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arxiv: astro-ph/0403293 · v1 · pith:XM6HOXGXnew · submitted 2004-03-11 · 🌌 astro-ph

The Complete Star Formation History of the Universe

classification 🌌 astro-ph
keywords formationhistoryuniversegalaxiesstarstellaryearsaround
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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 structure in the Universe forms and evolves. A picture has built up over recent years, piece-by-piece, by observing young stars in distant galaxies at different times in the past. These studies indicated that the stellar birthrate peaked some 8 billion years ago, and then declined by a factor of around ten to its present value. Here we report on a new study which obtains the complete star formation history by analysing the fossil record of the stellar populations of 96545 nearby galaxies. Broadly, our results support those derived from high-redshift galaxies elsewhere in the Universe. We find, however, that the peak of star formation was more recent - around 5 billion years ago. Our study also shows that the bigger the stellar mass of the galaxy, the earlier the stars were formed. This striking result indicates a very different formation history for high- and low-mass formation.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12

    astro-ph.GA 2026-05 unverdicted novelty 5.0

    Stacking of 850-micron data reveals SFR increasing with redshift and declining from irregular to spheroidal galaxies at 2<z<4.5, with a chemical evolution model reproducing the dust-to-stellar mass ratio rise to z~8.

  2. COSMOS-Web: Star formation along the early Hubble sequence and the evolution of dust over the redshift range 0<z<12

    astro-ph.GA 2026-05 unverdicted novelty 5.0

    Stacking analysis shows mean SFR in massive galaxies at 2<z<4.5 declines along the Hubble sequence from ~280 M⊙/yr in irregulars to ~80 M⊙/yr in spheroids, with a simple chemical evolution model explaining the rise in...