16 months after its outburst in April 2000, respectively. TheX-ray emission is faint in both cases, without any noticeable change inspectrum or intensity. Although the emission is very soft, it is not luminousenough to be due to late-time H-burning. This implies that the luminoussupersoft phase ended even before the time predicted by the most recentcalculations. The details of the X-ray spectrum, together with the fact thatthe observed X-ray intensity is brighter than pre-outburst (1992/1993), suggestthat the observed X-ray emission is either due to ionization of thecircumstellar material or due to the shocks within the wind and/or with thesurrounding medium.Comment: 10 pages ApJ style with 5 figures; accepted for publication in Ap

[ITAL]Chandra[/ITAL] Observations of the Recurrent Nova CI Aquilae after Its 2000 April Outburst