Title: Systematic Astro Statistics
1Systematic Astro Statistics
Vinay Kashyap CHASC
Hyunsook Lee, Jeremy Drake, Pete Ratzlaff, David
van Dyk, Rima Izem, Xiao-li Meng, Taeyoung
Park, Aneta Siemiginowska, Alanna Connors,
Andreas Zezas
2CHASC
CHASC AstroStatistics Collaboration
c.1997 Chandra X-ray Center and Harvard
University AstroStatistics Collaboration
Chandra AstroStatistics Cabal
California-Harvard AstroStatistics Collaboration
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3CHASC
high-energy, low-counts, Poisson workshops,
papers, codes, weblog
4CHASC webpage http//hea-www.harvard.edu/AstroSta
t/
The AstroStat Slog http//groundtruth.info/AstroS
tat/slog/
5AstroStat Slog visibility Apr 10 - Apr 30, 2008
6Project Incorporate Systematic Error In X-ray
Data Analysis
The three most important effects that affect data
analysis Calibration! Calibration! Calibration!
7X-ray analysis from model to data
van Dyk et al. 2001, ApJ, 548, 224
8from there to here
(E,p,t) photon energy, location, arrival
time (E,p) detector channel, chip location S
astrophysical source model R energy
redistribution function (RMF) P position
redistribution function (PSF) A effective area
(ARF) M predicted model counts
9uncertainty in effective area
Drake, Ratzlaff, et al. (2005)
10uncertainty in energy response
11effect on model parameter uncertainty
Probability density
?
12but how exactly?
13MCMC
14DATA
CALIBRATION
Draw parameters
Compute likelihood
Update parameters
15DATA
CALIBRATION
Draw effective areas
Draw parameters
Compute likelihood
Update parameters
16but where do the effective areas come from?
17Principal Components
18eigenvector
eigenvalue
N (0,1)
new
nominal
bias
PCs
residual
A A0 bias components residual
19what have we got so far?
- realistic error bars
- implemented in BLoCXS
- Sherpa
- 100x drop in storage
- 500x speed up in analysis
- generalize to any instrument
- extendable to model lacunae
- roll your own
20whats next?
unified file format for ingestion into
XSPEC/Sherpa other schemes of dimensionality
reduction RMFs 2D PCA, within and between
PCA PSFs multiscale residuals
21effect on parameter uncertainty