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Temporal &Spatial Dependency of the MOS RMF
1ES
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MOS1 Thin filter 0447
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MOS2 Thin filter 0433 0447
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- Able to do spectral analysis of on- and off-‘patch’ regions
1ES0102 keV images ‘Good’ spectra – clean images ‘Bad spectra’ – bright ‘patch’ - Able to do spectral analysis of on- and off-‘patch’ regions
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MOS1 Rev375 MOS1 Rev375 MOS1 Rev447 MOS2 Rev447 ‘patch’ ‘patch’ ‘non-patch’ ‘non-patch’
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Only 0447 lies on MOS1 Boresight
11 obs. Only 0447 lies on MOS1 Boresight 0447 MOS1 Boresight
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Only 0433 & 0447 lie on MOS2 Boresight
12 obs. Only 0433 & 0447 lie on MOS2 Boresight 0433 0447 MOS2 Boresight
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- Investigate possible photon damage at boresights
- Stacking of all-pattern, all-energy images from all imaging mode observations MOS1 (CCD1) 3249 Event Files Events MOS2 (CCD1) 3223 Event Files Events
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- Investigate possible photon damage at boresights
- Comparison of boresight positions (pn/RGS prime) with stacked images (zoom) MOS1 MOS2 RGS prime 299,299 RGS prime 309,295 pn prime 315,291 pn prime 303,305 310 300 290 280 300 320 290 310
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N132D Mos1 Searching for ‘patch’ in other datasets/objects… 0283 Thin
keV keV keV keV 0283 Thin 0606 Med 0771 Thin No Thin filter, ‘On-Patch’ Observations 0828 Thin
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N132D Mos2 0283 Thin 0606 Med 0771 Thin No Thin filter, ‘On-Patch’
keV keV keV keV 0283 Thin 0606 Med 0771 Thin No Thin filter, ‘On-Patch’ Observations 0828 Thin
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N132D - Rev 0606 - Medium filter M1 - ‘On-Patch’ M1 M2 M2 0.1-0.35 keV
smoothed M2 M2 smoothed
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N132D Mos1 0474 - Medium filter 0538 0542 0552 0.1-0.35 keV
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N132D Mos2 0474 - Medium filter 0538 0542 0552 0.1-0.35 keV
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- No spatial evidence for ‘patch’ found in N132D (larger remnant - more complex, spatially and spectrally - no thin-filter, on-boresight observations) - Other Objects? Coma – Many observations – All Medium Filter Tycho – 1 observation – Medium filter Kepler – 1 observation – Thick filter (No such features [spectral enhancements, spatial ‘patch’] seen in pn analysis - remnant however sometimes on CCD gap, or non-thin filter used)
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1ES0102 - Proposed On- Boresight Raster Observation
- Performed in Revs 894/900 4 observations: - 894 - 900a - 900b1 & 900b2 (flare-damaged) - 900c
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0447
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0447
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0433 0447
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433&447
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- Fluxes calculated and compared (dotted lines show ±10% variation)
keV - Models (continuum + multi-Gaussian) fitted to spectra in narrow energy bands - Fluxes calculated and compared (dotted lines show ±10% variation) - On-Axis observations (433, 447, 894, 900) show marked departures from mean keV keV
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- Zoom of 894-900 region (all on-axis)
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- At higher energies, flux is very constant
keV - At higher energies, flux is very constant keV - Across whole energy band, flux is quite well conserved keV
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M1(raw/smoothed) M2(raw/smoothed)
MOS1 in timing mode keV RAWX/Y images M1(raw/smoothed) M2(raw/smoothed) from Revs. 433, 447, 894, 900(a,b1/2,c) - MOS2 patch is compact, stationary, distinct - MOS1 patch is fuzzier, not so distinct, more diffuse - Are able to compare ‘patch’ and ‘non- patch’ spectra ,as before…
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MOS1 Rev375 MOS1 Rev375 MOS1 Rev447 MOS2 Rev447 ‘patch’ ‘patch’ ‘non-patch’ ‘non-patch’
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- peak ‘level’ (?) reached by rev 447 - little evolution thereafter
M1 On-patch - peak ‘level’ (?) reached by rev 447 - little evolution thereafter 447 375 (off-axis)
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- low-moderate effect at rev 447 - moderate evolution thereafter
M1 Off-patch - low-moderate effect at rev 447 - moderate evolution thereafter 894 447 375 (off-axis)
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- moderate effect at rev 433/447 (lower than M1)
M2 On-patch - moderate effect at rev 433/447 (lower than M1) - moderate evolution (to peak level?) 447 375 (off-axis) 433
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- low (zero) effect at rev 433/447 - moderate evolution thereafter
M2 Off-patch - low (zero) effect at rev 433/447 - moderate evolution thereafter 375 (off-axis) 433 447
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On-patch – Off-patch M1 375 (off-axis) M2 375 (off-axis)
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On-patch – Off-patch M1 447 M2 447
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On-patch – Off-patch M1 894 M2 894
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On-patch – Off-patch M1 900a M2 900a
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On-patch – Off-patch M1 900c M2 900c
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Spatial Analysis of ‘Patch’
- Mosaic all ‘good’ off-axis sky (X/Y) images to obtain keV images of ‘non-patch’ remnant - Using knowledge of remnant detector position and observation position angle, rotate and flip this image to correct RAWX/RAWY position & orientation for each ‘bad’ on-axis pointing - Subtract rotated/flipped image from each ‘bad’ on-axis RAWX/RAWY image (correcting for relative exposures) to obtain images of the remainder – the ‘patch’
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- M1 patch is bright, and quite large already at rev 447
- Outer regions become larger and even brighter at later times
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- M2 patch is not as bright as M1, and is initially compact
- Outer regions become effected at later times
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Mosaics (raw & smoothed) of ‘patch’ images for MOS1
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Mosaics (raw & smoothed) of ‘patch’ images for MOS2
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- Patch is only visible when remnant illuminates the particular area of detector
- 1ES0102 acts like a torchlight – Final correction is made for this
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New Boresights? MOS2 MOS1 Obvious places that are close, equidistant from pn/RGS boresights (and by pn-RGS boresight offset) and with relatively little photon impact
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Discussion: Dealing with ‘The Patch’? – - New Boresight(s)? - Spatio-temporal RMF? - Correct on photon-by-photon basis?
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