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GSFC XMM-Newton GOF Status Report #069: Useful Information
Contents:
1) AO-3 scientific justification file size limitation
2) RGS Background files available (repeated notice)
3) PIMMS and WebPIMMS updated with AO-3 area curves
4) MOS low energy epoch-dependent response variation
5) U.S. XMM-Newton automatic data CD distribution to stop
6) Useful Information for XMM-Newton Data Analysis
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1) AO-3 scientific justification file size limitation
Please note that the size of the scientific justification
file to be uploaded with the AO-3 proposal submission
can not exceed 10 Mb. This requirement is listed on
pages 15/16 of the XMM-Newton Announcement of
Opportunity: Policies and Procedures.
http://xmm.vilspa.esa.es/external/xmm_science/AO3/ao3_policy_proc/node22.shtml
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2) RGS Background files available
RGS Background template event files have been provided by
T. Tamura, from the RGS Team at SRON. These files have been
derived from blank-sky observations, and have total exposure
times ranging from 80 to 390 ksec. They are useful when the
background cannot be accurately derived from the standard
off-axis regions, e.g. in the case of extended sources.
These files are accessible through the XMM-Newton Calibration
Portal at the following URL:
http://xmm.vilspa.esa.es/external/xmm_sw_cal/calib/index.shtml
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3) PIMMS and WebPIMMS updated with AO-3 area curves
PIMMS v3.3a has now been released which includes the latest
effective area curves for XMM-Newton, appropriate for use
for AO-3 proposals. If you had already run PIMMS for
your AO-3 proposal, please rerun them again now.
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4) MOS low energy epoch-dependent response variation
Recent observations of calibration targets confirm a significant
difference in the low energy redistribution characteristics of the
MOS cameras with respect to early observations.
More details can be read in Status Report #068:
http://heasarc.gsfc.nasa.gov/mail_archive/xmmnews/msg00064.html
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5) U.S. XMM-Newton automatic data CD distribution to stop
Beginning May 1, the U.S. XMM-Newton GOF will only be distributing
data CDs to PIs that request the service. While we will still
archive and encrypt the data for retrieval, in the near
future the XMM SOC in Vilspa will no longer send these CDs to us
as we will transition to a fully electronic transfer system.
If you have any questions on this policy, please write to:
xmmhelp@athena.gsfc.nasa.gov
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6) Useful Information for XMM-Newton Data Analysis
Below are links to information that you may find useful if you
haven't done much work with XMM-Newton and the SAS software
package. Please feel free to cut this out and post it on your
refrigerator or monitor for quick and easy referencing
> Observation Status - Does an observation contain the type of
data I'm looking for:
http://xmm.vilspa.esa.es/external/xmm_obs_info/obs_view_frame.shtml
> Getting the Data:
SOC: http://xmm.vilspa.esa.es/xsa/
GSFC: http://heasarc.gsfc.nasa.gov/db-perl/W3Browse/w3browse.pl
> Useful Documentation:
http://heasarc.gsfc.nasa.gov/docs/xmm/about_docs.html
> But you REALLY should at least read:
http://heasarc.gsfc.nasa.gov/docs/xmm/abc/
> Calibration Status information:
http://xmm.vilspa.esa.es/external/xmm_sw_cal/calib/index.shtml
> AO-3 Questions: (Deadline 30 April, 2003, 12:00 UT)
http://xmm.vilspa.esa.es/external/xmm_science/AO3/
> How to find out what a SAS error/warning message means:
From the SAS GUI select:
Help > Tasks
This will bring up a browser window with the following links:
Index of task warnings
Index of task errors
> XMM-Newton Publication List:
http://heasarc.gsfc.nasa.gov/docs/xmm/xmmhp_bibliography.html
> XMM-News Email archive:
http://heasarc.gsfc.nasa.gov/mail_archive/xmmnews/maillist.html
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