XMM-Newton 1 M.Stuhlinger, March 2010 Status of XMM-Newton cross-calibration using SASv10.0 Madrid, 24. March 2010.

Slides:

Advertisements

Similar presentations

WORK PLAN FOR THE EPIC CALIBRATION TEAM (AND BEYOND)

Advertisements

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

Epic-Cal 4 Feb 2003 Flux check Richard Saxton XMM-SOC/SSC Flux Comparisons.

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”

XMM EPIC Andy Read IACHEC 2013 Leicestershire, UK, 25-28/03/13 XMM-Newton EPIC Cross- Calibration Andy Read With contributions from Matteo.

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.

24-28 October 2005 Elena Belsole University of Bristol Distant clusters of Galaxies Ringberg Workshop X-ray constraints on cluster-scale emission around.

Statistical analysis of the X-ray emission properties of type-1 AGN in the XMM-2dF Wide Angle Survey Silvia Mateos Leicester University (UK) Leicester.

Jonathan Gimeno Boal, UCM MODEL PSF EFFECTS OF PILE-UP Jonathan Gimeno Boal, UCM Tutor: Martin Stuhlinger.

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.

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 Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton MOS Timing Mode calibration Marcus.

Chandra Calibration Status  Recent releases  Current Calibration projects  Cross-Calibration between Chandra and other X-ray telescopes  Revisions.

I. Balestra, P.T., S. Ettori, P. Rosati, S. Borgani, V. Mainieri, M. Viola, C. Norman Galaxies and Structures through Cosmic Times - Venice, March 2006.

Matteo Guainazzi ESAC-ESA M.Guainazzi, "Status of EPIC-pn timing mode calibration", EPIC-BOC, Madrid, 23/3/2010.

XMM EPIC SOC Richard Saxton Background, Operations & Calibration (BOC) meeting Mallorca, 30/03/09-01/04/09 The Timing Mode PSF Richard Saxton, Maria Diaz.

Testing the EPIC hard band calibration S. Molendi (IASF/CNR)

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.

Chandra Calibration Status  Highlights of the IACHEC Meeting  Updates to the LETG/HRC-S calibration  Continuous Clocking (CC) mode calibration.

XMM-Newton 1 A.Garcia, ESAC Spectral effects of PSF core excisting Madrid, 24. March 2009.

Early Results from SWIFT's BAT AGN Survey: XMM Follow-up Observations for 22 BAT AGNs Lisa Winter Lisa Winter (Grad Student at UMD) Richard Mushotzky (GSFC),

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

XMM 1 EPIC MOS Monitoring CAL/OPS Meeting Mallorca

XMM EPIC MOS Andy Read EPIC Calibration Meeting Saclay 24/09/03-25/09/03 Analysis of the X-ray PSF PSFs in the CCF MCG C273.

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.

Guillermo Buenadicha SOC Operations Support Group Page 1 XMM-Newton Status of EPICs Operations Guillermo Buenadicha PALERMO 11/04/07.

XMM EPIC MOS Steve Sembay EPIC Calibration Meeting Ringberg 2-5/April/2002 Broad-Band MOS v PN Cross-Calibration Study 8 Observations.

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.

Matteo Guainazzi Science Operations & Data Systems Division Research & Scientific Support Department “Stellar-mass, intermediate-mass and supermassive.

XMM-Newton observation of the distant (z  0.4) galaxy clusters: RX J , RX J and RX J Sergey Anokhin,

RXJ a soft X-ray excess in a low luminosity accreting pulsar La Palombara & Mereghetti astro-ph/

Conclusions We established the characteristics of the Fe K line emission in these sources. In 7 observations, we did not detect the source significantly.

The variable X-ray spectrum of PDS456 and High-Velocity Outflows Shai Kaspi Technion – Haifa; Tel-Aviv University Israel & Ehud Behar, James Reeves “ The.

RAS National Astronomy Meeting April 2006, University of Leicester, UK The XMM-Newton Slew Survey The excellent sensitivity of the XMM-Newton.

Are Atlantic basin tropical cyclone intensity forecasts improving? Jonathan R. Moskaitis 67 th IHC / 2013 Tropical Cyclone Research Forum Naval Research.

