WMAP Q - 9yr survey collection Virtual Observatory Resource

Authors

1. Fernique P.

Published by

CDS

Abstract

The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The Q-band is centered at 7.3 mm (41 GHz), its beam size is 0.51 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."

Keywords

1. Sky survey
2. Radio astronomy

See also HTML

https://alasky.cds.unistra.fr/WMAP9yr/WMAPQ9yr

IVOA Identifier IVOID

ivo://CDS/P/WMAP/Q/9yr

Access

Unknown endpoint

Capability for unknown standard ivo://ivoa.net/std/hips#hips-1.0. The VO Registry may have more details; look for IVOID ivo://CDS/P/WMAP/Q/9yr.