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Matrix Template Matching Reloaded Third ATNF Gravitational Wave Workshop 2009 Willem van Straten. Synopsis. “The Matrix”: polarisation and pulsar timing invariant interval & matrix template matching “The One”: PSR J0437-4715 use bright source to calibrate itself “The Reload”: PSR J1022+1001
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Matrix Template Matching ReloadedThird ATNF Gravitational Wave Workshop 2009Willem van Straten
Synopsis • “The Matrix”: polarisation and pulsar timing • invariant interval & matrix template matching • “The One”: PSR J0437-4715 • use bright source to calibrate itself • “The Reload”: PSR J1022+1001 • use bright source to calibrate weak sources • “The Future”
Stokes 4-vector • Total intensity (time-like) S0 = I • Polarization vector (space-like) S = (S1, S2, S3)
Transformations Jones matrix, J Mueller matrix, M
Rotations and Boosts • Rotations: • rotate Sabout an axis by an angle • leave S0 unchanged • Boosts: • boost along an axis by a Lorentz factor • modify both S0 and S
Boosts: Instrumental • Non-orthonormality of receptors: • differential gain (along S1 axis) • cross-coupling (along S2 & S3 axes) • Mixing of S0 and S depends on S• • Produce pulse phase dependent distortions of total intensity profile
Template Matching P() = aS(+ ) + b FFT P() = aS()e-i2 + ()b
Frequency Domain • High frequency power yields greatest constraint on slope,
The One: PSR J0437-4715 • The good: • closest and brightest MSP known • narrow pulse peak • The ugly: • OPM sweep near pulse peak • TOA strongly distorted by calibration errors
Enter the Invariant • Form the invariant profile, Sinv(), whereSinv2 = S02 - |S|2 • Dramatically reduced systematic error in PSR J0437-4715 data(Britton 2000; van Straten et al 2001)
Caveats • Limited by S/N: • depolarization due to time/frequency variations of instrumental response • baseline estimation error/bias • no longer normally distributed error • Limited by degree of polarization: • Sinv 0 as|S|/S0 1
Matrix Template Matching (MTM) • Replace scalars with matrices • 6 new degrees of freedom • 4 times the number of constraints
Limitations • Also limited by S/N: • depolarization due to time/frequency variations of instrumental response • Calibration before integration …
Calibration Options (2007) • Measurement equation modeling(MEM; van Straten 2004) • unknown source and calibrators observed over a range of parallactic angles • Matrix template matching(MTM; van Straten 2006) • known source matched to a single (short) observation; no calibrator input
MTM Reloaded • Merge MEM and MTM methods • use template to also constrain calibrator • model time-variations and multiple observations • Derive 20 MEM solutions (~8hr each) • Integrate into standard (~150hr) • Derive 150 MEM/MTM solutions (~3.5hr) • both receiver and calibrator
Arrival Time Comparison • 234 TOAS (Nfree=217) • r.m.s reduced by 39% (predicted 33%)
Conclusions • Long-term stability of PSR J0437-4715 can be exploited to calibrate instrumental polarization • Matrix Template Matching can do better than doubling integration length
The Future • Turn MEM/MTM solutions back on PSR J0437-4715 • Quantify long-term stability of MSP polarization • Fit time- & frequency-varying receiver & calibrator model to MEM/MTM solutions