Äîêóìåíò âçÿò èç êýøà ïîèñêîâîé ìàøèíû. Àäðåñ îðèãèíàëüíîãî äîêóìåíòà : http://xmm.vilspa.esa.es/calibration/documentation/epic_cal_meetings/201504/Santos_Cal_2015.pdf Äàòà èçìåíåíèÿ: Fri Apr 10 16:10:19 2015 Äàòà èíäåêñèðîâàíèÿ: Wed Apr 13 13:32:05 2016 Êîäèðîâêà: Ïîèñêîâûå ñëîâà: m 101

Science Support Status

Maria Santos-Lleo EPIC calibration meeting, ESAC 9 April 2015


Overview
XMM-Newton Mission extension approved for 2 more years Team moves are now frequent, thank you to those who left (excellent contribution appreciated!) and welcome to new, very motivated people! Science Programme continues in good shape (next call in October) We keep on: calibrating (EPIC and) the other instruments, i.e. RGS and OM delivering data, improving the SAS, pipeline processing and archiving and organizing workshops

Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 2


Mission Extension
"During its meeting at the European Space Astronomy Centre, near Madrid, on 19 November, the
ESA' Science Programme Committee (SPC) gave the green light for the flotilla of spacecraft to continue their key scientific endeavours for at least another two years. (...) Decisions to extend ESA space science missions are made on a rolling two-year schedule. The next two-year mission extension cycle will begin in mid-2016."

XMM-Newton funded until end 2016 and
extension approved until end 2018, subject to review late 2016

Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 3


Science Support Team
Leaves: Anna Lia Longinotti: 15 Aug 2014

Matteo Guainazzi: 1 Sep 2014
New: Michael Smith EPIC Calibration Scientist Arrivals: Jacobo Ebrero, 21 April 2014 Simone Migliari, 2 Feb 2015 Jose Vicente Perea, pipeline software engineer, 7 April 2014
Science Operations | M. Santos-Lleo | EPIC calibration ! 9 April 2015 | Pag. 4


Community Support and Mission Planning: science programme
AO 13: Soon to be finished (end April)
95% of A+B time performed
50% of C time performed

A O 14 : t o s t a r t i n M a y
· Deadline was 10 October 2014 5.7 oversubscription · Results, 10 December. Two Very Large Programmes: ­ 1.6 Ms: z=0.4 blazar for WHIM ­ 1.4Ms: Draco dwarf galaxy: dark matter line?

A O 15
· Call for proposals 25 August ­ 9 October (12:00 UT) 2015 · OTAC results mid Dec 2015 · Phase II: 12 Jan ­ 5 Feb 2016
Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 5


Instruments: RGS and OM

Smooth operations for all instruments, no instrument anomalies (see Pedro Calderon´s talk) RGS meeting 7-8 April
· Summary by Rosario GonzÀlez (RGS Calibration Scientist)

OM fast mode improvements and upgrades used in catalogue processing

Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 6


Users Group: recommendations
Resolution 2014-04-11/04: The UG noted with satisfaction the enormous progress in the

calibration areas that were identified in 2013 as highest priorities, in particular
a) The on-going EPIC MOS-pn cross-calibration and multi-mission effective area calibration
b) The Timing Mode energy scale calibration which is now accurate to ~20 eV c) The start of the Burst Mode calibration activities d) The updated PSF calibration based on EPIC-pn Timing Mode data

e) The RGS absolute wavelength calibration scale, now accurate to 5-7 må.

Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 7


Users Group: recommendations
Recommendation 2014-04-11/01: The UG establishes the following priorities for the calibration activities: 1. Continue progress on non-finished issues should be the top priority: a. Finalise cross-calibration among EPIC cameras, with a proper scientific validation, within the next months and continue monitoring EPIC-RGS cross-calibration.

b. EPIC-pn issues to be fixed within SAS 14: fix the different calibration between single and double events, re-engineering of the long-term CTI and correct for the timeevolution of energy resolution.
c. Continue the Burst Mode calibration activity, leading to a new calibration in ~1 year timeframe. 2. Understanding the background for low-surface brightness observations a. Recognise Dr. David Lumb's contributions and encourage him to continue with the on-going progress on stray-light in-orbit calibration activities b. Make progress on the characterisation of the particle-generated background (either through protons or reflected X-rays) in the EPIC cameras
Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 8


Data analysis and archive
SAS (see Carlos Gabriel´s talk)
· SAS 14.0 released 10 Nov 2014

· SAS 15 planned for Autumn 2015

PPS (see Pedro Rodriguez´s talk)
· full responsibility for dev and ops, changes agreed with SSC (CCB) · PPS-sas14-based released Feb 2015

Catalogues
· 3XMM-DR5, incremental EPIC source catalogue to be released next week (TBC) · OM catalogue: new incremental update ready, includes all 2013 data

X SA
· XSA v8.3 released 4 Dec 2014 · Next release linked to 3XMM-DR5 release (i.e. next week TBC) · `old' XSA discontinued
Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 9


Data and Science Workshops
SAS Workshop 2014, 2 ­ 6 June at ESAC No SAS workshop planned for 2015 (lack of resources) Symposium: "The X-ray Universe 2014" 16 ­ 19 June in Dublin
· Participation: 335 scientists · Presentations are on the XMM SOC web, and indexed in ADS

Science workshop 2015: The Extremes of Black Hole Accretion, 8-10 June, ESAC

Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 10


Thank you

15 years of XMM-Newton 10 December 2014

Thank you for continuous contribution and support Questions?
Design: Ignacio de la Calle
Science Operations | M. Santos-Lleo | EPIC calibration | 9 April 2015 | Pag. 11