Abstract
The determination of the star-formation history of the Universe is a key goal of modern cosmology, as it is crucial to our understanding of how galactic structures form and evolve. Observations1,2,3,4,5,6,7,8,9,10,11,12 of young stars in distant galaxies at different times in the past have indicated that the stellar birthrate peaked some eight billion years ago before declining by a factor of around ten to its present value. Here we report an analysis of the ‘fossil record’ of the current stellar populations of 96,545 nearby galaxies, from which we obtained a complete star-formation history. Our results broadly support those derived from high-redshift galaxies. We find, however, that the peak of star formation was more recent—around five billion years ago. We also show that the bigger the stellar mass of the galaxy, the earlier the stars were formed, which indicates that high- and low-mass galaxies have very different histories.
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References
Gallego, J., Zamorano, J., Aragon-Salamanca, A. & Rego, M. The current star formation rate of the local Universe. Astrophys. J. Lett. 455, 1–4 (1995)
Lilly, S. J., Le Fevre, O., Hammer, F. & Crampton, D. The Canada-France redshift survey: The luminosity density and star formation history of the Universe to z ∼ 1. Astrophys. J. Lett. 460, 1–4 (1996)
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. Lett. 462, 17–21 (1996)
Connolly, A. J., Szalay, A. S., Dickinson, M., Subbarao, M. U. & Brunner, R. J. The evolution of the global star formation history as measured from the Hubble Deep Field. Astrophys. J. Lett. 486, 11–14 (1997)
Tresse, L. & Maddox, S. J. The Hα luminosity function and star formation rate at z ∼ 0.2. Astrophys. J. 495, 691–697 (1998)
Glazebrook, K., Blake, C., Economou, F., Lilly, S. & Colless, M. Measurement of the star formation rate from Hα in field galaxies at z = 1. Mon. Not. R. Astron. Soc. 306, 843–856 (1999)
Cowie, L., Songaila, A. & Barger, A. J. Evidence for a gradual decline in the universal rest-frame ultraviolet luminosity density for z < 1. Astron. J. 117, 2656–2665 (1999)
Sullivan, M. et al. An ultraviolet-selected galaxy redshift survey—II. The physical nature of star formation in an enlarged sample. Mon. Not. R. Astron. Soc. 312, 442–464 (2000)
Scott, S. et al. The SCUBA 8-mJy survey: I—Sub-mm maps, sources and source counts. Mon. Not. R. Astron. Soc. 331, 817–838 (2002)
Chapman, S. C., Blain, A. W., Ivison, R. J. & Smail, I. R. A median redshift of 2.4 for galaxies bright at submillimetre wavelengths. Nature 422, 695–698 (2003)
Ouchi, M. et al. A census of Lyman break galaxies at z = 4 and 5 in the Subaru Deep Fields: Photometric properties. Preprint at 〈http://www.arXiv.org/astro-ph/0309657〉 (2003).
