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Malmquist bias

(selection bias from detecting only the brighter objects)

The Malmquist bias is a selection bias applicable to astronomical surveys stemming from missing the dimmest objects. The further away, the larger percentage of objects at that distance will be too dim to be detected, and the collected observations will include both bright and dim objects at nearer distances but only the brighter ones at greater distances. In other words, the greater the distance, the stronger the preference (bias) toward brighter objects, meaning evaluation of the randomness of sample-sets must take this into consideration. Generally the brightness is associated with the type or size of the object, and population statistics at different distances need to take the bias into account.

This is in contrast to another type of observation bias, the Eddington bias. I've seen references that call two terms synonymous, but to my understanding, the Eddington bias stems from brightness measurement errors (or perhaps "errors" from seeing, reddening, extinction and the like), whereas the Malmquist bias stems from distance alone and applies even if there are no mistakes measuring the brightness. However, it is possible there is a means of compensating for them that address both biases.


(statistics,astronomy,bias)
Further reading:
http://en.wikipedia.org/wiki/Malmquist_bias
http://ned.ipac.caltech.edu/level5/March03/Teerikorpi/Teerikorpi2_2.html
https://hea-www.harvard.edu/AstroStat/slog/groundtruth.info/AstroStat/slog/2008/eddington-versus-malmquist/index.html
https://ui.adsabs.harvard.edu/abs/1920MeLuS..22....3M/abstract

Referenced by pages:
astronomical survey
Eddington bias
Scott effect
star count
stellar demographics
volume weighting

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