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Table 1

Percentages of preference in fitting the various SFHs to the sample, based on the .

SFHs CSFR(%) DECL(%) DEL(%) RIS(%)

Free AV 3.6 50.8 23.3 22.3
Fixed AV 1.9 43.0 17.0 38.1
Fixed AV, z> 3 0 22.2 18.5 59.3

Notes. In the first line we have the initial sample with for the CSFR models (704 sources). The second line considers only the energy conserving subsample where the LIR’s are correctly matched to observation (633 sources). In the third line we show the high-z end of the previous (27 sources), where the fraction of solutions preferring the rising model has absolute majority.

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