XMMXCS J021832.4-050054.1
| XCS ID | scts | z | z-source | Tx | -σ(Tx) | +σ(Tx) | Alternative Name |
| XMMXCS J021832.4-050054.1 | 335 | 0.88 | Lit | 3.5 | 0.6 | 0.8 | XLSSU J021832.0-050105 |
Note: Since compiling XCS-DR1, we have identified three clusters where XAPA failed to find obvious (to the eye) embedded point sources. In none of these cases does the point source dominate the cluster emission, but we are working to adjust the performance of XAPA in these cases.
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Fig. 1: XCS produced XMM image (produced from the ObsID 0112370101, see Fig. 3) of the cluster XMMXCS J021832.4-050054.1. 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 J021832.4-050054.1. 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 0112370101. 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 J021832.4-050054.1 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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