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GSFC XMM-Newton GOF Status Report #192: XMM-NEWTON NEWS #105



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_/           XMM-NEWTON  NEWS   #105   ---  15-Apr-2010           _/
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             XMM-Newton Science Operations Centre at
              ESA's European Space Astronomy Centre,
P.O. Box - Apdo. 78, 28691 Villanueva de la Canada, Madrid, Spain

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SOC Home Page:
  http://xmm.esac.esa.int/
Helpdesk web interface:
  http://xmm.esac.esa.int/external/xmm_user_support/helpdesk.shtml
Helpdesk email address:
  xmmhelp@sciops.esa.int
News Mailing List:
  http://xmm.esac.esa.int/external/xmm_news/news_list/index.php

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Contents:

- XMM-Newton Users Group meeting #11: comments to UG members are welcome
- XMM-Newton Workshop "Ultra-Luminous X-ray sources and Middle
   Weight Black Holes": programme and abstract booklet available
- Incorrect EPIC band-4 fluxes in the 2XMM and 2XMMi catalogues: problem
   description and correct data


XMM-Newton Users Group meeting #11: comments to UG members are welcome
======================================================================

The date of the next  Users Group (UG) meeting is 12th - 13th May, 2010. A
dedicated Web page of the Users Group is available at:

     http://xmm.esac.esa.int/external/xmm_user_support/usersgroup/

This web page provides, among others, the contact points for all interested
astronomers to send their comments and  suggestions to the UG members prior
to the meeting.

Please find herewith the agenda:

     1.  Welcome                                 M. Arnaud
     2.  Adoption of the agenda                  All
     3.  Overall mission status                  A. Parmar
     4.  Instrument operations                   R. Munoz
     5.  Report of the Project Scientist         N. Schartel
     6.  Calibration
       6.1 EPIC Calibration status               M. Guainazzi
           (and cross-calibration MOS/pn and
           Timing mode)
       6.2 RGS Calibration status                A. Pollock
           (and cross-calibration RGS/EPIC)
       6.3 OM Calibration status                 A. Talavera
       6.4 Cross-calibration status              M. Stuhlinger
           with other missions
     7.  SAS developments and future plans       C. Gabriel
     8.  SSC status                              M. Watson
     9.  Action items from last meeting          M. Ehle
     10. Input from the community                Mission Scientists
     11. General discussion/AOB                  All
     12. Dedicated discussion                    UG
     13. Date and time of next meeting           UG


XMM-Newton Workshop "Ultra-Luminous X-ray sources and Middle Weight
Black Holes": programme and abstract booklet available
===================================================================

As announced in issues #95, #103 and #104 of this Newsletter, the  XMM-Newton
Science Operations Centre is organising an astrophysical workshop from Monday
24th to  Wednesday 26th of  May 2010 at the  European Space Astronomy  Centre
(ESAC) near Madrid, Spain.

The programme and abstract booklet for this workshop are now available online
at the workshop website:

http://xmm.esac.esa.int/external/xmm_science/workshops/2010_science/


Incorrect EPIC band-4 fluxes in the 2XMM and 2XMMi catalogues:
problem description and correct data
==============================================================

The XMM-Newton Survey Science Centre (SSC) has uncovered an error in the 2XMM
and 2XMMi catalogues which needs to be brought to the  attention of users  of
these catalogues.

The key points are:

1) The error affects only the computation of the EPIC band 4 (2.0-4.5keV) flux
values for detections  (the EP_4_FLUX column) and  the corresponding  quantity
(the SC_EP_4_FLUX column) for unique sources when one or more of the 
constituent
detections is  affected. The  relevant (OBSMLI)  source lists  held in the XSA
archive also contain the incorrect EP_4_FLUX value.

2) Statistically, the impact of the error is that the correct EPIC band 4 flux
values are systematically larger than the erroneous values (typically by a few
sigma) - the mean shift is about a factor 2. While the scale of the correction
is modest, we emphasize that the uncorrected values are simply wrong and  that
the impact on XMM-Newton science analyses that exploit the EPIC  band 4 fluxes
can be significant.

A fuller description of the problem, its background and access to 
down-loadable
files containing the correct data is available from

http://xmmssc-www.star.le.ac.uk/Catalogue/ep4_flux/ep4flux.html

The new incremental version of the catalogue, 2XMMi-DR3, planned for 
release in
late April 2010, contains the correct EPIC band 4 fluxes. It will be  
available
soon from

http://xmmssc-www.star.le.ac.uk/Catalogue

and other  hosting sites listed therein, including the XSA.



Yours sincerely,
XMM-Newton SOC


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