debble 发表于 2025-3-23 11:53:39
Effect of Small Pulsar Distance Variations in Stochastic GW Background Searches with PTAs,in stochastic gravitational wave background searches with Pulsar Timing Arrays”, Phys. Rev. D 90, 062011 (2014). I calculated the magnitude of the overlap reduction functions presented here, the Taylor series expansion, wrote and executed all the numerical codes used to make Table 3.1 and all the fi小步舞 发表于 2025-3-23 15:06:06
http://reply.papertrans.cn/39/3883/388241/388241_12.png四牛在弯曲 发表于 2025-3-23 18:30:59
http://reply.papertrans.cn/39/3883/388241/388241_13.png凹室 发表于 2025-3-23 22:42:56
Cultural Citizenship and Beyond,rlap reduction functions presented here, the Taylor series expansion, wrote and executed all the numerical codes used to make Table 3.1 and all the figures except for the contour plots. I wrote the draft of this paper, and all the text included here.小虫 发表于 2025-3-24 06:11:13
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http://reply.papertrans.cn/39/3883/388241/388241_16.png领巾 发表于 2025-3-24 13:42:30
http://reply.papertrans.cn/39/3883/388241/388241_17.pngPelvic-Floor 发表于 2025-3-24 17:09:06
http://reply.papertrans.cn/39/3883/388241/388241_18.pngMalaise 发表于 2025-3-24 20:08:50
http://reply.papertrans.cn/39/3883/388241/388241_19.pngMELD 发表于 2025-3-25 00:45:47
Introduction,coherent superposition of the cosmic population of SMBHBs is expected to form a diffusive GW background, which has yet to be detected, cf. Hellings and Downs (1983), Rajagopal and Romani (.), Wyithe and Loeb (.), Sesana et al. (.), Jaffe and Backer (.), Jenet et al. (.), Sesana et al. (.), van Haast