Influence of sky pixelisation on False Discovery Rate method for

Transcription

Influence of sky pixelisation on False Discovery Rate method for
Influence of sky pixelisation on False Discovery Rate method for
Point Sources Analysis
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
What about ...

Sky pixelisation definition

Analysis principles

FDR Method 
Influence of the binning on the FDR

Conclusions and Outlook Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Sky Pixelisation
 Binning characteristics, taking into account the symetries of the
detector :
Constant solid angle : Equal Area
Iso­latitude pixelisation 3 differents pixelisations :
RECTANGLE
RECTANGLE­SINUS
RHOMBUS
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Defined by several parameters
Mathieu Labare
Université Libre Bruxelles
Pixelisation Parametrisation
RHOMBUS
N ≠ 0
N = 0
Rectangular
1 SINUS 0 RECTANGLE­SINUS
RECTANGLE
NROWS
SOLID_ANGLE
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Analysis Principles
 Systematical analysis on 10 000 skies randomized on right
ascension
 Wich binning would be the most efficient for Point Source Analysis ?
 Parameters optimisation in order to be as close as possible to
the required FDR.
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Analysis Principles
 Compute the amount of neutrinos in a sky bin  number ev.
 backgroung  significance nnu[j] Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Analysis Principles
 Background calculation row(j)
 number ev.
 backgroung  significance nbg[i] = Avg(nnu[k]) k ∈ row(i) k≠i Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Analysis Principles
 Compute the significance following a Poisson Law
 number ev.
 backgroung  significance sign[i] = ­ log(p[i])
∞
−nbg[i] nbg[i]
p[i]= ∑ e
x!
x=nnu[i]
Belgian IceCube Meeting
Brussels ­ July 6th 2006
x
Mathieu Labare
Université Libre Bruxelles
Rejection of Null Hypothesis
 Previously : 3 rejection 54.9 % of rejection
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Rejection of Null Hypothesis
 Now : FDR ­ Method
1.13 % of rejection
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
FDR vs Solid Angle
 RECTANGLE Work in progress
Restrictions on the parameters ?
Belgian IceCube Meeting
Brussels ­ July 6th 2006
RHOMBUS N=3 Mathieu Labare
Université Libre Bruxelles
FDR vs Solid Angle
 RECTANGLE ­ SINUS
Work in progress
linear behaviour ?
RHOMBUS N=3 Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
FDR vs Solid Angle
 RECTANGLE ­ SINUS
Work in progress
linear behaviour ?
stability ?
error estimation ?
...
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Pseudo­sources distributions
 RECTANGLE ­ SINUS 6
4
5
3
5
12
10
3
6
5
11
7
5
18
4
7
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Pseudo­sources distributions
 RECTANGLE 0
4
10
1
4
7
6
9
12
6
8
5
11
7
7
8
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Pseudo­sources distributions
 RHOMBUS 3
9
10
4
7
3
8
7
10
8
9
8
7
9
9
6
8
Belgian IceCube Meeting
Brussels ­ July 6th 2006
Mathieu Labare
Université Libre Bruxelles
Conclusions & Outlook
 Seems to have some interesting behaviors that have to be well understood :
 Strong influence of the pixelisation and its parameters  Links with the symetries of the detector (solid angle,
declination dependance,...)
 Systematical analysis will continue with others parameters :
 Shift on the binning
 Another calculation of the background
 Incorporation of a simulated Point Source
Belgian IceCube Meeting
th
Brussels ­ July 6 2006
Mathieu Labare
Université Libre Bruxelles

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