Martin Stuhlinger Mallorca, 06.11.2007 European Space Astronomy Centre Page 1 XMM-Newton ESAC Status of XMM-Newton cross-calibration with SASv7.1 CAL Meeting.

Slides:



Advertisements
Similar presentations
Astrometry and EPIC flux cross-calibration in 2XMMp/2XMM Silvia Mateos R. Saxton, S. Sembay and the XMM-Newton Survey Science Centre.
Advertisements

Epic-Cal 4 Feb 2003 Flux check Richard Saxton XMM-SOC/SSC Flux Comparisons.
AGN FEEDBACK IN TWO INTERESTING GROUPS F. Gastaldello (IASF-MI, UCI) D. Buote (UCI), P. Humphrey (UCI), W. Mathews (UCSC), F. Brighenti (U. Bologna), P.
Clusters as calibration tools S. Molendi (IASF-MI)
Comparison of XMM-Newton EPIC, Chandra ACIS-S3, ASCA SIS and GIS, and ROSAT PSPC results for G , 1ES , and MS A “Man on the street”
Strange Galactic Supernova Remnants G (the Tornado) & G in X-rays Anant Tanna Physics IV 2007 Supervisor: Prof. Bryan Gaensler.
Soft X-ray line reflection in NLS1 galaxies Th. Boller, A. Müller, A. Ibarra MPE Garching Excellence Cluster Universe Munich XMM SOC, Villa Franca, Spain.
Bruno Altieri EPIC Calibration meeting, Feb. 1-3, 2005 European Space Astronomy Centre Page 1 XMM-Newton ESAC Status of XMM-Newton cross-calibration with.
EPIC flux comparison from 2XMM sources S. Mateos, R. Saxton, S. Sembay & A. Read.
XMM 1 EPIC MOS Monitoring CAL/OPS Meeting MPE
Chandra Calibration Status ACIS 1.Gain correction files for epochs 30, 31 and 32 were released in CALDB (Sept 2007), (Dec. 2007) and
Chandra Calibration Status ACIS 1.Gain correction files for epochs 33 and 34 were released in CALDB (June 2008) and (Sep. 2008). HETG 1. An.
XMM EPIC MOS Steve Sembay ESAC 04/10/05 Implementation of the MOS spatial/temporal DRM: Does it work ? Zeta Puppis: Checking the line.
XMM-Newton/ Chandra Cross Calibration with Clusters of Galaxies CXC Calibration Workshop October L. David, J. Nevalainen, M. Bonamente, D. Jerius,
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton EPIC The XMM-Newton cross-calibration.
European Space Astronomy Centre Villafranca del Castillo, Madrid, Spain Andy Pollock XMM-Newton SOC RGS calibration Calibration of the XMM-Newton RGS Andy.
XMM-Newton 1 M.Stuhlinger/M.Smith, ESAC PN Monitoring Mallorca, November 2007.
XMM EPIC MOS Steve Sembay EPIC Calibration Meeting Saclay 24/09/03 Epoch dependant MOS QE and RMF and Cross-calibration with the PN.
European Space Astronomy Centre Villafranca del Castillo, Madrid, Spain A.M.T. Pollock XMM-Newton SOC EPIC calibration October 2006 Calibration of.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Marcus G. F. Kirsch Mallorca, Summary status of the EPIC calibration.
XMM-Newton 1 M.Stuhlinger, March 2010 Status of XMM-Newton cross-calibration using SASv10.0 Madrid, 24. March 2010.
Normal Galaxies Sample From 2dF-XMM Wide Angle Survey Jonathan Tedds, Silvia Mateos, Mike Watson, Matthew Page, Francisco Carrera, Mirko Krumpe, Jacobo.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton MOS Timing Mode calibration Marcus.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton EPIC Calibration of the EPIC MOS Timing.
Chandra Calibration Status  Recent releases  Current Calibration projects  Cross-Calibration between Chandra and other X-ray telescopes  Revisions.
MOS 3x3 mode slow slew survey Richard Saxton October 2006.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton XMM Newton cross calibration M.G.F.
XMM 1 MOS2 CCD5 anomaly Status of the investigations.
1 XMM-Newton Extended Source Analysis Software Steve Snowden & Kip Kuntz  Publicly Released 5 April 2006  XMM-Newton Extended Source Analysis Software.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton EPIC Cross calibration PKS
XMM-Newton 1 A.Garcia, ESAC Spectral effects of PSF core excisting Madrid, 24. March 2009.
An XMM-ESAS Update Steve Snowden NASA/Goddard Space Flight Center EPIC Operations and Calibration Meeting - BGWG Palermo - 11 March 2007.
High-Resolution X-ray Spectroscopy of AGN Warm Absorbers Rebecca Smith MSSL, UCL with G. Branduardi-Raymont and M. Page.
XMM-Newton 1 Michael Smith, ESAC PN Monitoring Mallorca, October 2006.
XMM EPIC MOS Steve Sembay Mallorca 26/10/06 MOS spectral redistribution function has evolved temporarily and spatially whilst in orbit.
