MAX searches for intermediate-scale anisotropy of the cosmic microwave background

P. L. Richards, A. Clapp, M. Devlin, M. Fischer, C. Hagmann, W. Holmes, A. Lange, S. Tanaka, P. Timbie, J. Gundersen, P. Meinhold, M. Lim, P. Lubin, G. Smoot

Research output: Contribution to journalArticlepeer-review

4 Scopus citations

Abstract

The balloon-borne Millimeter-Wave Anisotropy Experiment (MAX) is designed to measure the fluctuations in the cosmic microwave background (CMB) on angular scales from 0.3 to several degrees. The long term goal is to measure many pixels on the sky at a level approaching ΔT/T(CMB) = 1 × 10-6. These angular scales fill an important gap between the angular scales ≤10arcmin which are accessible from conventional radio telescopes and the angular scales ≥ 7 deg which have been measured by the COBE satellite. They are of particular importance to scientific issues such as galaxy formation, dark matter, and the Sunyaev-Zel'dovich effect.

Original languageEnglish (US)
Pages (from-to)431-438
Number of pages8
JournalInfrared Physics and Technology
Volume35
Issue number2-3
DOIs
StatePublished - Jan 1 1994
Externally publishedYes

ASJC Scopus subject areas

  • Electronic, Optical and Magnetic Materials
  • Atomic and Molecular Physics, and Optics
  • Condensed Matter Physics

Fingerprint Dive into the research topics of 'MAX searches for intermediate-scale anisotropy of the cosmic microwave background'. Together they form a unique fingerprint.

Cite this