Journal
ASTRONOMY & ASTROPHYSICS
Volume 518, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/201014675
Keywords
galaxies: evoluton; galaxies: formation; galaxies: high-redshift; submillimeter: galaxies
Categories
Funding
- CSA (Canada)
- NAOC (China)
- CEA (France)
- CNES (France)
- CNRS (France)
- ASI (Italy)
- MCINN (Spain)
- Stockholm Observatory (Sweden)
- STFC (UK)
- NASA (USA)
- STFC [PP/E001173/1, ST/G002630/1, ST/H004165/1, PP/C002229/1, ST/F007019/1, ST/F002858/1, ST/H001913/1, PP/E005306/1, ST/H004157/1, ST/H001530/1] Funding Source: UKRI
- Science and Technology Facilities Council [ST/H001913/1, PP/E001173/1, ST/H004165/1, PP/E005306/1, ST/G002630/1, ST/H004157/1, PP/C002229/1, ST/F007019/1, PP/E001181/1, ST/F002858/1] Funding Source: researchfish
- UK Space Agency [ST/G003874/1, ST/H00002X/1] Funding Source: researchfish
Ask authors/readers for more resources
We have carried out two extremely deep surveys with SPIRE, one of the two cameras on Herschel, at 250 mu m, close to the peak of the far-infrared background. We have used the results to investigate the evolution of the rest-frame 250-mu m luminosity function out to z = 2. We find evidence for strong evolution out to z similar or equal to 1 but evidence for at most weak evolution beyond this redshift. Our results suggest that a significant part of the stars and metals in the universe today were formed at z <= 1.4 in spiral galaxies.
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