Other astronomers say the method of pulling faint
planetary signals out of background noise needs to be verified.
In the process, they say they learned to better distinguish a
true planetary signal from astrophysical false alarms or instrumental noise.
In the case of Kepler 452 b, the team performed extensive simulations as well as ground - based observations of the star and its immediate surroundings to rule out the possibility of anything spoofing
the planetary signal.
The team used novel analysis techniques in squeezing
the planetary signals out of the data.
«Fortunately,
the planetary signal predicts how fast the apparent positions of the background star and planetary host star will separate, and our observations have confirmed this prediction.
In this example,
the planetary signal has been increased in strength relative by several orders of magnitude relative to the actual signal.