On September 14, 2015 at 09:50:45 UTC the two detectors of the Laser Interferometer Gravitational-Wave Observatory simultaneously observed a transient gravitational-wave signal. The signal sweeps upwards in frequency from 35 to 250 Hz with a peak gravitational-wave strain of 1.0×10−21. It matches the waveform predicted by general relativity for the inspiral and merger of a pair of black holes and the ringdown of the resulting single black hole. The signal was observed with a matched-filter signal-to-noise ratio of 24 and a false alarm rate estimated to be less than 1 event per 203 000 years, equivalent to a significance greater than 5.1σ. The source lies at a luminosity distance of 410+160−180 Mpc corresponding to a redshift z=0.09+0.03−0.04. In the source frame, the initial black hole masses are 36+5−4M⊙ and 29+4−4M⊙, and the final black hole mass is 62+4−4M⊙, with 3.0+0.5−0.5M⊙c2 radiated in gravitational waves. All uncertainties define 90% credible intervals. These observations demonstrate the existence of binary stellar-mass black hole systems. This is the first direct detection of gravitational waves and the first observation of a binary black hole merger.
I dabbled with GR many years ago, so I'd have been surprised if this hadn't turned up sooner or later... but My God, look at that... three earth masses-worth of radiated gravitational energy, I can hardly fathom that.
I understand frequency, SNR and significance. The other numbers are mysterious to me; anyone who understands the entirety of this abstract care to explain what the other numbers mean?
Thanks...but it was the rest of the paper itself I was wanting to look at! Trying to download the pdf...along with a fair few other from the slowness of the site.
That's some serious history of physics nerd funny - it's reference to a very embarrassing failure to include time zone discrepancies when analyzing some of the first gravity wave data back in the 1960's