Skip to main content

Thank you for visiting nature.com. You are using a browser version with limited support for CSS. To obtain the best experience, we recommend you use a more up to date browser (or turn off compatibility mode in Internet Explorer). In the meantime, to ensure continued support, we are displaying the site without styles and JavaScript.

  • Mission Control
  • Published:

Searching for the imprint of cosmic inflation

Nature Astronomy volume 4, page 1204 (2020)Cite this article

Subjects

The BICEP Array will bring a new level of sensitivity to observations of cosmic microwave background polarization patterns on large angular scales, says Clem Pryke on behalf of the BICEP/Keck Collaboration.

This is a preview of subscription content, access via your institution

Access options

Buy this article

  • Purchase on Springer Link
  • Instant access to full article PDF
Buy now

Prices may be subject to local taxes which are calculated during checkout

Fig. 1: The BICEP Array telescope mount at the South Pole.

Kenny Lau (University of Minnesota).

Author information

Authors and Affiliations

  1. School of Physics & Astronomy, University of Minnesota, Minneapolis, MN, USA

    Clement Pryke

Authors
  1. Clement Pryke
    View author publications

    You can also search for this author in PubMed Google Scholar

Corresponding author

Correspondence to Clement Pryke.

Rights and permissions

Reprints and permissions

About this article

Check for updates. Verify currency and authenticity via CrossMark

Cite this article

Pryke, C. Searching for the imprint of cosmic inflation. Nat Astron 4, 1204 (2020). https://doi.org/10.1038/s41550-020-01260-5

Download citation

  • Published:

  • Issue Date:

  • DOI: https://doi.org/10.1038/s41550-020-01260-5

Search

Advanced search

Quick links

Nature Briefing

Sign up for the Nature Briefing newsletter — what matters in science, free to your inbox daily.

Get the most important science stories of the day, free in your inbox. Sign up for Nature Briefing