'Epic pn' diaporamas de présentation

Adjustment of spatial gain variations of EPIC pn

Adjustment of spatial gain variations of EPIC pn. Gain correction factors. EPIC-pn:. image of all events with 20 adu in rev 332, processed without epreject. image of all events with 20 adu in rev 332, processed with epreject.

823 views • 73 slides

Adjustment of spatial gain variations of EPIC pn

Adjustment of spatial gain variations of EPIC pn. Gain correction factors. EPIC-pn:. image of all events with 20 adu in rev 332, processed without epreject. image of all events with 20 adu in rev 332, processed with epreject.

741 views • 73 slides

Correcting spatial inhomogeneities of the absolute energy scale

Correcting spatial inhomogeneities of the absolute energy scale. EPIC Calibration & Operations Meeting. Madrid, 2010 March 23-24. EPIC-Cal Meeting, MPE-Garching, Germany, 2006 May 4. 20 adu image, rev 546. Correcting spatial inhomogeneities of the absolute energy scale.

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EPIC pn: Update on the CTI, the absolute energy scale and the energy resolution

EPIC pn: Update on the CTI, the absolute energy scale and the energy resolution. FF. FF Mn-K CTI CCD 1 - 6. FF Mn-K CTI CCD 7 - 12. FF Mn-K CTI Quadrant 0. FF Al-K CTI Quadrant 0. FF Al-K CTI Quadrant 0. FF Mn-K FWHM CCD 1 - 6. ff.

520 views • 45 slides

Adjustment of spatial gain variations of EPIC pn

Adjustment of spatial gain variations of EPIC pn. Gain correction factors. EPIC-pn:. rev 80, K ? line energy (keV). no oot correction, no epreject. rev 80, K ? line energy (keV). no oot correction, no epreject. before launch. EPIC-pn: HK981002_MnK_1_col117. = ccd 5, col 11.

507 views • 42 slides

Status of XMM-Newton cross-calibration with SAS-6.1 B.Altieri

Status of XMM-Newton cross-calibration with SAS-6.1 B.Altieri with inputs/support from whole cross-calibration team (XMM SOC, Leicester, MPE ). Talk outline. Response stability at low energies : SNR (extended) AGN view (trend analysis)

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Long-term behaviour of the CTI.. for EPIC pn

Long-term behaviour of the CTI.. for EPIC pn. FF Mn-K CTI CCD 1 - 6. FF Mn-K CTI CCD 7 - 12. FF Mn-K CTI Quadrant 0. FF Al-K CTI Quadrant 0. FF Mn-K FWHM CCD 1 - 6. ff. FF Mn-K FWHM CCD 7 - 12. FF Mn-K FWHM Quadrant 0. ff.

456 views • 36 slides

476 views • 36 slides

Bruno Altieri on behalf of the cross-calibration team

Status of the XMM- Newton Cross-calibration. EPIC-MOS. EPIC-pn. RGS. OM. Bruno Altieri on behalf of the cross-calibration team. Cross-calibration team. Leicester : Steve Sembay(MOS rmf) , Andy Read MPE : Frank Haberl (EPIC-pn rmf), Michael Freyberg

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Bruno Altieri ESAC, 18.05.2005

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347 views • 21 slides

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Agenda:

Agenda:. Apologies: SS WP. Actions from last meeting (taken from minutes) 1/4. - 1.0 Action Items from last meetings (AR) - AI_EPIC_BG_WG_01_01: SS to provide by October 2005 to SOC - Proton screening tool

207 views • 20 slides

Health and cleanliness of the XMM- Newton science payload since launch

Health and cleanliness of the XMM- Newton science payload since launch.

307 views • 19 slides

An XMM-Newton view of Q2122-444: an AGN without Broad Line Region?

An XMM-Newton view of Q2122-444: an AGN without Broad Line Region?. Mario Gliozzi (GMU) L. Foschini (IASF Bo) R. Sambruna (GSFC) L. Kedziora-Chudczer (Sidney). * Type I and Type II AGN Unification Model HBLR vs non-HBLR

288 views • 18 slides

Science Operations Status

302 views • 14 slides

Science Operations Status

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Science Operations Status

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Crab: the standard X-ray candle with all (modern) X-ray satellites

Crab: the standard X-ray candle with all (modern) X-ray satellites.

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Supersoft and quasi-soft X-ray sources in the core of M31

Supersoft and quasi-soft X-ray sources in the core of M31. Marina Orio, INAF-Torino and University of Wisconsin (2005 preprint on supersoft X-ray sources in M31). The lower limit on the X-ray luminosity is

78 views • 7 slides