Abstract.
We revisit our recent results concerning comparisons of magnitude and photometric redshift data from the Hubble Deep Fields to statistical predictions from galaxy population models. More rigorous modeling techniques are applied but our earlier conclusion that, of the various models considered, an Einstein - de Sitter universe with simple passive evolution reproduced the data best.
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Bristow, P., Phillipps, S. Modeling Faint Morphological Number Counts. In: Cristiani, S., Renzini, A., Williams, R.E. (eds) Deep Fields. ESO ASTROPHYSICS SYMPOSIA. Springer, Berlin, Heidelberg. https://doi.org/10.1007/10854354_29
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DOI: https://doi.org/10.1007/10854354_29
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Publisher Name: Springer, Berlin, Heidelberg
Print ISBN: 978-3-540-42799-5
Online ISBN: 978-3-540-45514-1
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