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- W3100604483 abstract "We review an approach to observation-theory comparisons we call Taste-Testing. In this approach, synthetic observations are made of numerical simulations, and then both real and synthetic observations are tasted (compared) using a variety of statistical tests. We first lay out arguments for bringing theory to observational space rather than observations to theory space. Next, we explain that generating synthetic observations is only a step along the way to the quantitative, statistical, taste tests that offer the most insight. We offer a set of examples focused on polarimetry, scattering and emission by dust, and spectral-line mapping in starforming regions. We conclude with a discussion of the connection between statistical tests used to date and the physics we seek to understand. In particular, we suggest that the lognormal nature of molecular clouds can be created by the interaction of many random processes, as can the lognormal nature of the IMF, so that the fact that both the Clump Mass Function (CMF) and IMF appear lognormal does not necessarily imply a direct relationship between them." @default.
- W3100604483 created "2020-11-23" @default.
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- W3100604483 date "2010-05-01" @default.
- W3100604483 modified "2023-09-26" @default.
- W3100604483 title "A Guide to Comparisons of Star Formation Simulations with Observations" @default.
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- W3100604483 doi "https://doi.org/10.1017/s1743921311000901" @default.
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