pith. sign in

arxiv: 0912.0621 · v1 · pith:43RO6WRNnew · submitted 2009-12-03 · 🌌 astro-ph.CO

High-frequency radio polarization measurements of WMAP point sources

classification 🌌 astro-ph.CO
keywords measurementssourcespolarizationwmapradiobackgroundcalibrationcatalogue
0
0 comments X p. Extension
pith:43RO6WRN Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{43RO6WRN}

Prints a linked pith:43RO6WRN badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original abstract

We present polarization measurements at 8.4, 22, and 43 GHz made with the VLA of a complete sample of extragalactic sources stronger than 1 Jy in the 5-year WMAP catalogue and with declinations north of -34 degrees. The observations were motivated by the need to know the polarization properties of radio sources at frequencies of tens of GHz in order to subtract polarized foregrounds for future sensitive Cosmic Microwave Background (CMB) experiments. The total intensity and polarization measurements are generally consistent with comparable VLA calibration measurements for less-variable sources, and within a similar range to WMAP fluxes for unresolved sources. A further paper will present correlations between measured parameters and derive implications for CMB measurements.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.