Abstract
The first 900 million years (Myr) to redshift z ≈ 6 (the first seven per cent of the age of the Universe) remains largely unexplored for the formation of galaxies. Large samples of galaxies have been found at z ≈ 6 (refs 1–4) but detections at earlier times are uncertain and unreliable. It is not at all clear how galaxies built up from the first stars when the Universe was about 300 Myr old (z ≈ 12–15) to z ≈ 6, just 600 Myr later. Here we report the results of a search for galaxies at z ≈ 7–8, about 700 Myr after the Big Bang, using the deepest near-infrared and optical images ever taken. Under conservative selection criteria we find only one candidate galaxy at z ≈ 7–8, where ten would be expected if there were no evolution in the galaxy population between z ≈ 7–8 and z ≈ 6. Using less conservative criteria, there are four candidates, where 17 would be expected with no evolution. This demonstrates that very luminous galaxies are quite rare 700 Myr after the Big Bang. The simplest explanation is that the Universe is just too young to have built up many luminous galaxies at z ≈ 7–8 by the hierarchical merging of small galaxies.
This is a preview of subscription content, access via your institution
Relevant articles
Open Access articles citing this article.
-
The numerical frontier of the high-redshift Universe
Computational Astrophysics and Cosmology Open Access 28 March 2015
Access options
Subscribe to this journal
Receive 51 print issues and online access
$199.00 per year
only $3.90 per issue
Rent or buy this article
Get just this article for as long as you need it
$39.95
Prices may be subject to local taxes which are calculated during checkout



References
Bouwens, R. J., Illingworth, G. D., Blakeslee, J. P. & Franx, M. Galaxies at z∼6: The UV luminosity function and luminosity density from 506 UDF, UDF-Ps, and GOODS i-dropouts. Astrophys. J. (in the press); preprint at http://www.arXiv.org/astro-ph/0509641 (2005)
Dickinson, M. et al. Color-selected galaxies at z∼6 in the great observatories origins deep survey. Astrophys. J. 600, 99–102 (2004)
Yan, H. J. & Windhorst, R. A. Candidates of z∼5.5–7 galaxies in the Hubble Space Telescope Ultra Deep Field. Astrophys. J. 612, 93–96 (2004)
Bunker, A. J., Stanway, E. R., Ellis, R. S. & McMahon, R. G. The star formation rate of the Universe at z∼6 from the Hubble Ultra Deep Field. Mon. Not. R. Astron. Soc. 355, 374–384 (2004)
Steidel, C. C., Giavalisco, M., Pettini, M., Dickinson, M. & Adelberger, K. L. Spectroscopic confirmation of a population of normal star-forming galaxies at redshifts Z > 3. Astrophys. J. 462, 17–20 (1996)
Madau, P. Radiative transfer in a clumpy universe: The colors of high-redshift galaxies. Astrophys. J. 441, 18–27 (1995)
Becker, R. H. et al. Evidence for reionization at z∼6: detection of a Gunn-Peterson trough in a z = 6.28 quasar. Astron. J. 122, 2850–2857 (2001)
Fan, X. et al. Evolution of the ionizing background and the epoch of reionization from the spectra of z∼6 quasars. Astronom. J. 123, 1247–1257 (2002)
Skinner, C. J. et al. On-orbit properties of the NICMOS detectors on HST. Proc. SPIE 3354, 2–13 (1998)
Thompson, R. I. et al. The Near-Infrared Camera and Multi-Object Spectrometer Ultra Deep Field: observations, data reduction, and galaxy photometry. Astron. J. 130, 1–12 (2005)
Bouwens, R. J. et al. Galaxies at z∼7–8: z850-dropouts in the Hubble Ultra Deep Field. Astrophys. J. 616, 79–82 (2004)
Richard, J., Pello, R., Schaerer, D., Le Borgne, J.-F. & Kneib, J.-P. Constraining the population of 6 < z < 10 star-forming galaxies with deep near-IR images of lensing clusters. Astron. Astrophys. (in the press); preprint at http://www.arXiv.org/astro-ph/0606134 (2006)
Giavalisco, M. et al. The Great Observatories Origins Deep Survey: initial results from optical and near-infrared imaging. Astrophys. J. 600, 99–102 (2004)
Thompson, R. I. et al. Near-Infrared Camera and Multi-Object Spectroscopic observations of the Hubble Deep Field: observations, data reduction, and galaxy photometry. Astron. J. 117, 17–39 (1999)
Dickinson, M. A. Complete NICMOS map of the Hubble Deep Field North. AIP Conf. Proc. 470, 122–132 (1999)
Blakeslee, J. P., Anderson, K. R., Meurer, G. R., Benítez, N. & Magee, D. An automatic image reduction pipeline for the Advanced Camera for Surveys. in Astronomical Data Analysis Software and Systems XII (eds Payne, H. E., Jedrzejewski, R. I. & Hook, R. N.) 257–260 (ASP Conf. Ser. 295, Astronomical Society of the Pacific, 2003)
