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Define tomographic bins and n(z) via a SOM. Owner: Klara.
Plan (from the Bochum telecon with Angus Wright, 21 Sep; 22 Sep call notes): follow KiDS-Legacy. One SOM (one magnitude + four colours) trained on UNIONS photometry in W3, with the spectroscopic samples there. Gold weighting rather than a gold cut. Constant-shear image sims. Clustering redshifts (DESI overlap) cross-check the mean. The two UNIONS z filters are mapped onto one system. If W3 turns out unrepresentative of the survey, fall back to two SOMs with a transfer function (DES Y6). Pipeline: CosmoPipe. Next: a first n(z) on current data.
we currently can't file issues on the UNIONS PhotoPipe so this was the best i could do for now. see this Slack thread for more. but i agree this is CosmoPipe/PhotoPipe territory
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sachaguer commentedon Jul 16, 2026
It should be checked whether sp_validation is the good place for this or if it will be produced within CosmoPipe.
cailmdaley commentedon Jul 16, 2026
we currently can't file issues on the UNIONS PhotoPipe so this was the best i could do for now. see this Slack thread for more. but i agree this is CosmoPipe/PhotoPipe territory