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Major merging history in CANDELS I Evolution of the incidence of massive galaxy–galaxy pairs from z = 3 to z ∼ 0

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Figure

Figure 2.Stellar mass distributions for galaxies in the SDSSgroup catalog (Yang et al
Figure 3. Photometric redshift uncertainties (σz) as a function of zbest for galaxies with Mstellar ≥ 5 × 109M⊙ in each CANDELS field.The σz values are the 1σ photometric redshift errors from the optimized P(z) distributions originally derived by S
Figure 4. The number of massive galaxies hosting a major com-with no spectroscopic redshift information (panion in projected pairs as a function of projected separationfrom the SDSS: total (N′proj; bold line), the subset of galaxiesN′proj,nospec; dashedlin
Table 2. Detailed breakdown of variables involved in estimating thenumber of massive galaxies hosting a major projected companion (are shown in parenthesis; (5) number of massive galaxies with reliable(1) name of the CANDELS field; (2) the CANDELS teamproxi
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