reserve 发表于 2025-3-23 11:06:43
Alessandro Giammò,Antonella Biroli5200 kms. are shown to be significant. The second field at 12.30. < R.A. < 15.30., 35° < Dec. < 70° shows a string like structure recognized here for the first time for galaxies with redshifts 2300 < cz. < 2800 kms..Precursor 发表于 2025-3-23 14:56:49
http://reply.papertrans.cn/27/2627/262662/262662_12.png碌碌之人 发表于 2025-3-23 21:03:54
http://reply.papertrans.cn/27/2627/262662/262662_13.pngToxoid-Vaccines 发表于 2025-3-23 22:21:40
http://reply.papertrans.cn/27/2627/262662/262662_14.png波动 发表于 2025-3-24 02:54:24
Search for Bursts of Gamma-Ray Emission from the Crab Pulsar in the Cos-B Data by Adaptive Cluster Aanalysis performed by using photon arrival times not correlated with the Crab direction shows that the events have chance occurrence probabilities of about 10. and therefore may be consistent with (rare) random fluctuations of the background. Finally, 3 σ upper limits on the existence of bursts of emission from the Crab are given.Incise 发表于 2025-3-24 08:38:28
http://reply.papertrans.cn/27/2627/262662/262662_16.pngSTAT 发表于 2025-3-24 12:25:49
STSDAS: The Space Telescope Science Data Analysis Systemnized that many observers will wish to verify or modify the calibration themselves, so that the calibration software is also an integral part of the data analysis system. STSDAS — the Space Telescope Science Data Analysis System — is the software tool kit that allows HST observers to calibrate, reduce, and analyze HST observations.干涉 发表于 2025-3-24 17:04:29
http://reply.papertrans.cn/27/2627/262662/262662_18.pngPostulate 发表于 2025-3-24 20:19:52
http://reply.papertrans.cn/27/2627/262662/262662_19.png漂浮 发表于 2025-3-25 01:33:27
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