eustachian-tube
发表于 2025-3-23 10:26:31
nd ν. for a sample of radio sources complete to flux density S at the selection frequency ν. (flux densities will be expressed in Jy and frequencies in GHz). Such a detailed specification is necessary because g(α) has been found to depend on all three parameters. The effect of varying ν. is well-kno
拥护者
发表于 2025-3-23 15:39:56
nation. F (8) ~ve have F(e) : f (e) ~ (S" ) e. . ~ is a Bessel function. It is assumed here that the spectrum of gravitational waves takes the form 1 hI‘::: hoK for all relevant wavelengths, a is beam width of the radio antenna, d= d~, and ~ is the duration of the process of recombinations in -time.
Eructation
发表于 2025-3-23 20:32:43
including Warner, Kenderdine, Waggett, Masson and Mayer. The results of the first observations are at present in a preliminary state but we hope that in time they will form the first part of the 6C survey. The purpose of the survey is not to reach the faintest sources detected so far in aperture syn
FADE
发表于 2025-3-23 22:38:03
http://reply.papertrans.cn/88/8775/877484/877484_14.png
预示
发表于 2025-3-24 03:34:55
http://reply.papertrans.cn/88/8775/877484/877484_15.png
Pepsin
发表于 2025-3-24 09:06:54
http://reply.papertrans.cn/88/8775/877484/877484_16.png
aspect
发表于 2025-3-24 10:41:08
http://reply.papertrans.cn/88/8775/877484/877484_17.png
dragon
发表于 2025-3-24 15:14:12
http://reply.papertrans.cn/88/8775/877484/877484_18.png
意外
发表于 2025-3-24 19:54:47
http://reply.papertrans.cn/88/8775/877484/877484_19.png
表示向下
发表于 2025-3-25 00:20:51
http://reply.papertrans.cn/88/8775/877484/877484_20.png