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Paper IPM / Astronomy / 13761 |
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We analysed the XMM-Newton observations of the CFHTLS wide (W1) field as a part of the XMM-LSS survey (Pierre et al., 2007MNRAS.382..279P, Cat. J/MNRAS/382/279). The details of observations and data reduction are presented in Bielby et al. (2010A |
A...523A..66B). We concentrate on the low-z counterparts of the X-ray sources and use all XMM observations performed till 2009, covering an area of 2.276°x2.276°.
The CFHTLS wide observations have been carried out in the period between 2003 and 2008, covering an effective survey area of 154 square degrees. The optical images and data of the CFHTLS were obtained with the MegaPrime instrument mounted on the CFHT in the five filters u*, g', r', i' and z'.
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