WMAP K - 9yr survey collection Virtual Observatory Resource

Authors
  1. Fernique P.
  2. Published by
    CDS
Abstract

The WMAP (Wilkinson Microwave Anisotropy Probe) mission is designed to determine the geometry, content, and evolution of the universe.The K-band is centered at 13 mm (23 GHz), its beam size is 0.88 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/WMAPK9yr
IVOA Identifier IVOID
ivo://CDS/P/WMAP/K/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/K/9yr.

History

2014-11-25T18:10:00Z
Resource record created
2014-11-25T18:10:00Z
Created
2019-05-05T07:50:00Z
Updated

Contact

Name
CDS Helpdesk
E-Mail
cds-question@unistra.fr