Mathematics – Logic
Scientific paper
Oct 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005xmm..prop..184p&link_type=abstract
XMM-Newton Proposal ID #04049646
Mathematics
Logic
Groups Of Galaxies, Clusters Of Galaxies, Supercluster, Xmm-Lss_4, Xmm-Lss_13, Xmm-Lss_17, Xmm-Lss_32, Xmds Om_4, Xmm-Lss_33, Xmm-Lss_34, Xmm-Lss_35, Xmm-Lss_36, Xmm-Lss_37, Xmm-Lss_38, Xmm-Lss_39, Xmm-Lss_40, Xmm-Lss_41, Xmm-Lss_42, Xmm-Lss_43, Xmm-Lss_44, Xmm-Lss_45, Xmm-Lss_46, Xmm-Lss_47, Xmm-Lss_48, Xmm-Lss_49, Xmm-Lss_50, Xmm-Lss_51, Xmm-Lss_52, Xmm-Lss_53, Xmm-Lss_54, Xmm-Lss_55, Xmm-Lss_56, Xmm-Lss_57, Xmm-Lss_58, Xmm-Lss_59, Xmm-Lss_60, Xmm-Lss_61, Xmm-Lss_62, Xmm-Lss_63, Xmm-Lss_64, Xmm-Lss_65, Xm
Scientific paper
We propose to complete, by an additional 5 deg2, the XMM-LSS Survey region overlying the Spitzer/SWIRE field. This field already has CFHTLS and Integral coverage, and will encompass about 10 deg2. The resulting multi-wavelength medium-depth survey, which complements XMM and Chandra deep surveys, will provide a unique view of large-scale structure over a wide range of redshift, and will show active galaxies in the full range of environments. The complete coverage by optical and IR surveys provides high-quality photometric redshifts, so that cosmological results can quickly be extracted. In the spirit of a Legacy survey, we will make the raw X-ray data immediately public. Multi-band catalogues and images will also be made available on short time scales.
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