PLANCK R2 nominal frequency LFI map 30 Ghz survey collection Virtual Observatory Resource

Authors
  1. CDS
  2. Published by
    CDS
Abstract

The Planck mission will collect and characterise radiation from the Cosmic Microwave Background (CMB) using sensitive radio receivers operating at extremely low temperatures. These receivers will determine the black body equivalent temperature of the background radiation and will be capable of distinguishing temperature variations of about one microkelvin. These measurements will be used to produce the best ever maps of anisotropies in the CMB radiation field.

Keywords
  1. Sky survey
  2. Radio astronomy
  3. Cosmic microwave background radiation
See also HTML
https://alasky.cds.unistra.fr/PLANCK/R2/LFI_SkyMap_030_1024_R2.01
IVOA Identifier IVOID
ivo://CDS/P/PLANCK/R2/LFI030

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/PLANCK/R2/LFI030.

History

2015-02-05T16:40:00Z
Resource record created
2015-02-05T16:40:00Z
Created
2019-05-05T06:51:00Z
Updated

Contact

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