Neutrino Point Source Searches with AMANDAII mDAQ - PowerPoint PPT Presentation

About This Presentation
Title:

Neutrino Point Source Searches with AMANDAII mDAQ

Description:

Neutrino Point Source Searches with AMANDA-II m-DAQ. Jim Braun ... Neutrino Point Source Searches with AMANDA-II m-DAQ. 3. Data Filtering. Two main data sets: ... – PowerPoint PPT presentation

Number of Views:53
Avg rating:3.0/5.0
Slides: 10
Provided by: jbr6
Category:

less

Transcript and Presenter's Notes

Title: Neutrino Point Source Searches with AMANDAII mDAQ


1
Neutrino Point Source Searches with AMANDA-II
m-DAQ
  • Jim Braun

2
m-DAQ Point Source Searches
Would like to combine all years into a reasonably
unified final event sample and publish point
source result in early 2008 Sample will also be
used by John K. and others
3
Data Filtering
  • Two main data sets
  • 2000-2004 Filtered to L3 (1G events ? 1M
    events) with Zeuthen scheme
  • 2005-2006 Filtered to L3 with UW scheme
  • Zeuthen and UW filtering very similar
  • Do not need to refilter to achieve a reasonably
    uniform event sample

4
Final Event Sample
  • Final event samples are significantly different!
  • Zuethen 2000-2004
  • Strong likelihood difference cut (downgoing vs.
    unconstrained)
  • Strong P_hit smoothness cut
  • Strong paraboloid error cut
  • 1K events/year
  • High Purity
  • UW 2005-2006
  • Weaker likelihood difference cut at horizon
  • Weaker P_hit smoothness cut
  • Strong paraboloid error cut
  • Weak direct length cut
  • Maximum sensitivity near horizon

5
Event Selection
  • Need a uniform event selection for all years
  • Non-uniform selection is confusing
  • Non-uniform selection would tend to combine the
    undesirable properties of both selections
  • Choose Zeuthen cuts for final event sample
  • Match 2000-2004 publication
  • 91 of events from 2005-2006 with Zeuthen cuts
    are already contained in UW sample

6
Final Event Sample
6166 Total events in final sample
7
Normalization
  • Data normalized to average of Barr et al. and
    Honda 2006 model atmospheric neutrino predictions
  • Corrects for uncertainties in MC
  • (e.g. ice properties, OM sensitivity)
  • Final normalization 0.901
  • ? Ratio of starting/final normalization indicates
    sample is 97 pure

8
Final Sample
9
Final Sample
Write a Comment
User Comments (0)
About PowerShow.com