Comments:
If my estimates are correct, and they may be little off, it looks like about a 6 dB increase in signal at ~1.4 gHz. At first I thought this wasn't much, since that's only about 1 standard S Unit or doubling the signal twice. However, since we're talking about noise level, this could mean detecting signals from stars much farther away than currently. It should also gives us better resolution in looking at the clumping of galaxies in the observable universe and help in deciding if the standard model or some other explanation is more realistic.
A monumental waste of time and money...
Great article :-)
Particularly interesting if you have read Cixen Liu's "Three Body Problem." <br><br>http://www.barnesandnoble.com/w/the-three-body-problem-cixin-liu/1119317099?ean=9780765377067
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