XMMXCS J015558.0+053200.8
| XCS ID | scts | z | z-source | Tx | -σ(Tx) | +σ(Tx) | Alternative Name |
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| XMMXCS J015558.0+053200.8 | 127 | | NXS | | | | |
Note: This NXS Field was not only non-photometric, but the guide-star tracking was lost mid-exposure. However, the data were deemed to be of sufficient quality to be included in the optical confirmation work presented in
Mehrtens et al. (2012).
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Fig. 1: XCS produced XMM image (produced from the ObsID 0153030701, see Fig. 3) of the cluster XMMXCS J015558.0+053200.8. 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: NXS colour composite image of the XCS cluster XMMXCS J015558.0+053200.8 using r-band and z-band data from the NXS FieldID 0153030701. Position mouse over X-ray contours: [on] to reveal 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 0153030701. 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 J015558.0+053200.8 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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