Skip to main content
SpringerLink
Log in

Cosmology

Shedding light on dark matter

  • News & Views
  • Published:

From Nature

View current issue Submit your manuscript

This is a preview of subscription content, log in via an institution to check access.

Access this article

Log in via an institution

Price excludes VAT (USA)
Tax calculation will be finalised during checkout.

Instant access to the full article PDF.

Institutional subscriptions

Figure 1: The observed brightness of supernovae at a redshift of one, corresponding to a time of explosion halfway back to the Big Bang.
Figure 2: A type Ia supernova (SN1994D) imaged with the Hubble Space Telescope.

Peter Challis, Center for Astrophysics

References

  1. Metcalf, R. B. & Silk, J. Astrophys. J. 519, L1–L4 (1999).

    Google Scholar 

  2. Linder, E., Schneider, P. & Wagoner, R. Astrophys. J. 324, 786–793 (1988).

    Google Scholar 

  3. Rauch, K. Astrophys. J. 374, 83–90 (1991).

    Google Scholar 

  4. Holz, D. E. & Wald, R. M. Phys. Rev. D 58, 063501 (1998).

    Google Scholar 

  5. Turner, M. S. http://xxx.lanl.gov/abs/astro-ph/9901109

  6. Riess, A. G. et al. Astron. J. 116, 1009–1038 (1998).

    Google Scholar 

  7. Perlmutter, S. et al. Astrophys. J. 517, 565–586 (1999).

    Google Scholar 

  8. Glanz, J. Science 282, 2156–2157 (1998).

    Google Scholar 

Download references

Author information

Authors and Affiliations

  1. Albert Einstein Institute (Max Planck Institute for Gravitational Physics), Am Mühlenberg 5, D-14476, Golm, Germany

    Daniel E. Holz

Authors
  1. Daniel E. Holz
    View author publications

    You can also search for this author in PubMed Google Scholar

Rights and permissions

Reprints and permissions

About this article

Cite this article

Holz, D. Shedding light on dark matter. Nature 400, 819–820 (1999). https://doi.org/10.1038/23589

Download citation

  • Issue Date:

  • DOI: https://doi.org/10.1038/23589

  • Springer Nature Limited

Search

Navigation