Chandra X-Ray Observatory CXC Paul Plucinsky February A Comparison of Spectral Fit Results of E0102 from the Chandra and XMM CCDs Paul Plucinsky.
Low frequency radio observations of galaxy groups With acknowledgements to: R. Athreya, P. Mazzotta, T. Clarke, W. Forman, C. Jones, T. Ponman S.Giacintucci.
XMM 1 EPIC MOS Monitoring CAL/OPS Meeting Mallorca
Chandra X-Ray Observatory CXC Paul Plucinsky EPIC Cal October Comparison of RGS Model for 1E to the HETG data 2.BI CCD CTI Correction.
Vadim Burwitz EPIC Cal., Nov 6, 2007 Update on the Low Energy Isolated Neutron Star and White Dwarf Cross-Calibration Standards Vadim Burwitz EPIC Calibration.
1 Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton Ops. AGENDA Operations status and.
Martin Stuhlinger X-Ray Universe 2005, Sep.26-30, 2005 European Space Astronomy Centre Page 1 XMM-Newton ESAC Status of XMM-Newton cross-calibration with.
XMM 1 EPIC MOS Monitoring. XMM-Newton 2 Martin Stuhlinger, ESAC MOS Bad Pixel Monitoring.
XMM EPIC MOS Steve Sembay Mallorca 02/02/05 Temporal and spatial variability of the MOS RMF 1.Introduction and brief history of the.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Long term EPIC in-orbit calibration plan Marcus G. F. Kirsch.
XMM EPIC MOS Steve Sembay Mallorca 06/11/07 Report on three NRCO calibration observations On axis observation of absorbed Seyfert.
Chandra X-Ray Observatory CXC Paul Plucinsky EPIC Cal Update on ACIS Calibration 1) Update to the ACIS contamination model 2) Temperature-dependent.
Astronomical GRID Applications at ESAC Science Archives and Computer Engineering Unit Science Operations Department ESA/ESAC.
1 XMM-Newton Extended Source Analysis Software Steve Snowden & Kip Kuntz  Publicly Released 5 April 2006  XMM-Newton Extended Source Analysis Software.
RXJ a soft X-ray excess in a low luminosity accreting pulsar La Palombara & Mereghetti astro-ph/
The variable X-ray spectrum of PDS456 and High-Velocity Outflows Shai Kaspi Technion – Haifa; Tel-Aviv University Israel & Ehud Behar, James Reeves “ The.
The IACHEC Matteo Guainazzi XMM-Newton Science Operations Centre ESAC-ESA.
The X-ray Universe September 2005, El Escorial, Madrid, Spain The XMM-Newton Slew Survey XMM-Newton Slew 1 (XMMSL1) Fig 1. Slew observation.
X-ray astronomy 7-11 September 2009, Bologna, Italy XMM-Newton slew survey hard band sources XMM-Newton slew survey hard band sources R.D. Saxton a, A.M.
Cross-Calibration between XMM-Newton and Chandra Herman L. Marshall Chandra X-ray Center, MIT Kavli Institute.
The XMM SSC Bright Source sample * November 2006 Report to the SSC XID R. Della Ceca A. Caccianiga T. Maccacaro P. Severgnini F. Cocchia * on behalf of.
Extreme soft X-ray emission from the broad-line quasar REJ R.L.C. Starling 1*, E.M. Puchnarewicz 1, K.O. Mason 1 & E. Romero- Colmenero 2 1 Mullard.
X-ray emission properties of BLAGN in the XMM-2dF Wide Angle Survey S. Mateos, M.G. Watson, J. A. Tedds and the XMM-Newton Survey Science Centre Department.
A new look at AGN X-ray spectra - the imprint of massive and energetic outflows Ken Pounds University of Leicester Prague August 2006.
Chandra X-Ray Observatory CXC Paul Plucinsky IACHEC March Thermal SNR Working Group: Summary Report Paul Plucinsky on behalf of the IACHEC Thermal.
Lockman Hole (XMM PV) PN CCD (MPE Garching) MOS1 CCD (Leicester U) PN CCD (MPE Garching) MOS1 CCD (Leicester U) PV Observations ksec.
Monitoring the Seyfert Galaxy Mkn766 Continuum and Fe line variability Mkn766 is a highly variable Seyfert 1 galaxy. The richness of.
Metal abundance evolution in distant galaxy clusters observed by XMM-Newton Alessandro Baldi Astronomy Dept. - University of Bologna INAF - OABO In collaboration.
Swift observations of Radio-quiet Fermi pulsars Swift and the Surprising Sky 24th-25th November 2011 In collaboration with Patrizia Caraveo and Andrea.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Status of the EPIC calibration Presentation for XMM Newton UG 18 May 2006 Marcus.
XMM-Newton 1 Michael Smith, ESAC PN Monitoring Mallorca, April 2008.
EVALUATION OF THE XMM NEWTON CROSS CALIBRATION ARCHIVE
Cross-Cal paper Kristin Kruse Madsen.
XMM v Chandra - Cluster Analysis
A.Malizia, L. Bassani , M. Molina
Presentation transcript:

