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	<title>Comments on: Bump Hunting (Redux)</title>
	<atom:link href="http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/feed/" rel="self" type="application/rss+xml" />
	<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/</link>
	<description>Random samplings from a universe of ideas.</description>
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		<title>By: tommaso dorigo</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33071</link>
		<dc:creator>tommaso dorigo</dc:creator>
		<pubDate>Sun, 09 Dec 2007 22:43:40 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33071</guid>
		<description>Hi John,

I let a few weeks pass before pitching in on this, now that fewer eyes are looking. What I really would like to know is the details of the modeling of the QCD background, the fat red histogram that is responsible for the shape of the falling spectrum at high reconstructed mass.

Because, if I am not mistaken, the fact that you now see no excess is due to a remodeling of the QCD background (which used to be quite a bit leaner in the 1/fb analysis). So I really wonder, was it really a statistical fluctuation or a systematic underestimate of the background ?

Sorry for being quite direct... I decided not to post on this issue in my blog and just ask you here. If the new QCD model is better than the old one it is entirely to your credit, not the other way round. I think you, Anton and the others did a terrific job and I cannot see a way to improve the analysis.

Cheers,
T.</description>
		<content:encoded><![CDATA[<p>Hi John,</p>
<p>I let a few weeks pass before pitching in on this, now that fewer eyes are looking. What I really would like to know is the details of the modeling of the QCD background, the fat red histogram that is responsible for the shape of the falling spectrum at high reconstructed mass.</p>
<p>Because, if I am not mistaken, the fact that you now see no excess is due to a remodeling of the QCD background (which used to be quite a bit leaner in the 1/fb analysis). So I really wonder, was it really a statistical fluctuation or a systematic underestimate of the background ?</p>
<p>Sorry for being quite direct&#8230; I decided not to post on this issue in my blog and just ask you here. If the new QCD model is better than the old one it is entirely to your credit, not the other way round. I think you, Anton and the others did a terrific job and I cannot see a way to improve the analysis.</p>
<p>Cheers,<br />
T.</p>
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		<title>By: Thomas D</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33047</link>
		<dc:creator>Thomas D</dc:creator>
		<pubDate>Tue, 30 Oct 2007 18:19:04 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33047</guid>
		<description>I&#039;m not sure I like the smell of the phrase &#039;to catch wind of breaking news&#039;...</description>
		<content:encoded><![CDATA[<p>I&#8217;m not sure I like the smell of the phrase &#8216;to catch wind of breaking news&#8217;&#8230;</p>
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		<title>By: loses to monkeys</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33070</link>
		<dc:creator>loses to monkeys</dc:creator>
		<pubDate>Sat, 27 Oct 2007 18:28:32 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33070</guid>
		<description>what&#039;s plotted on the y axis of those graphs? people never label axis these days!</description>
		<content:encoded><![CDATA[<p>what&#8217;s plotted on the y axis of those graphs? people never label axis these days!</p>
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		<title>By: jlm</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33069</link>
		<dc:creator>jlm</dc:creator>
		<pubDate>Fri, 26 Oct 2007 12:27:48 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33069</guid>
		<description>Hi John,

I&#039;m confused. If I look at the paper you linked to describing this analysis
I see that the combined efficiency listed for a 90 (250) gev higgs is 1.0% (3.1%).
And the cdf higgs webpage has a paper describing the 1.0/fb analysis which
lists the combined efficiency for the same masses as 1.1% (3.3%).  Also, the
ratio of the total number of predicted taus faking jets in the two analyses is 1.6 (slightly less than the 1.8 that comes just from luminosity scaling).

