Article record

Further constraints on the evolution of Ks-selected galaxies in the GOODS/CDFS field

Caputi K. I., McLure R. J., Dunlop J. S., Cirasuolo M., Schael A. M. | 2006

arXiv | ADS | Publisher page

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Figure 6 (rest-frame Ks luminosity functions)

Caputi+06_Fig6_Ks_original.csv | 25 rows | 2341 bytes | CSV

Digitized empty 1/Vmax symbols and error bars from Figure 6, all four panels (25 points). Columns: M_Ks_Vega = rest-frame absolute Ks magnitude (Vega); log10_Phi_Mpc-3_mag-1 = log10 number density per magnitude; upper_logPhi_error and lower_logPhi_error = positive asymmetric error amplitudes in log10 Phi; z = panel central redshift; z_min, z_max = published redshift-bin bounds; lower_endpoint_is_floor = 1 only when the lower endpoint was assigned a plotting floor. Redshift intervals: [0.75,1.25], [1.25,1.75], [1.75,2.25], [2.00,3.00], centred at z=1,1.5,2,2.5. The last two bins overlap as in the paper. Original magnitude and per-mag density units retained; no Vega-to-AB, per-dex, or cosmology rescaling applied. H0=70 km/s/Mpc, Omega_m=0.3, Omega_Lambda=0.7. Published errors are the maximum of Poisson and cosmic-variance errors. For the brightest z=2 point, the lower endpoint is set to log10 Phi=-9 as a plotting floor, not a measured bound or an observational upper/lower limit. Fitted curves and literature comparison points excluded.

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