%0 Journal Article %1 Liu2009 %A Liu, Hao %A Li, Ti-Pei %D 2009 %K CMB WMAP cosmology %T Improved CMB Map from WMAP Data %U http://arxiv.org/abs/0907.2731 %X The cosmic microwave background (CMB) temperature maps published by the Wilkinson Microwave Anisotropy Probe (WMAP) team are found to be inconsistent with the differential time-ordered data (TOD), from which the maps are reconstructed. The inconsistency indicates that there is a serious problem in the map making routine of the WMAP team, and it is necessary to reprocess the WMAP data. We develop a self-consistent software package of map-making and power spectrum estimation independently of the WMAP team. Our software passes a variety of tests. New CMB maps are then reconstructed, which are significantly different with the official WMAP maps. In the new maps, the inconsistency disappeared, along with the hitherto unexplained high level alignment between the CMB quadrupole and octopole components detected in released WMAP maps. An improved CMB cross-power spectrum is then derived from the new maps which better agrees with that of BOOMRANG. Two important results are hence obtained: the CMB quadrupole drops to nearly zero, and the power in multiple moment range between 200 and 675 decreases on average by about 13%, causing the best-fit cosmological parameters to change considerably, e.g., the total matter density increases from 0.26 up to 0.32 and the dark energy density decreases from 0.74 down to 0.68. These new parameters match with improved accuracy those of other independent experiments. Our results indicate that there is still room for significant revision in the cosmological model parameters.

@article{Liu2009, abstract = { The cosmic microwave background (CMB) temperature maps published by the Wilkinson Microwave Anisotropy Probe (WMAP) team are found to be inconsistent with the differential time-ordered data (TOD), from which the maps are reconstructed. The inconsistency indicates that there is a serious problem in the map making routine of the WMAP team, and it is necessary to reprocess the WMAP data. We develop a self-consistent software package of map-making and power spectrum estimation independently of the WMAP team. Our software passes a variety of tests. New CMB maps are then reconstructed, which are significantly different with the official WMAP maps. In the new maps, the inconsistency disappeared, along with the hitherto unexplained high level alignment between the CMB quadrupole and octopole components detected in released WMAP maps. An improved CMB cross-power spectrum is then derived from the new maps which better agrees with that of BOOMRANG. Two important results are hence obtained: the CMB quadrupole drops to nearly zero, and the power in multiple moment range between 200 and 675 decreases on average by about 13%, causing the best-fit cosmological parameters to change considerably, e.g., the total matter density increases from 0.26 up to 0.32 and the dark energy density decreases from 0.74 down to 0.68. These new parameters match with improved accuracy those of other independent experiments. Our results indicate that there is still room for significant revision in the cosmological model parameters. }, added-at = {2009-08-04T13:37:35.000+0200}, author = {Liu, Hao and Li, Ti-Pei}, biburl = {https://www.bibsonomy.org/bibtex/214752a2b5a518e6e4743d3c5e089f1aa/jpschaar}, description = {Improved CMB Map from WMAP Data}, interhash = {c65eb6f29c256ec67f1973bd12fe3f96}, intrahash = {14752a2b5a518e6e4743d3c5e089f1aa}, keywords = {CMB WMAP cosmology}, note = {cite arxiv:0907.2731 Comment: submitted to MNRAS}, timestamp = {2009-08-04T13:43:38.000+0200}, title = {Improved CMB Map from WMAP Data}, url = {http://arxiv.org/abs/0907.2731}, year = 2009 }