Bias and beyond

dc.creatorTegmark, Max
dc.date1998-09-15
dc.date.accessioned2026-07-07T02:27:56Z
dc.date.available2026-07-07T02:27:56Z
dc.descriptionIt is becoming increasingly clear that galaxy bias is complicated, with evidence indicating that it can be time-dependent, morphology-dependent, scale-dependent, non-linear and non-deterministic. We discuss strategies for overcoming these complications and performing precision cosmological tests with upcoming redshift surveys.
dc.description4 pages, with 1 figure included. Links and more figures at http://www.sns.ias.edu/~max/biasframe.html or from max@ias.edu. To appear in ``Wide Field Surveys in Cosmology'', S. Colombi and Y. Mellier (eds), Editions Frontieres (1998)
dc.identifierhttps://arxiv.org/abs/astro-ph/9809185
dc.identifierhttp://arxiv.org/abs/astro-ph/9809185
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/12907
dc.subjectAstrophysics
dc.titleBias and beyond
dc.typetext

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