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Titlebook: Optogenetics; Light-Sensing Protei Hiromu Yawo,Hideki Kandori,Amane Koizumi Book 20151st edition Springer Japan 2015 Channelrhodopsin.Halor

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發(fā)表于 2025-3-23 10:08:15 | 只看該作者
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發(fā)表于 2025-3-24 03:51:13 | 只看該作者
Hideji Murakoshi,Akihiro C. E. Shibatathe WDVs over the past 20 years; it is worthwhile to note that the most important tools in all this work have been modest 1-meter class telescopes. Using the observed pulsation spectra of the WDVs, pulsation theory has been able to determine some important quantities describing white dwarfs, such as
16#
發(fā)表于 2025-3-24 10:07:29 | 只看該作者
Hiroshi Kohsaka,Akinao Nosethe WDVs over the past 20 years; it is worthwhile to note that the most important tools in all this work have been modest 1-meter class telescopes. Using the observed pulsation spectra of the WDVs, pulsation theory has been able to determine some important quantities describing white dwarfs, such as
17#
發(fā)表于 2025-3-24 10:51:31 | 只看該作者
Yuki Tsukada,Ikue Morithe WDVs over the past 20 years; it is worthwhile to note that the most important tools in all this work have been modest 1-meter class telescopes. Using the observed pulsation spectra of the WDVs, pulsation theory has been able to determine some important quantities describing white dwarfs, such as
18#
發(fā)表于 2025-3-24 18:07:54 | 只看該作者
19#
發(fā)表于 2025-3-24 22:46:40 | 只看該作者
the WDVs over the past 20 years; it is worthwhile to note that the most important tools in all this work have been modest 1-meter class telescopes. Using the observed pulsation spectra of the WDVs, pulsation theory has been able to determine some important quantities describing white dwarfs, such as
20#
發(fā)表于 2025-3-25 02:16:33 | 只看該作者
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