Matches in SemOpenAlex for { <https://semopenalex.org/work/W2952708358> ?p ?o ?g. }
- W2952708358 abstract "Context. The contribution of the merging process to the early phase of galaxy assembly at z > 1 and, in particular, to the build-up of the red sequence, still needs to be accurately assessed. Aims. We aim to measure the major merger rate of star-forming galaxies at 0.9 < z < 1.8, using close pairs identified from integral field spectroscopy (IFS). Methods. We use the velocity field maps obtained with SINFONI/VLT on the MASSIV sample, selected from the star-forming population in the VVDS. We identify physical pairs of galaxies from the measurement of the relative velocity and the projected separation (rp) of the galaxies in the pair. Using the well constrained selection function of the MASSIV sample, we derive at a mean redshift up to z = 1.54 the gas-rich major merger fraction (luminosity ratio μ = L2/L1 ≥ 1/4), and the gas-rich major merger rate using merger time scales from cosmological simulations." @default.
- W2952708358 created "2019-06-27" @default.
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- W2952708358 date "2013-05-01" @default.
- W2952708358 modified "2023-10-16" @default.
- W2952708358 title "MASSIV: Mass Assembly Survey with SINFONI in VVDS , V. The major merger rate of star-forming galaxies at 0.9 < z < 1.8 from IFS-based close pairs" @default.
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