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Cited by 220

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The evolution of stellar mass and the implied star formation history

Open access
Wilkins, Stephen M., Trentham, Neil, Hopkins, Andrew M.·2008·Monthly Notices of the Royal Astronomical Society

Abstract

We present a compilation of measurements of the stellar mass density as a function of redshift. Using this stellar mass history we obtain a star formation history and compare it to the instantaneous star formation history. For z < 0.7 there is good agreement between the two star formation histories. At higher redshifts the instantaneous indicators suggest star formation rates larger than that implied by the evolution of the stellar mass density. This discrepancy peaks at z= 3 where instantaneous indicators suggest a star formation rate around 0.6 dex higher than those of the best fit to the stellar mass history. We discuss a variety of explanations for this inconsistency, such as inaccurate dust extinction corrections, incorrect measurements of stellar masses and a possible evolution of the stellar initial mass function.

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Crossref · 10.1111/j.1365-2966.2008.12885.x

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Metadata

Authors
Wilkins, S. M., Trentham, N., & Hopkins, A. M.
Venue
Monthly Notices of the Royal Astronomical Society
Published
2008-04
Volume
385
Issue
2
Pages
687-694
ISSN
  • 0035-8711 (ISSN-L)
  • 1365-2966
OpenAlex
W2030098530
Cited by
220
References
1
FWCI
17.49
Type
journal article
Language
en
Open access
green

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CoChat. (2026). Citation check: The evolution of stellar mass and the implied star formation history. https://app.cochat.ai/papers/10.1111/j.1365-2966.2008.12885.x
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Wilkins, S. M., Trentham, N., & Hopkins, A. M. (2008). The evolution of stellar mass and the implied star formation history. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1111/j.1365-2966.2008.12885.x

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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).

Semantic Scholar’s data is described in: Kinney, R., et al. (2023). The Semantic Scholar Open Data Platform. arXiv:2301.10140.