Abstract
We present an internal consistency test of South Pole Telescope (SPT) measurements of the cosmic microwave background (CMB) temperature anisotropy using three-band data from the SPT-SZ survey. These measurements are made from observations of similar to 2500 deg(2) of sky in three frequency bands centered at 95, 150, and 220 GHz. We combine the information from these three bands into six semi-independent estimates of the CMB power spectrum (three single-frequency power spectra and three cross-frequency spectra) over the multipole range 650 < l < 3000. We subtract an estimate of foreground power from each power spectrum and evaluate the consistency among the resulting CMB-only spectra. We determine that the six foreground-cleaned power spectra are consistent with the null hypothesis, in which the six cleaned spectra contain only CMB power and noise. A fit of the data to this model results in a chi(2) value of 236.3 for 235 degrees of freedom, and the probability to exceed this chi(2) value is 46%.
Dokumententyp: | Zeitschriftenartikel |
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Fakultät: | Physik |
Themengebiete: | 500 Naturwissenschaften und Mathematik > 530 Physik |
ISSN: | 1475-7516 |
Sprache: | Englisch |
Dokumenten ID: | 82766 |
Datum der Veröffentlichung auf Open Access LMU: | 15. Dez. 2021, 15:03 |
Letzte Änderungen: | 15. Dez. 2021, 15:03 |