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8篇 您的检索式：作者名="Zane K"

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		题名	作者	年代	出处	被引量
	1	The cognitive perspective in strategy: An integrative review显示文摘	Narayanan V K Zane L J Kemmerer B	2011	Journal of Management2011，37，：	1
	2	Analysis of pesticide residues in sugarcane juice using QuEChERS sample preparation and gas chromatography with electron capture detection 显示文摘	Zanes Furlani R P Marcilio K M Leme F M	2011	Food Chem2011，126，3：	1
	3	Abortion surveillance-United States,2007显示文摘	Pazol K Zane S Parker W	2011	MMVCR Surveill Suture2011，60，1：	1
	4	YMDD motif in hepatitis B virus DNA polymerase influences on replication and Camivudeine resistance:A study by in vitro full-length viral DNA transfertion显示文摘	Naoya K Yasushi S	1999	Hepatology1999，29，3：	1
	5	Performance measurement of Hawaii State public libraries:An application of data envelopment analysis (DEA)显示文摘	Sharma K R Leung P Zane L	1999	Agricultural and Resource Economics Review1999，，10：	1
	6	Correlation between virulence and colony morphology in Vibrio vulnificus显示文摘	SIMPSON L M WHITE V K ZANE S F	1987	Infect Immun1987，55，1：	1
	7	Condylar and mandibular morpho- logical criteria in the 2D and 3D MSCT imaging for patients with Class II division 1 subdivision malocclusion 显示文摘	Zane K Ilga U Gaida K	2007	Stomatologija2007，9，3：	1
	8	Dense matter with eXTP显示文摘In this White Paper we present the potential of the Enhanced X-ray Timing and Polarimetry(eXTP) mission for determining the nature of dense matter; neutron star cores host an extreme density regime which cannot be replicated in a terrestrial laboratory. The tightest statistical constraints on the dense matter equation of state will come from pulse profile modelling of accretion-powered pulsars, burst oscillation sources, and rotation-powered pulsars. Additional constraints will derive from spin measurements, burst spectra, and properties of the accretion flows in the vicinity of the neutron star. Under development by an international Consortium led by the Institute of High Energy Physics of the Chinese Academy of Sciences, the eXTP mission is expected to be launched in the mid 2020 s.	Anna L.Watts WenFei Yu Juri Poutanen Shu Zhang Sudip Bhattacharyya Slavko Bogdanov Long Ji Alessandro Patruno Thomas E.Riley Pavel Bakala Altan Baykal Federico Bernardini Ignazio Bombaci Edward Brown Yuri Cavecchi Deepto Chakrabarty Jér?me Chenevez Nathalie Degenaar Melania Del Santo Tiziana Di Salvo Victor Doroshenko Maurizio Falanga Robert D.Ferdman Marco Feroci Angelo F.Gambino MingYu Ge Svenja K.Greif Sebastien Guillot Can Gungor Dieter H.Hartmann Kai Hebeler Alexander Heger Jeroen Homan Rosario Iaria Jean in 't Zand Oleg Kargaltsev Aleksi KurkelaTheoretical Physics Department CERN XiaoYu Lai Ang Li XiangDong Li ZhaoSheng Li Manuel Linares FangJun Lu Simin Mahmoodifar Mariano Méndez M.Coleman Miller Sharon Morsink Joonas N?ttil? Andrea Possenti Chanda Prescod-Weinstein JinLu Qu Alessandro Riggio Tuomo Salmi Andrea Sanna Andrea Santangelo Hendrik Schatz Achim Schwenk LiMing Song Eva?rámková Benjamin Stappers Holger Stiele Tod Strohmayer Ingo Tews Laura Tolos Gabriel T?r?k David Tsang Martin Urbanec Andrea Vacchi RenXin Xu YuPeng Xu Silvia Zane GuoBao Zhang ShuangNan Zhang WenDa Zhang ShiJie Zheng Xia Zhou	2019	Science China(Physics,Mechanics & Astronomy)2019，62，2：	0

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