1 / 17

ACTIONS

ACTIONS. EPIC_10/1 on Munoz. Closed: MS delivered Slew Data Files EPIC_10/2 on Smith: to verify whether PHS_tools checks for optical loading in the complete pn fov Open ?? EPIC_9/2 on Altieri: to provide new CCFs reflecting the current MOS bad pixels . Closed with latest CCF/SAS release

larya
Download Presentation

ACTIONS

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. ACTIONS • EPIC_10/1 on Munoz. • Closed: MS delivered Slew Data Files • EPIC_10/2 on Smith: to verify whether PHS_tools checks for optical loading in the complete pn fov • Open ?? • EPIC_9/2 on Altieri: to provide new CCFs reflecting the current MOS bad pixels. • Closed with latest CCF/SAS release • EPIC_8/1 on Palombara: to propose work-around for EMDH limitation of 50 bad pixels flagged per CCD(cooling perhaps makes it less critical)

  2. ACTIONS (from cooling review) AI Wrap-1:on the SOC (MK) to summarise current planning for CALCLOSED measurements with a view confirming PI agreement to the strategy at the EPIC/TTD/Calibration meeting. AI Wrap-2 :on the SOC (MK) to specify any ongoing monitoring of CCDnoise with a view to confirming a strategy with the PI atthe upcoming EPIC TTD/Calibration Meeting. AI Wrap-3 :on the SOC (MK) to specify current planning for bright-pixelmonitoring with a view to confirming a strategy with the PI at the upcoming EPIC TTD/Calibration Meeting.

  3. Status of science operationsEPIC OPS Meeting 03. January 2003University of Tübingen (IAAT)

  4. Content • Instruments, S/C & Cal. • XSA, SAS, misc. • operational efficiency • radiation: “space weather” • spacecraft status • v manoeuvre (Mauro)

  5. INSTRUMENTS AND S/C GENERAL : • Earth Limb constraintset(from47) to 42 degrees • Single boresight died: it put the OVIII Ly alpha lineontoRGS defect • Meteor shower avoidance : • Perseids (Revs.490 and 491) and Leonids (Revs.538 and 540) avoidance • probable meteoroid impact occurred on Rev.490 few-frame flash seen on MOS2: no lasting effects seen • in the following days the "MOS blobs" were noticed • Eclipse season in September (another one coming up)

  6. INSTRUMENTS AND S/C(Contd.) EPIC : • MOS cooling (to -120)(see talk of LM) • new temperature calibration • pn Full Frame with masking tested(see talk of UB) • optimization of the pn Offset per observation(see talk of EK) RGS : • RGS cooling (to -110) • RGS HTR mode (not in A03)

  7. CALIBRATION GENERAL : • enhanced installation of SciSIM. Commitment to maintenance. • new portal for calibration: http://xmm.vilspa.esa.es/external/xmm_sw_cal/calib/index.shtml • Capella cross-calibration with Chandra: GRB021004 killed first effort second attempt it went ahead with simultaneous observations EPIC : • See specific calibration talks and Cooling report RGS : • RGS IDT believes great improvements of wavelength calibration possible • key is better pointing reconstruction.

  8. XSA • XSA v1.5 release on 15/11/2002 • Product and Postcard Server • custom retrieval • dataset size indicator • links to publications • tar option in shopping basket • quota on volume

  9. SAS • Version 5.4.1 of the Science Analysis System released • need a new SAS Manual version soon • full restructuring of the SAS web pages done in period • VilSpa took over of SAS RGS tasks from Columbia • second SAS workshop (very positive feedback)

  10. MISCELLANEOUS • intensive efforts on HEASARC-based RPS tool for A03 • CD distribution to PIs to be discontinued beginning 2003 notification of data availability through XSA • SOC contact for EPIC OPS/Cal. meetings  Marcus K. from time to time have a look at: http://xmm.vilspa.esa.es/

  11. MOS1 efficiency 103-525

  12. MOS1 efficiency: 436-525

  13. PN efficiency 103-525

  14. pn efficiency: 436-525

  15. observing statistics XMM Time Targets 96.0% 91.2% 19.1% 93.7% 89.6% 16.2%

  16. radiationby courtesy of Rosario Gonzalez Riestra ESA(XMM-RGS) RGS count rate bg region of CCD9 29-31 h after Perigee 34-38 h after Perigee Revolution RGS count rate bg region of CCD9 38-41 h after Perigee 41-43 h after Perigee Time (~Revolution) Phase

  17. spacecraft status • All spacecraft subsystems on primary chain. No redundancy used sofar. • hydrazine: ~5 kg/year • solar power: nominal • earth limb constraint : since 10/02 47º  42 º • next eclipses: 19/02/2003 until 13/03/2003

More Related