Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC A time jump analysis on EPIC-pn with some side results Marcus G. F. Kirsch M.J.

Slides:



Advertisements
Similar presentations
We can think of numbers being on a number line: These numbers are all positive numbers.
Advertisements

EPIC Calibration Meeting, K. Dennerl VILSPA/Spain, 2003 Mar Temporal variation of the energy response determined with the internal calibration source.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 ESAC Crab: the standard X-ray candle with all (modern) X-ray satellites M.G.F. Kirsch.
MATH 685/ CSI 700/ OR 682 Lecture Notes
XMM 1 EPIC MOS Monitoring CAL/OPS Meeting MPE
EPIC Calibration Meeting, MPE K. Dennerl, 2006 May 04 CTI.. update for EPIC pn Long-term behaviour of the CTI.. for EPIC pn.
XMM-Newton 1 Michael Smith, ESAC PN Monitoring MPE, May 2006.
Isabel Caballero, Anne Wellbrock Page 1 XMM-Newton ESAC XMM-Newton EPIC relative timing analysis Isabel Caballero Anne Wellbrock M.G.F. Kirsch.
XMM-Newton 1 Michael Smith, ESAC PN Monitoring Palermo, April 2007.
Guillermo Buenadicha SOC Operations Support Group Page 1 XMM-Newton EPIC SW Status Guillermo Buenadicha TOS/OFX, SOC Operations Support Group MPE, 4 th.
XMM-Newton 1 M.Stuhlinger/M.Smith, ESAC PN Monitoring Mallorca, November 2007.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Marcus G. F. Kirsch Mallorca, Summary status of the EPIC calibration.
EPIC Calibration Meeting, K. Dennerl Saclay/France, 2003 Sept Temporal variation of the energy response determined with the internal calibration.
EPIC Calibration Meeting, MPE K. Dennerl, 2006 May 04 EPIC pn at low energies: LW mode Properties of EPIC pn at low energies: LW mode.
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.
XMM-Newton 1 M.Stuhlinger/P.Calderon, ESAC Re-appearance of the MOS1 CCD1 meteorite column during revs Madrid, 23. March 2010.
EPIC Calibration Meeting, ESAC K. Dennerl, 2005 October 04 CTI.. update for EPIC pn Long-term behaviour of the CTI.. for EPIC pn.
XMM-Newton 1SCI-SA Status of MOS and PN Realtime Operations 1) Current Operations Status 2) Eclipse preparation improvements 3) Slew Exposures 4) Offset.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton EPIC Results from the EPIC- Calibration-Workshop.
XMM-Newton 1 Maria Santos-Lleo Science Operations Status EPIC Ops-Cal Meeting April 8, 2008, Mallorca María Santos-Lleó (XMM-Newton Science Support Manager)
EPIC Calibration Meeting, Mallorca K. Dennerl, 2006 October 26 EPIC pn: Jumps in the energy scale Sudden jumps in the absolute energy scale and their origin.
XMM 1 MOS2 CCD5 anomaly Status of the investigations.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton Status of EPIC time jump problems Marcus.
Pedro Calderón/Guillermo Buenadicha SOC Operations Support Group Page 1 XMM-Newton Status of EPICs Operations Pedro Calderón Riaño Guillermo Buenadicha.
EPIC TTD#16 SCIENCE OPERATIONS MPE, 04 May 2006 L. Metcalfe SCI-SDX XMM-Newton Science Support Manager 1 Science Operations & Data Systems Division Research.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Page 1 XMM-Newton EPIC Cross calibration PKS
EPIC Calibration Meeting, ESAC K. Dennerl, 2005 October 04 Adjustment of spatial gain variations Adjustment of spatial gain variations of EPIC pn.
EPIC Calibration Meeting, Mallorca K. Dennerl, 2006 October 26 CTI.. update for EPIC pn EPIC pn: Update on the CTI, the absolute energy scale and the energy.
EPIC Calibration Meeting, Mallorca K. Dennerl, 2006 October 26 Suppression of the low-energy noise Suppression of the low-energy noise: an improved approach.
XMM-Newton 1 Michael Smith, ESAC PN Monitoring Mallorca, October 2006.
Martin Stuhlinger Mallorca, European Space Astronomy Centre Page 1 XMM-Newton ESAC Status of XMM-Newton cross-calibration with SASv7.1 CAL Meeting.
Mallorca, 1st of February 2005 Page 1 XMM-Newton Status of EPICs Operations Stéphane RIVES 1st of February 2005.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC XMM-Newton Instrument Anomaly Tool & Cross-Calibration Tool Marcus G. F. Kirsch.
XMM 1Michael Smith, ESAC EPIC PN Monitoring Provided by Michael Smith.
The XMM slew survey: status and future Richard Saxton, Andrew Read, Michael Freyberg, Bruno Altieri.
EPIC Calibration Meeting, K. Dennerl VILSPA/Spain, 2004 March Detector noise & Vela observations application to Vela observations EPIC pn detector.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Correct treatment of fast mode ARFs Marcus G. F. Kirsch, G. Schoenherr, E. Kendziorra,
XMM 1 EPIC MOS Monitoring CAL/OPS Meeting Mallorca
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Energy calibration refinement of the EPIC-pn Burst mode M.G.F. Kirsch 1, E.
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.
Marcus Kirsch Science Operations & Data Systems Division Research & Scientific Support Department Amon Presentation: 23 April 2002Page 1 XMM-Newton In-Orbit.
XMM 1 EPIC MOS Monitoring. XMM-Newton 2 Martin Stuhlinger, ESAC MOS Bad Pixel Monitoring.
Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC Long term EPIC in-orbit calibration plan Marcus G. F. Kirsch.
EPIC Calibration Meeting, Madrid Correcting spatial inhomogeneities of the absolute energy scale K. Dennerl, 2010 March 23 Correcting spatial inhomogeneities.
Starter Write an equation for a line that goes through point (-3,3) and (0,3) y = 1/2 x + 3/2.
RAS National Astronomy Meeting April 2006, University of Leicester, UK The XMM-Newton Slew Survey The excellent sensitivity of the XMM-Newton.
SPIE, San Diego, CA - 1 August 2005 Bruno Altieri, XMM-Newton European Space Astronomy Centre Page 1 The XMM-Newton Slew Survey: processing challenges.
TIME TAGGING. HYPACK ® Timing Basics  The internal clock on your computer is a lousy clock.  HYPACK SURVEY and DREDGEPACK ® use a proprietary clock.
SAG+SASWG Meeting Potsdam /15 PN Tasks – Status Report (update since Leicester) Hermann Brunner - MPE  epframes:  The dark quadrant problem.
A look at XMM slew data Richard Saxton, Andrew Read, Michael Freyberg, Bruno Altieri, Puri Munuera.
The X-ray Universe September 2005, El Escorial, Madrid, Spain The XMM-Newton Slew Survey XMM-Newton Slew 1 (XMMSL1) Fig 1. Slew observation.
M. Pilar Esquej, XMM-Newton European Space Astronomy Centre Page 1 Status of the XMM-Newton Slew Survey P. Esquej, R. Saxton, B. Altieri, A. Read, M. Freyberg,
M. Pilar Esquej, XMM-Newton European Space Astronomy Centre Page 1 Status of the XMM-Newton Slew Survey P. Esquej, R. Saxton, B. Altieri, A. Read, M. Freyberg,
The Slow Slew Survey Richard Saxton / Pedro Rodriguez November 2006.
Status of EPIC operations Pedro Calderón Riaño, ESAC Leicester BOC meeting 6-8 March 2012.
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.
Ten Frame Practice Directions - Click the space bar. Look at the Ten Frame. Without counting, say the number of dots that are shown. Then, click the space.
Quantum Optics meets Astrophysics Frequency Combs for High Precision Spectroscopy in Astronomy T. Wilken, T. Steinmetz, R. Probst T.W. Hänsch, R. Holzwarth,
XMM-Newton 1 Michael Smith, ESAC PN Monitoring Mallorca, April 2008.
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.
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.
The XMM-Newton Slew Survey
EVALUATION OF THE XMM NEWTON CROSS CALIBRATION ARCHIVE
Soccer Team A: Soccer Team B:
EPIC Calibration & Operations Meeting
Karen Meech Institute for Astronomy TOPS 2003
Negative Numbers.
Long-term trends in EPIC pn energy response
Negative Numbers.
Presentation transcript:

