论文标题
随机重力波背景的限制和单源检测的前景，宽限
Limits on the Stochastic Gravitational Wave Background and Prospects for Single Source Detection with GRACE Follow-On
论文作者
论文摘要
通过重新解释最近的结果，宽限期的跟进使命可以应用于引力波天文学。现有的宽限期跟随数据将随机重力波背景限制为$ω_{gw} <3.3 \ times10^{7} $在100 MHz时。通过专门的分析，Grace的跟进可能能够检测到局部中性星星二进制二进制物的灵感，这是恒星恒星 - 质量黑洞二进制二进制物的灵感，或中间质量黑洞二进制物的合并。
With a reinterpretation of recent results, the GRACE Follow-On mission can be applied to gravitational wave astronomy. Existing GRACE Follow-On data constrain the stochastic gravitational wave background to $Ω_{GW}<3.3\times10^{7}$ at 100 mHz. With a dedicated analysis, GRACE Follow-On may be able to detect the inspiral of local neutron star binaries, inspiral of subgalactic stellar-mass black hole binaries, or mergers of intermediate-mass black hole binaries within the Milky Way.
