gait-cycle 发表于 2025-3-23 11:59:21
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https://doi.org/10.1007/978-3-8348-9516-5ta from it. These two goals might require different processing techniques. For instance, you don’t want to do any kind of histogram stretch of the data to see a faint star or nebula if you want to do photometry as this changes the relative brightness of the data recorded. But to bring out faint nebulosity for a wall print, that would be fine.companion 发表于 2025-3-23 19:00:42
http://reply.papertrans.cn/20/1916/191526/191526_13.pngFID 发表于 2025-3-23 23:56:26
http://reply.papertrans.cn/20/1916/191526/191526_14.pngovershadow 发表于 2025-3-24 02:27:41
http://reply.papertrans.cn/20/1916/191526/191526_15.png笨拙的我 发表于 2025-3-24 08:59:10
http://reply.papertrans.cn/20/1916/191526/191526_16.pngfloaters 发表于 2025-3-24 10:57:32
http://reply.papertrans.cn/20/1916/191526/191526_17.png–LOUS 发表于 2025-3-24 18:22:12
Masterkurs Parallele und Verteilte Systemeject that is closer to the observer. So the light gathering capability of the telescope is the primary consideration when choosing a system for both visual or photographic applications. This means size, and yes, it does matter.排斥 发表于 2025-3-24 19:53:39
http://reply.papertrans.cn/20/1916/191526/191526_19.png潜伏期 发表于 2025-3-25 01:31:06
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