XMMXCS J033049.7-522836.5
| XCS ID | scts | z | z-source | Tx | -σ(Tx) | +σ(Tx) | Alternative Name |
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| XMMXCS J033049.7-522836.5 | 14935 | 0.44 | Lit | 4.5 | 0.1 | 0.1 | ABELL 3128 NE |
Note: This cluster was also detected serendipitously by Werner et al. 2007. On the basis of deep (100 ks) XMM-Newton data, they detected two X-ray peaks separated by ~12 arcmins for the cluster A3128 (at z=0.06). By detecting the redshifted Fe K line they confirmed the Northeast peak toward A3128 NE to be a distant luminous cluster of galaxies at redshift z=0.44.
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Fig. 1: XCS produced XMM image (produced from the ObsID 0400130201, see Fig. 3) of the cluster XMMXCS J033049.7-522836.5. Brighter regions show areas of increased X-ray flux. Position mouse over XAPA sources: [on] to reveal the shape of XAPA detected extended (point) sources highlighted in green (red). Image size is 3 x 3 arcmins.
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Fig. 2: DSS image of the XCS cluster XMMXCS J033049.7-522836.5. Position mouse over X-ray contours: [on] to reveal both the XCS X-ray contours overlaid in blue. Image size is 3 x 3 arcmins.
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Fig. 3: The XCS produced image of XMM ObsID 0400130201. Brighter regions show areas of increased X-ray flux. Position mouse over [XAPA Sources] to reveal X-ray sources detected by the XCS Automated Pipeline Algorithm (XAPA). The shape of XAPA detected extended (point) sources are highlighted in green (red). If applicable, the shape of XAPA sources deemed close to the PSF of the instrument are highlighted in pink, and those dominated by an internal point-source/sources are highlighted in blue. The source belonging to the cluster XMMXCS J033049.7-522836.5 is highlighted in bold. Occasionally, areas of an XCS ObsID are masked to remove regions deemed unsuitable for cluster detection. Position mouse over [Unmasked Image] to display any masked regions of this XCS ObsID.
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