xmm-newton 1 m.stuhlinger/m.smith, esac pn monitoring mallorca, november 2007
Post on 19-Dec-2015
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XMM-Newton
1
M.Stuhlinger/M.Smith, ESAC
PN Monitoring
Mallorca, November 2007
XMM-Newton
2
M.Stuhlinger/M.Smith, ESAC
Hot Pixels
Mainly Column 64 Hot Pixels
M. Smith
XMM-Newton
3
M.Stuhlinger/M.Smith, ESAC
Noisy Pixels
Decrease in number of Noisy Pixels due tomodified blanking of Column 64 segments in latest BPT update (Rev 1408 onwards)
M. Smith
XMM-Newton
4
M.Stuhlinger/M.Smith, ESAC
EPIC Telemetry
M. Stuhlinger
XMM-Newton
5
M.Stuhlinger/M.Smith, ESAC
Offset Median
Increase in offset median: 2 – 5 ADU for Q0 CCDs since ~ Rev 1410
Perhaps other CCDs also, e.g. CCD5
Coincides with latest PN BPT implementation (Rev 1409); however, the changes in the BPT affected CCD11 only…
Similar to onset of theoffset median trend seen in Revs 605 – 660
M. Smith
XMM-Newton
6
M.Stuhlinger/M.Smith, ESAC
Offset Median (cont.)
Regarding the Rev 605 – 680 offset median trend:
A correlation was found with the respective Quadrant VC Currents (params F1189-92)
(discussed at the Saclay 2003 Ops Meeting)…
J. Fauste, S. Rives
M. Smith
XMM-Newton
7
M.Stuhlinger/M.Smith, ESAC
Offset Median (cont.)
F1189: Q0 VC Current
…however, in the recent trend:
NO correlation with VC Current found.
G. Buenadicha, P. Calderon
M. Smith
XMM-Newton
8
M.Stuhlinger/M.Smith, ESAC
Offset VarianceFirst Observations per Revolution
Eclipse Season Boundaries
Behaviour still not understood
M. Smith
XMM-Newton
9
M.Stuhlinger/M.Smith, ESAC
M. Kirsch
Energy Scale vs Time very good, esp. for FF mode.
Slight over-correction for EFF mode.
SW mode under-correction, esp. at Mn
(Result of SAS 7.1 Processing)
XMM-Newton
10
M.Stuhlinger/M.Smith, ESAC
M. Kirsch
Line width trend is stable
~0.5 ADU/year increase at Mn
(Result of SAS 7.1 Processing)
M. Kirsch
XMM-Newton
11
M.Stuhlinger/M.Smith, ESAC
MOS Monitoring
Mallorca, November 2007
XMM-Newton
12
M.Stuhlinger/M.Smith, ESAC
MOS1 Bad Pixels MOS2
Still fewer Bad Pixels than before cooling
Nevertheless, steadily increasing trend for most CCDs
M. Smith
XMM-Newton
13
M.Stuhlinger/M.Smith, ESAC
New MOS fixed offsets from Rev. 1400 onwards.
MOS fixed offsets lowered by 1 ADU for:
- MOS1 CCD 5
- MOS2 CCDs 1, 2, 3 and 6
M. Smith
XMM-Newton
14
M.Stuhlinger/M.Smith, ESAC
M. Stuhlinger
XMM-Newton
15
M.Stuhlinger/M.Smith, ESAC
MOS1_Al_width.ps
M. Stuhlinger
XMM-Newton
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M.Stuhlinger/M.Smith, ESAC
M. Stuhlinger
XMM-Newton
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M.Stuhlinger/M.Smith, ESAC
Low Energy Noise (MOS2CCD5-Effect):
MOS2
MOS1
XMM-Newton
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M.Stuhlinger/M.Smith, ESAC
Low Energy Noise (MOS2CCD5-Effect):
XMM-Newton
19
M.Stuhlinger/M.Smith, ESAC
Due to Charge Injection?
RAWY
~40
XMM-Newton
20
M.Stuhlinger/M.Smith, ESAC
Charge Injection Spectra along RAWY