Using White Dish CMB Anisotropy Data to Probe Open and Flat-Lambda CDM Cosmogonies

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We use data from the White Dish experiment to set limits on cosmic microwave background radiation anisotropies in open and spatially-flat-Lambda cold dark matter cosmogonies. We account for the White Dish calibration uncertainty, and marginalize over the offset and gradient removed from the data. Our 2-sigma upper limits are larger than those derived previously. These upper limits are consistent with those derived from the $COBE$-DMR data for all models tested.
17 pages of latex. Uses aasms4.sty. 4 figures included. Submitted to ApJS

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/198131

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/9710270
 http://arxiv.org/abs/astro-ph/9710270
 Astrophys.J.505:8-11,1998
 doi:10.1086/306139

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arXiv