ARGO CMB Anisotropy Measurement Constraints on Open and Flat-A CDM
We use data from the ARGO cosmic microwave background (CMB) anisotropy experiment to constrain cosmogonies. We account for the ARGO beamwidth and calibration uncertainties, and marginalize over the offset removed from the data. Our derived amplitudes of the CMB anisotropy detected by the ARGO experi...
| Main Authors: | , , , , , |
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| Other Authors: | |
| Format: | Text |
| Language: | English |
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1505
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| Online Access: | http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.590.2282 http://trs-new.jpl.nasa.gov/dspace/bitstream/2014/20148/1/98-1010.pdf |
| Summary: | We use data from the ARGO cosmic microwave background (CMB) anisotropy experiment to constrain cosmogonies. We account for the ARGO beamwidth and calibration uncertainties, and marginalize over the offset removed from the data. Our derived amplitudes of the CMB anisotropy detected by the ARGO experiment are smaller than those derived previously. We consider open and spatially-flat-A cold dark matter cosmogonies, with clustered-mass density parameter 00 in the range 0.1-1, baryonic-mass density parameter 0 ~ in the range (0.005-0.029)h-2, and age of the universe t o in the range (10-20) Gyr. Marginalizing over all parameters but 00, the ARGO data favors an open (spatially-flat-A) model with 00 = 0.23 (O.l), amongst the models considered. At the 2 u confidence level model normalizations deduced from the ARGO data are consistent with those drawn from the UCSB South Pole 1994, MAX 4+5, White Dish, and SuZIE data sets. The ARGO open model normalizations are also consistent with those deduced from the DMR data. However, for most spatially-flat-A models the DMR normalizations are more than 2 u above the ARGO ones. Subject headings: cosmic microwave background-cosmology: observations-largescale structure of the universe |
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