期刊
ASTROPHYSICAL JOURNAL
卷 647, 期 2, 页码 833-839出版社
IOP PUBLISHING LTD
DOI: 10.1086/505557
关键词
cosmic microwave background
资金
- STFC [PP/D001048/1] Funding Source: UKRI
We present a measurement of the polarization- temperature angular cross power spectra, < TE > and < TB >, of the cosmic microwave background. The result is based on similar to 200 hr of data from eight polarization- sensitive bolometers operating at 145 GHz during the 2003 flight of BOOMERANG. We detect a significant < TE > correlation in the l-range between 50 and 950 with a statistical significance of > 3.5 sigma. Contamination by polarized foreground emission and systematic effects are negligible in comparison with statistical uncertainties. The spectrum is consistent with previous detections and with the ``concordance model'' that assumes adiabatic initial conditions. This is the first measurement of polarization- temperature angular cross-power spectra using bolometric detectors.
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