Hans Blaster
On August Recess
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Fact: stellar parallax values are either positive, negative or zero.
Fact: the Bayesian experts that “clean-up” the observed data are biased towards their preferred model (the model they philosophically believe in)
It might help to learn about how the parallaxes from Gaia are actually calculated and what they mean.
This review covers how to use Gaia parallaxes, particularly section 3 discusses negative parallaxes.
Gaia Data Release 2 - Using Gaia parallaxes | Astronomy & Astrophysics (A&A)
The model includes two primary components -- the linear motion of the object across the sky (the proper motion as it is known) and the back-and-forth wiggle relative to that moving point (the parallax). Figure 2 from that paper illustrates how noisy simulated data generated from a modeled star with positive parallax (which all ideal stars must have) results in *negative* parallax when processed through the data analysis algorithms.
Gaia Data Release 2 - Using Gaia parallaxes | Astronomy & Astrophysics (A&A)
In other words:
NEGATIVE PARALLAX IS A CONSEQUENCE OF NOISY DATA
Other parts of the paper warn users of Gaia data not to toss out "negative parallax" objects because that would bias the sample towards brighter stars (brighter stars have less noise), closer stars (close stars have proper motions and parallaxes that larger and therefore easier to detect) and most insidious of all, toward the equally noisy distant objects that have small parallaxes that are randomly larger due to noise.
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