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 1 EPIC ESAC A time jump analysis on EPIC-pn with some side results Marcus G. F. Kirsch M.J. Freyberg, E. Kendziorra

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 2 EPIC ESACmenu Do we still have time jumps? How can we measure those? Can a time jump detection be implemented in a sort of routine check (Qcheck)? Are there time issues that we still do not understand ?

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 3 EPIC ESAC What is a time jump CCD frames Photon a Photon b n*frame time If the time difference between the two arrival times of photon a and photon b is not a multiple of the frame time TIME JUMP

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 4 EPIC ESAC How to detect the jump Take all frame times in array: T =(T(i+1)-T(i))/frametime =difference of  to next full frametime Plot () If  >tolerance  time jump   0 Counting mode Time jumps

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 5 EPIC ESAC Mega processing Past: only known problem cases have been checked at MPE Now: processing of all public and non public available archive data at ESAC Some characteristic results: FFLWSW

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 6 EPIC ESACfindings Slope: –Is the clock drifting? –Are the frame times correctly used? Diagonal patterns: numerical effects

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 7 EPIC ESAC slopes for all ODF Different slopes for different modes LW similar to Burst –1E-5 Rest similar around 1E-5 Errors: –FF group: 1E-5 frametimes per frame Slight drift in frame times Oscillator stable, otherwise relative differences should show same shift Relative difference of measured frame time

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 8 EPIC ESAC resulting absolute error Burst, Timing and Small Window mode do show negligible absolute errors FF, eFF and LW show room for improvement  frame times are not fully correct  can be calibrated using the result of that analysis Measured error of frame time [sec] Not critical for exposure time and timing Analysis can be used to refine frame times with very high accuracy

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 9 EPIC ESAC Numeric effects mjf

Marcus Kirsch, XMM-Newton European Space Astronomy Center Page 10 EPIC ESAC How to proceed now Determine frametimes Repeat analysis with correct frametimes and search for time jumps