WMAP W - 9yr survey collection

The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The W-band is centered at 3.2 mm (94 GHz), its beam size is 0.22 deg (square-root of the beam solid angle). Original acknowledgement for data: We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center."

Identifier
Source https://dc.g-vo.org/rr/q/lp/custom/CDS/P/WMAP/W/9yr
Related Identifier https://alasky.cds.unistra.fr/WMAP9yr/WMAPW9yr
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS/P/WMAP/W/9yr
Provenance
Creator Fernique P.
Publisher CDS
Publication Year 2014
Rights This HiPS is distributed under ODbL license by Unistra/CNRS; https://cds.unistra.fr/aladin-org/licences_aladin.html
OpenAccess true
Contact CDS Helpdesk <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Natural Sciences; Observational Astronomy; Physics
Temporal Coverage 2001-08-10T00:00:00Z 2010-08-19T00:00:00Z