QUaD

Images Courtesy of the Stanford University Church Group

Overview

QUaD was a bolometric array receiver used to search for polarization in the CMB. The spatial distribution of polarization contains important information about cosmological parameters and about the origin of temperature anisotropies in the CMB. Although the signal is tiny (1-10% of the temperature fluctuations) the scientific rewards are large. QUaD observed a ∼100 square degree area of sky, centered on RA 5.5h, Dec −50°.

The heart of QUaD was a 31-element focal plane shown schematically below. There were 31 corrugated feed horns, each feeding a polarization-sensitive bolometer (PSB) pair manufactured at the Jet Propulsion Laboratory. Each device comprised a linear mesh of metalized silicon-nitride that absorbs only one direction of linear polarization. The temperature change in the bolometer was then detected by an NTD (neutron transmutation-doped) germanium thermistor (the dark rectangle at the edge of the web). A PSB pair measures the intensity of the radiation in orthogonal linear polarizations as the telescope scanned across the sky. These signals were then processed into a map of the polarization pattern on the sky.

QUaD's name means: QUEST (Q and U Extragalactic Sub-mm Telescope) at DASI (Degree Angular Scale Interferometer)

Experiment Information:

  • Experiment Date Range in Years: 2005 - 2010
  • Frequency (GHz): 100, 150
  • l-min: ~200
  • l-max: 2000

The QUaD website can be viewed HERE.

A service of the HEASARC and of the Astrophysics Science Division at NASA/GSFC

HEASARC Director: Dr. Andrew F. Ptak

LAMBDA Director: Dr. Thomas M. Essinger-Hileman

NASA Official: Dr. Thomas M. Essinger-Hileman

Web Curator: Mr. Michael R. Greason