Bertin, E. & Arnouts, S. SExtractor: software for source extraction. Astron. Astrophys. 117 (Suppl.), 393–404 (1996)
Bouwens, R. J., Broadhurst, T. J. & Silk, J. Cloning Hubble Deep Fields. I. A model-independent measurement of galaxy evolution. Astrophys. J. 506, 557–578 (1998)
Bouwens, R. J., Broadhurst, T. J. & Illingworth, G. D. Cloning dropouts: implications for galaxy evolution at high redshift. Astrophys. J. 593, 640–660 (2003)
Mo, H. J. & White, S. D. M. An analytic model for the spatial clustering of dark matter haloes. Mon. Not. R. Astron. Soc. 282, 347–361 (1996)
Somerville, R. S. et al. Cosmic variance in the Great Observatories Origins Deep Survey. Astrophys. J. 600, 171–174 (2004)
Giavalisco, M. et al. The rest-frame ultraviolet luminosity density of star-forming galaxies at redshifts z > 3.5. Astrophys. J. 600, 103–106 (2004)
Eyles, L. et al. Spitzer imaging of i'-drop galaxies: old stars at z∼6. Mon. Not. R. Astron. Soc. 364, 443–454 (2005)
Yan, H. et al. Rest-frame ultraviolet-to-optical properties of galaxies at z∼6 and 5 in the Hubble Ultra Deep Field: from Hubble to Spitzer. Astrophys. J. 634, 109–127 (2005)
Dow-Hygelund, C. C. et al. UV continuum spectroscopy of a 6L* z = 5.5 galaxy. Astrophys. J. 630, 137–140 (2005)
Yan, H. J. et al. The stellar masses and star formation histories of galaxies at z∼6: constraints from Spitzer observations in the Great Observatories Origins Deep Survey. Astrophys. J. (in the press); preprint at http://www.arXiv.org/astro-ph/0604554 (2006)
Stark, D., Bunker, A. J., Ellis, R. S., Eyles, L. P. & Lacy, M. A new measurement of the stellar mass density at z∼5: implications for the sources of cosmic reionization. Astrophys. J. (submitted); preprint at http://www.arXiv.org/astro-ph/0604250 (2006)
Spergel, D. et al. Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology. Astrophys. J. (submitted); preprint at http://www.arXiv.org/astro-ph/0603449 (2006)
Steidel, C. C., Adelberger, K. L., Giavalisco, M., Dickinson, M. & Pettini, M. Lyman-break galaxies at z > ∼4 and the evolution of the ultraviolet luminosity density at high redshift. Astrophys. J. 519, 1–17 (1999)
Schiminovich, D. et al. The GALEX-VVDS measurement of the evolution of the far-ultraviolet luminosity density and the cosmic star formation rate. Astrophys. J. 619, 47–50 (2005)
Labbé, I., Bouwens, R. J., Illingworth, G. D. & Franx, M. Confirmation of z-dropout galaxies in the HUDF with Spitzer IRAC imaging: stellar masses and ages. Astrophys. J. (in the press); preprint at http://www.arXiv.org/astro-ph/0608444 (2006)
Madau, P., Pozzetti, L. & Dickinson, M. The star formation history of field galaxies. Astrophys. J. 498, 106–116 (1998)
Stanway, E. R., McMahon, R. G. & Bunker, A. J. Near-infrared properties of i-drop galaxies in the Hubble Ultra Deep Field. Mon. Not. R. Astron. Soc. 359, 1184–1192 (2005)
Acknowledgements
We are grateful to L. Bergeron, S. Kassin, D. Magee, M. Stiavelli, R. Thompson and A. Zirm for their help in reducing the NICMOS data, to M. Franx for critical reading of this manuscript, to S. Malhotra for making the NICMOS parallels to her PEARS program public early, and to I. Labbe for assistance in interpreting the IRAC data.
Author information
Authors and Affiliations
Corresponding author
Ethics declarations
Competing interests
Reprints and permissions information is available at www.nature.com/reprints. The authors declare no competing financial interests.
Supplementary information
Supplementary Notes
This file contains Supplementary Methods, Supplementary Figures 1–2, Supplementary Tables 1–2 and Supplementary Notes. (PDF 473 kb)
Rights and permissions
About this article
Cite this article
Bouwens, R., Illingworth, G. Rapid evolution of the most luminous galaxies during the first 900 million years. Nature 443, 189–192 (2006). https://doi.org/10.1038/nature05156
Received:
Accepted:
Issue Date:
DOI: https://doi.org/10.1038/nature05156
This article is cited by
-
The numerical frontier of the high-redshift Universe
Computational Astrophysics and Cosmology (2015)
-
The Role of Energy Conservation and Vacuum Energy in the Evolution of the Universe
Foundations of Science (2010)
-
Astrophysics in 2006
Space Science Reviews (2007)
-
Dawn after the dark age
Nature (2006)
Comments
By submitting a comment you agree to abide by our Terms and Community Guidelines. If you find something abusive or that does not comply with our terms or guidelines please flag it as inappropriate.