XMM-Newton surveys of X-ray galaxy groups Alexis Finoguenov MPE/UMBC+ S.Giodini, V.Allevato, M. Tanaka, A. Leauthaud, O. Ilbert, N.Cappelluti, J.Silverman,

Jet/environment interactions in FR-I and FR-II radio galaxies Judith Croston with Martin Hardcastle, Mark Birkinshaw and Diana Worrall.

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.

The nature of X-ray selected Broad Absorption Line Quasars Alex Blustin With Tom Dwelly (Southampton), Mat Page (UCL-MSSL)‏ UCL-MSSL and IoA, Cambridge.

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.

Discovery of ABSORPTION LINES in Low Mass X-ray Binaries: MXB and GX13+1 L. Sidoli (IASF, Milano) A.N. Parmar T. Oosterbroek D. Lumb & C. Erd.

X-ray Absorption and Scattering by Interstellar Dust: the XMM view Elisa Costantini Max Planck Institute for extraterrestrial Physics (MPE) P. Predehl,

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.

Chandra X-Ray Observatory CXC Paul Plucinsky IACHEC March Thermal SNR Working Group: Summary Report Paul Plucinsky on behalf of the IACHEC Thermal.

An XMM-Newton View of the Luminous X-ray Source Population of M101 Leigh Jenkins Tim Roberts, Robert Warwick, Roy Kilgard*, Martin Ward University of Leicester,

Andrii Elyiv and XMM-LSS collaboration The correlation function analysis of AGN in the XMM-LSS survey.

X-ray observation of the Cygnus Loop with Suzaku and XMM-Newton

Metal abundance evolution in distant galaxy clusters observed by XMM-Newton Alessandro Baldi Astronomy Dept. - University of Bologna INAF - OABO In collaboration.

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.

The XMM Distant Cluster Project: Survey limits and Pilot Survey Georg Lamer A. Schwope, V. Hambaryan, M. Godolt (AIP) H. Böhringer, R. Fassbender, P. Schücker,

Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton Feedback between circumnuclear gas and AGN: implications.

New XMM-Newton deep Survey in the Lockman Hole Vincenzo Mainieri MPE Workshop on AGN Surveys, Puebla, June 23- July 11, 2003 Guenther Hasinger Hans Boehringer.

The X-ray Universe September 2005, El Escorial, Madrid, Spain Extended Sources in the XMM-Newton slew survey V. Lazaro a, R. Saxton a, A.M.Read.

Multi-wavelength behaviour of III Zw 2

XMM-Newton slew sources A quick analysis

XMM v Chandra - Cluster Analysis

A.Malizia, L. Bassani , M. Molina

Long-term trends in EPIC pn energy response

Presentation transcript:

XMM-Newton 1 M.Stuhlinger, March 2010 Status of XMM-Newton cross-calibration using SASv10.0 Madrid, 24. March 2010

XMM-Newton 2 M.Stuhlinger, March 2010 Example: 1H SW modes without pile-up. Absorbed single power law model.

XMM-Newton 3 M.Stuhlinger, March 2010 Examples: Recent observations SW modes with pile-up. PKS : Absorbed broken power law model. 3C273: Absorbed double power law model.

XMM-Newton 4 M.Stuhlinger, March 2010 Example: Galaxy clusters FF modes. Absorbed plasma model (mekal). A2029:kT ~ 7.2 keV A262: kT ~ 2.2 keV

XMM-Newton 5 M.Stuhlinger, March 2010 M. Stuhlinger Statistical evaluation: Flux distributions

XMM-Newton 6 M.Stuhlinger, March 2010 Statistical evaluation: Time evolution

XMM-Newton 7 M.Stuhlinger, March 2010 Statistical evaluation: Flux distribution 2XMM MOS1/pnMOS2/pn Matteo Guainazzi

XMM-Newton 8 M.Stuhlinger, March 2010 Statistical evaluation: Time evolution 2XMM Matteo Guainazzi MOS1/pnMOS2/pn

XMM-Newton 9 M.Stuhlinger, March 2010 Summary Statistical analyses of XCAL archive (dominated by piled-up SW observations) and 2XMM sample (285 pile-up free FF observations) are consistent. Significant spread between single observations in nearly all energy bands, both for fluxes and slopes. EPICs show only weak flux time evolution for higher energies (>0.85 keV), some evolution is seen at lower energies (<0.85 keV). RGS and EPIC fluxes diverge with time at low energies. Nearly no time evolution of EPIC/RGS slopes in any of the energy bands.