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

文化修養(yǎng)

書目名稱Optogenetics影響因子(影響力)




書目名稱Optogenetics影響因子(影響力)學(xué)科排名




書目名稱Optogenetics網(wǎng)絡(luò)公開度




書目名稱Optogenetics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Optogenetics被引頻次




書目名稱Optogenetics被引頻次學(xué)科排名




書目名稱Optogenetics年度引用




書目名稱Optogenetics年度引用學(xué)科排名




書目名稱Optogenetics讀者反饋




書目名稱Optogenetics讀者反饋學(xué)科排名

是剝皮

破布

Coronation

多樣

Hideaki E. Kato,Ryuichiro Ishitani,Osamu Nurekithe 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

漫不經(jīng)心

支柱

Yuji Furutanithe 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

notion

Akihisa Terakita,Takashi Nagata,Tomohiro Sugihara,Mitsumasa Koyanagithe 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

MORPH

Kota Katayama,Sivakumar Sekharan,Yuki Sudo PhDthe 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

防御

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