the epic-pn spectral response frank haberl epic cal meeting, tübingen, 3.-4. february 2003 status...

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The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments in the pn spectral response

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Page 1: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

The EPIC-pn spectral response

Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003

•Status of the pn spectral response in SAS5.4.1

•Latest developments in the pn spectral response

Page 2: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Status of the pn spectral response in SAS5.4.1

Last meeting (Vilspa July 2002) The Oxygen edge: Fudge to reduce the depth RX J1856.5-3754: Redistribution at low energies (PEM)

Now implemented (SAS5.4.1) New Quantum Efficiency curve RX J1856.5-3754: Redistribution re-adjustment SW mode CTI correction: reduce over-correction

Page 3: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

pn Quantum Efficiency (QE)

Page 4: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

RX J1856.5-3754 (PEM)

Page 5: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

PKS 2155 SW/TI medium EPIC-pn response 6.2

2 = 10700 / 2012 dof

Page 6: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

PKS 2155 SW medium EPIC-pn response 6.2+QE around O-edge

Page 7: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

PKS 2155 SW medium EPIC-pn response 6.3

Page 8: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Latest developments in the pn spectral response

The energy scale Au-edge, O-edge (BL Lacs) Emission lines (N132D and 1E0102) Vela SNR Long-term stability Internal cal source Isolated neutron stars

Page 9: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Energy shift at Au- and O-edge

Page 10: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Au-edge (SW mode)

Average 0.995 +- 0.001

Page 11: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

O-edge (SW mode)

Page 12: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

SNRs N132D and 1E0102

Page 13: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Spectrum

Page 14: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

O VII / VIII line energies

Average 1.004 +- 0.001

Page 15: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

PEM Energy to channel conversion

Page 16: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Vela SNR

0.2 – 1.2 keV Rev 533+534

Page 17: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Vela SNR spectra

Near CAMEX Away CAMEX

Page 18: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

O VII line energies in Vela

Page 19: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments
Page 20: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments
Page 21: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments
Page 22: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Long term trends (internal cal source)

Page 23: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Long term trends (internal cal source)

Page 24: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Long term trends (soft response)

Page 25: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Long term trends (soft response)

Page 26: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

RXJ0720.4-3125 pn summary

Revolution 0078 0175 0533 0534Readout mode FF FF FF FFFilter thin medium thin thinEvent pattern singles singles singles singles

Ext. rad. (´´) 40 40 40 40 87% PSFFlux (10-12 erg s-1) 9.78 9.92 9.74 9.78 0.1-2.4 keVFlux relative 1.000 1.015 0.995 1.002Flux (10-12 erg s-1) 11.24 11.40 11.20 11.24 PSF corrected PSPC: 11.5 LETG: 9.9Ext. rad. (´´) 20-40 15-40 20-40 20-40NH (1020) 1.55 1.69 1.68 1.39 typical error 0.2 LETG: 1.59Bbody kT (eV) 82.8 82.5 86.2 86.9 typical error 1.1 LETG: 81.6

Page 27: The EPIC-pn spectral response Frank Haberl EPIC Cal meeting, Tübingen, 3.-4. February 2003 Status of the pn spectral response in SAS5.4.1 Latest developments

Current status of EPIC-pn responsePN 6.4

CTI under correction at 600 eV in FF mode (Vela) change will influence all modes (increases energies which are already too high) needs ´gain´ reduction at low energies can be done in energy-channel conversion in PEMCTE degradation seems to slow down some further monitoring before action