The example you have given is completely different from "confirmed with n-sigma".
In your example, theory predicts 1, and the experiment agrees, with a roughly 20% error bar. That's it.
Now if the experiment had measured $2\pm 0.2$, we could talk about ruling the theory out with a certain confidence level, which can be subtle and involved.
The idea of detecting a signal at $k$-sigma goes a follows: particle physics detectors don't see new particles, they see the decay products of new particles, and the decay products have the same signature as many well understood background processes.
So you make a histogram and look for a bump over background. For simplicity, consider a 1-bin bump. Your Monte Carlo model, which combines the Standard Model with your detector, tells you there will be $N$ background events in the bin, but your data has $T$ events (where $N$ and $T$ are integers, we are counting events).
If $T>N$, you have signal! You created a new particle $S$ times, where $S$ is:
$$ S = T - N$$
Suppose $N=100$ and $T=105$? Do you really believe those 5 events are your Nobel Prize? No, and neither does anybody else.
Both processes are subject to the usual rules of random counting. The expected statistical fluctuations are:
$$ \sigma_N = \sqrt N $$
$$ \sigma_T = \sqrt T $$
The uncertainty on $S$ is then:
$$ \sigma_S^2 = \sigma_T^2 + \sigma_N^2 = T + N $$
You're measurement of the signal is then:
$$ S \pm \sigma_S = [T-N] \pm \sqrt{T + N} $$
and the "number of sigmas" with which you have discover the new particle is:
$$ \frac S {\sigma_S} = \frac{T-N}{\sqrt{T +N}}$$
If we look at the Higgs Boson discovery (and sum over bins to reproduce my "1 bin histogram" analysis):

we can eye-ball (I am sure they were more careful before the announcement), we can eye-ball:
$$ S \approx 240 $$
$$ N \approx 3000$$
so that
$$ \frac S {\sigma_S} = \frac{3240-3000}{\sqrt{3240 + 3000}} =\frac{240}{6240} \approx 3$$
(Note: the real data has background constrained to better than $\sqrt N$...it's not a "1 bin" analysis).
There are several take aways here. Your SNR falls as the square root of your runtime, so a 3rd year of data would have been only a 20% improvement. It also pays huge dividends to find ways to reject background, esp. when your signal-to-noise ration is 1/12 (1 Higgs for every 12 background events).