And it also enable us to continue to detect these individual supermassive black hole binary systems.

它还能让我们继续探测这些单个超大质量黑洞双星系统。

We've done something like the combined signal of 100,000 to up to a million merging supermassive black hole binaries.

而它是 10 万到 100 万个超级黑洞双星合并信号的综合信号。

Which really boosts our ability to that only detect the gravitational wave background, but potentially gravitational waves from the individual in spiraling supermassive black hole binaries.

这提高了我们的能力，使我们不仅能探测到引力波背景，还可能探测到单个螺旋状超大质量黑洞双星的引力波。

Well, the amplitude of the gravitational wave background that we detected is really at the upper limit of what we can model as coming from supermassive black hole binary system.

我们探测到的超大质量黑洞双星系统的引力波背景，其振幅确实达到了我们所能模拟的上限。

So it's not just one signal, it's something like 100,000, potentially a million merging supermassive black hole binaries all at the same time, creating this, you know, symphony of sound that very low frequencies.

所以，这不仅仅是一个信号，而是 10 万个甚至 100 万个超级黑洞双星同时合并发出的信号，创造出了这首低频交响乐。

And what's really important about the signal is that if it really does come from the cosmic mergers, supermassive black hole binaries, it means that supermassive black holes eventually do merge with each other.

这个信号最重要的一点是，如果它真的来自宇宙合并，来自超大质量黑洞双星，那就意味着超大质量黑洞真的最终会彼此合并。