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		<updated>2015-03-18T07:49:27Z</updated>

		<summary type="html">&lt;p&gt;1 revision imported&lt;/p&gt;
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		<author><name>Lhep</name></author>
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	<entry>
		<id>https://wiki.lhep.unibe.ch/index.php?title=Nicola&amp;diff=356&amp;oldid=prev</id>
		<title>Lhep at 02:37, 12 March 2010</title>
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		<updated>2010-03-12T02:37:51Z</updated>

		<summary type="html">&lt;p&gt;&lt;/p&gt;
&lt;p&gt;&lt;b&gt;New page&lt;/b&gt;&lt;/p&gt;&lt;div&gt;== Walk-through presentation ==&lt;br /&gt;
&lt;br /&gt;
Link to Indico talk [http://indico.cern.ch/getFile.py/access?contribId=0&amp;amp;resId=0&amp;amp;materialId=slides&amp;amp;confId=71656]&lt;br /&gt;
&lt;br /&gt;
&lt;br /&gt;
== Comments Michele ==&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&amp;lt;span style=&amp;quot;background:red&amp;quot;&amp;gt;&lt;br /&gt;
Prepare a table with the cross sections and expected number of events after selection cuts for 10 pb-1&lt;br /&gt;
W + 0,1,2 jets (note _jets_, not partons)&lt;br /&gt;
&amp;lt;span style=&amp;quot;background:#00FF00&amp;quot;&amp;gt;&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Same for background, and also Wbb, Wcc. Include k-factors to NLO.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
Prepare plots of signal+background (for example W transverse mass) to&lt;br /&gt;
get a feeling on how good the signal could be detected (again&lt;br /&gt;
normalized to 10 pb-1).&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
Get the numbers/plots above for 7 TeV, or describe how you will be&lt;br /&gt;
quickly able to get 7 TeV estimates.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
Get an estimate for 900 GeV too.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Define the measurement to be done. Likely W+0/W+1 ? Alpha_s ? &lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Who else in ATLAS will be doing this measurement ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
What are the plans and timescales of the W+jets ATLAS group for a&lt;br /&gt;
similar measurement ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
What can/has to be done with MC until January/February ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
You will have to use release 15. Do this asap and report issues.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Describe how data quality and luminosity are implemented in the&lt;br /&gt;
analysis.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
How will duplicated events be removed ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Prepare technical howto on how alpha_s can be changed in the MC and&lt;br /&gt;
how and when you can get such samples for testing the analysis&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Prepare a detailed list of samples that you need, as much as possible&lt;br /&gt;
add the file names, release, location of the files, etc...&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Tell us how you are going to get a multi-jet/QCD sample (from data,&lt;br /&gt;
who is going to provide it for you ?)&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Which background samples are you getting from data, which ones&lt;br /&gt;
from MC ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Evaluate the CPU hours you will need (order of magnitude) and disk space&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
How is you analysis run ? grid ? All configs in some TopAnalysis.py ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
How will you make sure that certified code is used ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
What is the location of your analysis code in SVN (preferrably in&lt;br /&gt;
ATLAS, Bern also OK)&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
What will be the backup trigger if the single electron 20 GeV is not&lt;br /&gt;
usable ? What is the efficiency ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Will all the data you need be in the e-gamma stream ? Do you need&lt;br /&gt;
other streams ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
How will the trigger efficiency be applied to MC ? As a weight ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Will the trigger efficiency plateau be evaluated as a function&lt;br /&gt;
of eta ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Describe possible systematics studies to be done on a comparison&lt;br /&gt;
between Alpgen and Herwig MC. Or also Pythia, Sherpa, etc...&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Make a list of expected systematic uncertainties and describe where&lt;br /&gt;
will you will be taking them from. In particular for the ratio&lt;br /&gt;
measurement.&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Prepare a technical howto for changing the jet-energy-scale for&lt;br /&gt;
systematics evaluation. Also evaluate to what level the JES has to be&lt;br /&gt;
known as a function of jet energy (do not forget the low energies).&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Describe in detail the jet reconstruction and object definition&lt;br /&gt;
criteria you will use including jet quality. Also describe the jet&lt;br /&gt;
corrections  you will use (muons in jet ? what scale ? overlaps ?&lt;br /&gt;
include track-jet information ? reconstruction pt threshold ?&lt;br /&gt;
generator pt threshold in MC ? Etc...&lt;br /&gt;
What jet branch are you using ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
Describe the Met reconstruction and corrections you will use. What is&lt;br /&gt;
the expected Met resolution ? Met branch ?&lt;br /&gt;
&lt;br /&gt;
----&lt;br /&gt;
&lt;br /&gt;
e-jet overlap: evaluate on MC, how often the &amp;quot;electron&amp;quot; was actually a&lt;br /&gt;
jet/quark/gluon (mistake in overlap removal)&lt;/div&gt;</summary>
		<author><name>Lhep</name></author>
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