Matches in SemOpenAlex for { <https://semopenalex.org/work/W3100976744> ?p ?o ?g. }
- W3100976744 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 total, more than one thousand having robust z_(spec)> 2.5). The increased exposure time in the DR2, along with our panchromatic detection strategy, allow us to improve the completeness at high z with respect to previous UltraVISTA catalogues (e.g. our sample is >75% complete at 10^(10)M⊙ and z = 5). We also identify passive galaxies through a robust colour–colour selection, extending their SMF estimate up to z = 4. Our work provides a comprehensive view of galaxy-stellar-mass assembly between z = 0.1 and 6, for the first time using consistent estimates across the entire redshift range. We fit these measurements with a Schechter function, correcting for Eddington bias. We compare the SMF fit with the halo mass function predicted from ΛCDM simulations, finding that at z > 3 both functions decline with a similar slope in thehigh-mass end. This feature could be explained assuming that mechanisms quenching star formation in massive haloes become less effective at high redshifts; however further work needs to be done to confirm this scenario. Concerning the SMF low-mass end, it shows a progressive steepening as it moves towards higher redshifts, with α decreasing from -1.47^(+0.02)_(-0.02) at z ≃ 0.1 to -2.11^(+0.30)_(-0.13) at z ≃ 5. This slope depends on the characterisation of the observational uncertainties, which is crucial to properly remove the Eddington bias. We show that there is currently no consensus on the method to quantify such errors: different error models result in different best-fit Schechter parameters." @default.
- W3100976744 created "2020-11-23" @default.
- W3100976744 creator A5011211151 @default.
- W3100976744 creator A5024335460 @default.
- W3100976744 creator A5031401057 @default.
- W3100976744 creator A5031967114 @default.
- W3100976744 creator A5035438463 @default.
- W3100976744 creator A5039049327 @default.
- W3100976744 creator A5046172456 @default.
- W3100976744 creator A5046824037 @default.
- W3100976744 creator A5046833250 @default.
- W3100976744 creator A5046987116 @default.
- W3100976744 creator A5051323119 @default.
- W3100976744 creator A5052031270 @default.
- W3100976744 creator A5053165153 @default.
- W3100976744 creator A5054190787 @default.
- W3100976744 creator A5057229420 @default.
- W3100976744 creator A5058017131 @default.
- W3100976744 creator A5061314579 @default.
- W3100976744 creator A5063568570 @default.
- W3100976744 creator A5072059052 @default.
- W3100976744 creator A5072816933 @default.
- W3100976744 creator A5079315006 @default.
- W3100976744 creator A5081052936 @default.
- W3100976744 creator A5081204604 @default.
- W3100976744 creator A5089805698 @default.
- W3100976744 date "2017-01-01" @default.
- W3100976744 modified "2023-10-16" @default.
- W3100976744 title "The COSMOS2015 galaxy stellar mass function - Thirteen billion years of stellar mass assembly in ten snapshots" @default.
- W3100976744 cites W1494146418 @default.
- W3100976744 cites W1573578139 @default.
- W3100976744 cites W1603779598 @default.
- W3100976744 cites W1764480375 @default.
- W3100976744 cites W1766563480 @default.
- W3100976744 cites W1826791147 @default.
- W3100976744 cites W1848338669 @default.
- W3100976744 cites W1869477344 @default.
- W3100976744 cites W1882938068 @default.
- W3100976744 cites W1894812898 @default.
- W3100976744 cites W1909359706 @default.
- W3100976744 cites W1911215022 @default.
- W3100976744 cites W1911876284 @default.
- W3100976744 cites W1912798299 @default.
- W3100976744 cites W1917783267 @default.
- W3100976744 cites W1921256341 @default.
- W3100976744 cites W1929287038 @default.
- W3100976744 cites W1964280853 @default.
- W3100976744 cites W1964385238 @default.
- W3100976744 cites W1967532042 @default.
- W3100976744 cites W1969388479 @default.
- W3100976744 cites W1969717379 @default.
- W3100976744 cites W1970196846 @default.
- W3100976744 cites W1973977373 @default.
- W3100976744 cites W1974394716 @default.
- W3100976744 cites W1977609574 @default.
- W3100976744 cites W1980454973 @default.
- W3100976744 cites W1981635330 @default.
- W3100976744 cites W1982533357 @default.
- W3100976744 cites W1985500852 @default.
- W3100976744 cites W1985952407 @default.
- W3100976744 cites W1990491187 @default.
- W3100976744 cites W1992834467 @default.
- W3100976744 cites W1994671833 @default.
- W3100976744 cites W1994915027 @default.
- W3100976744 cites W1995942510 @default.
- W3100976744 cites W1996926090 @default.
- W3100976744 cites W1997151814 @default.
- W3100976744 cites W2000030959 @default.
- W3100976744 cites W2000840256 @default.
- W3100976744 cites W2008991538 @default.
- W3100976744 cites W2012056991 @default.
- W3100976744 cites W2012886609 @default.
- W3100976744 cites W2013355735 @default.
- W3100976744 cites W2015295900 @default.
- W3100976744 cites W2016966639 @default.
- W3100976744 cites W2018388366 @default.
- W3100976744 cites W2019562528 @default.
- W3100976744 cites W2019814288 @default.
- W3100976744 cites W2024175772 @default.
- W3100976744 cites W2024297548 @default.
- W3100976744 cites W2025105301 @default.
- W3100976744 cites W2027297109 @default.
- W3100976744 cites W2029842890 @default.
- W3100976744 cites W2034241894 @default.
- W3100976744 cites W2036920580 @default.
- W3100976744 cites W2037526471 @default.
- W3100976744 cites W2037878575 @default.
- W3100976744 cites W2038153124 @default.
- W3100976744 cites W2040520625 @default.
- W3100976744 cites W2042369320 @default.
- W3100976744 cites W2046315396 @default.
- W3100976744 cites W2048828609 @default.
- W3100976744 cites W2051907414 @default.
- W3100976744 cites W2053265856 @default.
- W3100976744 cites W2057672934 @default.
- W3100976744 cites W2057756810 @default.
- W3100976744 cites W2061255732 @default.
- W3100976744 cites W2062298152 @default.
- W3100976744 cites W2067649418 @default.
- W3100976744 cites W2067773898 @default.