- Abstract:
-
We measure the stellar mass function (SMF) and stellar mass density of galaxies in the COSMOS field up to z ~ 6. We select them in the near-IR bands of the COSMOS2015 catalogue, which includes ultra-deep photometry from UltraVISTA-DR2, SPLASH, and Subaru/Hyper Suprime-Cam. At z> 2.5 we use new precise photometric redshifts with error σ z = 0.03(1 + z) and an outlier fraction of 12%, estimated by means of the unique spectroscopic sample of COSMOS (~100 000 spectroscopic measurements in tota...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's Version
- Files:
-
-
(pdf, 5.0MB)
-
- Publisher copy:
- 10.1051/0004-6361/201730419
-
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- Publisher:
- EDP Sciences Publisher's website
- Journal:
- Astronomy and Astrophysics Journal website
- Volume:
- 605
- Pages:
- Article: A70
- Publication date:
- 2017-09-12
- Acceptance date:
- 2017-05-17
- DOI:
- EISSN:
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1432-0746
- ISSN:
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0004-6361
- Pubs id:
-
pubs:731360
- URN:
-
uri:69d0fbb9-f82e-4268-8755-62581ebac98b
- UUID:
-
uuid:69d0fbb9-f82e-4268-8755-62581ebac98b
- Local pid:
- pubs:731360
- Keywords:
- Copyright holder:
- ESO
- Copyright date:
- 2017
- Notes:
- © ESO 2017. Article published by EDP Sciences.
Journal article
The COSMOS2015 galaxy stellar mass function
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