Stanway, E. R., Bunker, A. J. & McMahon, R. G. Lyman break galaxies and the star formation rate of the Universe at z ∼ 6. Mon. Not. R. Astron. Soc. 342, 439–445 (2003)
Shen, S. et al. The size distribution of galaxies in the Sloan Digital Sky Survey. Mon. Not. R. Astron. Soc. 343, 978–994 (2003)
Jimenez, R., MacDonald, J., Dunlop, J. S., Padoan, P. & Peacock, J. A. Synthetic stellar populations: single stellar populations, stellar interior models and primordial protogalaxies. Mon. Not. R. Astron. Soc. 349, 240–254 (2004)
Baldry, I. K. et al. The 2dF galaxy redshift survey: Constraints on cosmic star formation history from the cosmic spectrum. Astrophys. J. 569, 582–594 (2002)
Glazebrook, K. et al. The Sloan Digital Sky Survey: The cosmic spectrum and star formation history. Astrophys. J. 587, 55–70 (2003)
Spergel, D. N. et al. First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters. Astrophys. J. Suppl. 148, 175–194 (2003)
Gordon, K. D., Clayton, G. C., Misselt, K. A., Landolt, A. U. & Wolff, M. J. A quantitative comparison of the Small Magellanic Cloud, Large Magellanic Cloud, and Milky Way ultraviolet to near-infrared extinction curves. Astrophys. J. 594, 279–293 (2003)
Heavens, A. F., Jimenez, R. & Lahav, O. Massive lossless data compression and multiple parameter estimation from galaxy spectra. Mon. Not. R. Astron. Soc. 317, 965–972 (2000)
Reichardt, C., Jimenez, R. & Heavens, A. F. Recovering physical parameters from galaxy spectra using MOPED. Mon. Not. R. Astron. Soc. 327, 849–867 (2001)
Panter, B., Heavens, A. F. & Jimenez, R. Star formation and metallicity history of the SDSS galaxy survey: unlocking the fossil record. Mon. Not. R. Astron. Soc. 343, 1145–1154 (2003)
Dickinson, M., Papovich, C., Ferguson, H. C. & Budavri, T. The evolution of the global stellar mass density at 0 < z < 3. Astrophys. J. 587, 25–40 (2003)
Dunlop, J. S. in Deep Millimetre Surveys (eds Lowenthal, J. D. & Hughes, D. H.) 11–18 (World Scientific, Singapore, 2001)
Perez-Gonzalez, P. G. et al. Stellar populations in local star-forming galaxies—II. Recent star formation properties and stellar masses. Mon. Not. R. Astron. Soc. 338, 525–543 (2003)
Fujita, S. S. et al. The Hα luminosity function and star formation rate at z ∼ 0.24 based on Subaru deep imaging data. Astrophys. J. Lett. 586, 115–118 (2003)
Waddington, I., Dunlop, J. S., Windhorst, R. A. & Peacock, J. A. The LBDS Hercules sample of milliJansky radio sources at 1.4 GHz: II. Redshift distribution and radio luminosity function. Mon. Not. R. Astron. Soc. 328, 882–896 (2001)
Hasinger, G. The X-ray background and AGNs. in The Restless High Energy Universe (eds van den Heavel, E. P. J., in't Zand, J. J. M. & Wijers, R. A. M. J.) (Nucl. Phys. B. Suppl. Ser. in the press); preprint at 〈http://www.arXiv.org/astro-ph/0310804〉 (2003)
Calzetti, D. Reddening and star formation in starburst galaxies. Astron. J. 113, 162–184 (1997)
Bruzal, G. & Charlot, S. Spectral evolution of stellar populations using isochrone synthesis. Astrophys. J. 405, 538–553 (1993)
Acknowledgements
We are grateful to M. Pettini and M. Ouchi for helpful remarks. The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions. The participating institutions are The University of Chicago, Fermilab, the Institute for Advanced Study, the Japan Participation Group, The Johns Hopkins University, Los Alamos National Laboratory, the Max Planck Institute for Astronomy (MPIA), the Max Planck Institute for Astrophysics (MPA), New Mexico State University, the University of Pittsburgh, Princeton University, the United States Naval Observatory and the University of Washington.
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Supplementary information
Supplementary Figure 1
Recovered star formation histories fromspectra for synthesised galaxies with the global SDSS star formation rate, showing effectiveness of MOPED recovery. (JPG 19 kb)
Supplementary Figure 2
Star formation rate histories, from volume-limitedsubsamples of the SDSS, showing expected shifting of peak of star formation to higher redshift of more distant, more luminous samples. (JPG 28 kb)
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Heavens, A., Panter, B., Jimenez, R. et al. The star-formation history of the Universe from the stellar populations of nearby galaxies. Nature 428, 625–627 (2004). https://doi.org/10.1038/nature02474
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DOI: https://doi.org/10.1038/nature02474
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