So it doesn&#039;t appear that a looser event selection has led to increased predictions for the signal or the fake background.  However, as I wrote in my previous post, it looks like the prediction for the jet faking tau background in the mass region the excess was observed in the 1.0/fb analysis has increased by 3.5 instead of 1.8.  Did I misunderstand your answer?</description>
		<content:encoded><![CDATA[<p>Hi John,</p>
<p>I&#8217;m confused. If I look at the paper you linked to describing this analysis<br />
I see that the combined efficiency listed for a 90 (250) gev higgs is 1.0% (3.1%).<br />
And the cdf higgs webpage has a paper describing the 1.0/fb analysis which<br />
lists the combined efficiency for the same masses as 1.1% (3.3%).  Also, the<br />
ratio of the total number of predicted taus faking jets in the two analyses is 1.6 (slightly less than the 1.8 that comes just from luminosity scaling).</p>
<p>So it doesn&#8217;t appear that a looser event selection has led to increased predictions for the signal or the fake background.  However, as I wrote in my previous post, it looks like the prediction for the jet faking tau background in the mass region the excess was observed in the 1.0/fb analysis has increased by 3.5 instead of 1.8.  Did I misunderstand your answer?</p>
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		<title>By: Eric</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33046</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Fri, 26 Oct 2007 03:23:12 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33046</guid>
		<description>John, you&#039;re right--after rereading your posts I agree that you were more fair than I gave you credit for.  Guess I succumbed to the usual irresistible temptation of over-sarcasm (it&#039;s quite enjoyable).  ;)</description>
		<content:encoded><![CDATA[<p>John, you&#8217;re right&#8211;after rereading your posts I agree that you were more fair than I gave you credit for.  Guess I succumbed to the usual irresistible temptation of over-sarcasm (it&#8217;s quite enjoyable).  <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_wink.gif' alt=';)' class='wp-smiley' /> </p>
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		<title>By: Brian Drell</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33044</link>
		<dc:creator>Brian Drell</dc:creator>
		<pubDate>Fri, 26 Oct 2007 01:45:54 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33044</guid>
		<description>Glad to know LHC hasn&#039;t lost usefulness before they even collide beam.

;)</description>
		<content:encoded><![CDATA[<p>Glad to know LHC hasn&#8217;t lost usefulness before they even collide beam.<br />
 <img src='http://blogs.discovermagazine.com/cosmicvariance/wp-includes/images/smilies/icon_wink.gif' alt=';)' class='wp-smiley' /> </p>
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		<title>By: John</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33043</link>
		<dc:creator>John</dc:creator>
		<pubDate>Thu, 25 Oct 2007 17:35:57 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33043</guid>
		<description>Hi jlm (#22): the reason the background did not scale is that we loosened our selection a bit to get better sensitivity (more backgorund but more signal too...)

Eric, #25, apaprently you didn&#039;t read my original posts.  I think if you go back and do your homework, you can tone down the sarcasm a bit.   I never hyped anything...the media did.  It was a typical cycle with this sort of fluctuation.  The main point is if the Higgs *had* been there this is *exactly* how it would have appeared.  My first post, and this one, was all about how important it is to remain skeptical, while being human.  This is exciting!  Are you saying you never expect to see a Higgs anywhere?

In response to your comment #28, our estimate of the probability of a fluctuation *of course* took into account that a fluctuation could have been anwhere.  This was discussed in the first posts, which, as I say, you really should take the tme to read.  I stand by every word I wrote.</description>
		<content:encoded><![CDATA[<p>Hi jlm (#22): the reason the background did not scale is that we loosened our selection a bit to get better sensitivity (more backgorund but more signal too&#8230;)</p>
<p>Eric, #25, apaprently you didn&#8217;t read my original posts.  I think if you go back and do your homework, you can tone down the sarcasm a bit.   I never hyped anything&#8230;the media did.  It was a typical cycle with this sort of fluctuation.  The main point is if the Higgs *had* been there this is *exactly* how it would have appeared.  My first post, and this one, was all about how important it is to remain skeptical, while being human.  This is exciting!  Are you saying you never expect to see a Higgs anywhere?</p>
<p>In response to your comment #28, our estimate of the probability of a fluctuation *of course* took into account that a fluctuation could have been anwhere.  This was discussed in the first posts, which, as I say, you really should take the tme to read.  I stand by every word I wrote.</p>
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		<title>By: Eric</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33050</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Thu, 25 Oct 2007 02:01:04 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33050</guid>
		<description>Furthermore, there is an experimental bias because one selectively pays attention to fluctuations that occur in quantities of interest and ignores fluctuations elsewhere.  An experimenter should really consider the probability of getting a 2-sigma fluctuation *anywhere* (not just here), which is pretty high due to combinatorics.  J. Conway is reputed to be a statistics guru, so maybe that was done, I&#039;m not sure.</description>
		<content:encoded><![CDATA[<p>Furthermore, there is an experimental bias because one selectively pays attention to fluctuations that occur in quantities of interest and ignores fluctuations elsewhere.  An experimenter should really consider the probability of getting a 2-sigma fluctuation *anywhere* (not just here), which is pretty high due to combinatorics.  J. Conway is reputed to be a statistics guru, so maybe that was done, I&#8217;m not sure.</p>
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		<title>By: Eric</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33068</link>
		<dc:creator>Eric</dc:creator>
		<pubDate>Thu, 25 Oct 2007 01:48:37 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33068</guid>
		<description>Neil, there&#039;s no obvious way to know, assuming all other checks have been made.

