Galactic Foregrounds in Owens Valley Radio Observatory and UCSB South Pole 1994 Cosmic Microwave Background Anisotropy Data
dc.contributor.author | Mukherjee, P. | en |
dc.contributor.author | Dennison, B. | en |
dc.contributor.author | Ratra, B. | en |
dc.contributor.author | Simonetti, John H. | en |
dc.contributor.author | Ganga, K. | en |
dc.contributor.author | Hamilton, J. C. | en |
dc.contributor.department | Institute for Particle, Nuclear and Astronomical Sciences (IPNAS) | en |
dc.contributor.department | Physics | en |
dc.date.accessed | 2014-02-28 | en |
dc.date.accessioned | 2014-03-10T13:18:51Z | en |
dc.date.available | 2014-03-10T13:18:51Z | en |
dc.date.issued | 2002-11 | en |
dc.description.abstract | We study Galactic emission foreground contamination of the Owens Valley Radio Observatory and UCSB South Pole 1994 cosmic microwave background anisotropy data by cross-correlating with templates of infrared dust emission and new high-resolution Virginia Tech Spectral Line Survey (VTSS) and Southern Halpha Sky Survey Atlas (SHASSA) Halpha data. Halpha data provide rough upper limits on the level of free-free emission in the data sets. The cross-correlation analysis does not contradict a two-component foreground emission hypothesis, with the two dust-correlated components being free-free emission and spinning-dust emission. | en |
dc.description.sponsorship | NSF AST 98-00476, AST 00-98487, AST 98-75031 | en |
dc.description.sponsorship | Horton Foundation Grant | en |
dc.identifier.citation | Pia Mukherjee et al. 2002 ApJ 579 83 doi:10.1086/342702 | en |
dc.identifier.doi | https://doi.org/10.1086/342702 | en |
dc.identifier.issn | 0004-637X | en |
dc.identifier.uri | http://hdl.handle.net/10919/25853 | en |
dc.identifier.url | http://iopscience.iop.org/0004-637X/579/1/83 | en |
dc.language.iso | en_US | en |
dc.publisher | IOP PUBLISHING LTD | en |
dc.rights | In Copyright | en |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | en |
dc.subject | cosmic microwave background | en |
dc.subject | cosmology : observations | en |
dc.subject | diffuse | en |
dc.subject | radiation | en |
dc.subject | dust, extinction | en |
dc.subject | dark-matter cosmogonies | en |
dc.subject | spinning dust grains | en |
dc.subject | h-alpha emission | en |
dc.subject | measurement constraints | en |
dc.subject | sky maps | en |
dc.subject | infrared cirrus | en |
dc.subject | tenerife data | en |
dc.subject | radiation | en |
dc.subject | scales | en |
dc.subject | power | en |
dc.title | Galactic Foregrounds in Owens Valley Radio Observatory and UCSB South Pole 1994 Cosmic Microwave Background Anisotropy Data | en |
dc.title.serial | Astrophysical Journal | en |
dc.type | Article - Refereed | en |
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