On the suspected timing error in WMAP map-making
Boudewijn F. Roukema (Torun Centre for Astronomy)

TL;DR
This paper investigates a suspected timing error in WMAP map-making, using image sharpness metrics to reject the hypothesis of a specific timing offset, thus questioning previous assumptions about the data processing.
Contribution
It introduces a novel method of assessing timing errors in WMAP data by analyzing the sharpness of bright foreground object images across different timing offsets.
Findings
Rejects the -25.6 ms timing offset hypothesis at 4.6σ significance.
Demonstrates that the WMAP data processing likely contains a timing error affecting the quadrupole signal.
Suggests that a timing error during calibration cannot be ruled out.
Abstract
A large fraction of the previously estimated WMAP CMB quadrupole signal would be an artefact of incorrect Doppler dipole subtraction if the hypothesis of a small timing interpolation error were correct. Observations of bright foreground objects constitute part of the time-ordered-data (TOD). Scans of an object in different directions should be shifted by the would-be timing error, causing a blurring effect. Three half-years of the calibrated, filtered WMAP TOD are compiled individually for the four W band differencing assemblies (DA's), with no masking of bright objects, giving 12 maps for each timing offset. Percentiles of the temperature-fluctuation distribution in each map at HEALPix resolution N_side=2048 are used to determine the dependence of all-sky image sharpness on the timing offset. In the W band, the 99.999% percentile, i.e. the temperature fluctuation in the approx 503-rd…
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