A 3-sigma effect is decent, but any good particle experimentalist will tell you that 5 sigma is the gold standard.  Many people (especially theorists) ask:  a 3-sigma fluctuation is so statistically unlikely already--why need 5?  The answer:  Well, the probability of a 5 sigma is exponentially suppressed compared to 3 sigma.  But more saliently, it also offers robustness against mistakes in error estimation.  For example, if you accidentally underestimate your error by a factor of 2, your great 3-sigma effect now becomes a 1.5 sigma effect, which happens quite frequently.  Similar reasoning applies to error estimation from Monte Carlo, which may not properly model new physics, etc.

The point of having 5 sigma is so that claims of discovery are robust against not only statistical fluctuations, but also against experimenter-related mistakes.  Until one is near that, I think it&#039;s misleading to imply a near-discovery (as it seemed to me was done here at CV, New Scientist, etc.)  There was no legitimate reason to hype up the result so much.</description>
		<content:encoded><![CDATA[<p>Neil, there&#8217;s no obvious way to know, assuming all other checks have been made.</p>
<p>A 3-sigma effect is decent, but any good particle experimentalist will tell you that 5 sigma is the gold standard.  Many people (especially theorists) ask:  a 3-sigma fluctuation is so statistically unlikely already&#8211;why need 5?  The answer:  Well, the probability of a 5 sigma is exponentially suppressed compared to 3 sigma.  But more saliently, it also offers robustness against mistakes in error estimation.  For example, if you accidentally underestimate your error by a factor of 2, your great 3-sigma effect now becomes a 1.5 sigma effect, which happens quite frequently.  Similar reasoning applies to error estimation from Monte Carlo, which may not properly model new physics, etc.</p>
<p>The point of having 5 sigma is so that claims of discovery are robust against not only statistical fluctuations, but also against experimenter-related mistakes.  Until one is near that, I think it&#8217;s misleading to imply a near-discovery (as it seemed to me was done here at CV, New Scientist, etc.)  There was no legitimate reason to hype up the result so much.</p>
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		<title>By: Neil B.</title>
		<link>http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/comment-page-1/#comment-33067</link>
		<dc:creator>Neil B.</dc:creator>
		<pubDate>Thu, 25 Oct 2007 01:04:00 +0000</pubDate>
		<guid isPermaLink="false">http://blogs.discovermagazine.com/cosmicvariance/2007/10/22/bump-hunting-redux/#comment-33067</guid>
		<description>OK... Eric (or anyone) have we advanced in our ability to figure whether a given marginal signal is likely real or just noise etc?  The basic simple math has been known and likely not changed for awhile, but I figure there have been advances (whether in the math or the computational power.)  I don&#039;t hear much about it.</description>
		<content:encoded><![CDATA[<p>OK&#8230; Eric (or anyone) have we advanced in our ability to figure whether a given marginal signal is likely real or just noise etc?  The basic simple math has been known and likely not changed for awhile, but I figure there have been advances (whether in the math or the computational power.)  I don&#8217;t hear much about it.</p>
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