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 1 XMM-Newton ESAC Status of XMM-Newton cross-calibration with SASv7.1 CAL Meeting Mallorca, November 2007 Martin Stuhlinger with inputs/support from whole cross-calibration team

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 2 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 3 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 4 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 5 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 6 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 7 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 8 XMM-Newton ESAC Flux ratios using 3C273 SASv7.1SASv7.0

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 9 XMM-Newton ESAC AGN

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 10 XMM-Newton ESAC H : Single Power Law PL. Index PN:1.812 ±0.003 ±0.003 MOS1:1.773 ±0.006 ±0.006 MOS2:1.801 ±0.008 ±0.008 RGS1:1.86±0.03 RGS2:1.88±0.03

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 11 XMM-Newton ESAC Galaxy Clusters

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 12 XMM-Newton ESAC Galaxy Clusters

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 13 XMM-Newton ESAC Galaxy Cluster: Temperatures A3112MKW3s PN 4.06±0.05 keV 3.23±0.05 keV MOS1 4.29±0.09 keV 3.32±0.07 keV MOS2 4.14±0.09 keV 3.16±0.07 keV

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 14 XMM-Newton ESAC Low Energy Stability: RXJ

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 15 XMM-Newton ESAC RXJ : Absorbed black body Energy band keV N H [10 19 cm -2 ] Temperature [eV] Norm. 1keV [10 -4 ] PN6.7± ± ±0.03 MOS ± MOS2 < ± ±0.01

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 16 XMM-Newton ESAC Cross-calibration archive  to go public by end 2007 to go public by end 2007 to go public by end 2007  Current content: –~ 250 observations –~ 150 checked in for automated processing (XMM only) –~ 20 checked in for automated processing (XMM-Chandra) –all will be checked in by end 2007 (definition of extraction region/times and check for pile up needs to be checked and iterated ONCE manually)  Using ESAC grid: –10 nodes so far, each node has 2 CPUs Intel(R) Xeon(TM) 3.00GHz with 6GB of memory ➡ process and fit 150 Observations /24 hours

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 17 XMM-Newton ESAC Cross-calibration: Statistics SASv6.5 SASv7.0 SASv7.1

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 18 XMM-Newton ESAC XMM-Newton / Chandra

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 19 XMM-Newton ESAC XMM-Newton / Chandra

Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 20 XMM-Newton ESAC XMM-Newton / Suzaku Suzaku extraction script ready. Spectral slopes agree well. Correct normalisation still slightly unclear due to open questions on data extraction.