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11篇 您的检索式：作者名="E. Stech"

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		题名	作者	年代	出处	被引量
	1	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	2
	2	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	2
	3	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	4	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	5	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	6	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	7	Blood pressure and metabolic control as risk factors for nephropathy in Type 1 (insulin-dependent) diabetes显示文摘	Ch. Hasslacher W. Stech P. Wahl E. Ritz	1985	Diabetologia1985，，1：	1
	8	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	9	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	10	Universal primer set for the full-length amplification of all influenza A viruses显示文摘	E. Hoffmann J. Stech Y. Guan R. G. Webster D. R. Perez	2001	Archives of Virology2001，，12：	1
	11	2-6 First Direct Measurement of 12C(12C, n)23Mg at Stellar Energies显示文摘The first stars in the early Universe were formed about 400 million years after the big bang. Verification of the existence of these stars is important for our understanding of the evolution of the Universe[1]. It has been predicted that for Population-III stellar production yields, the abundances of odd-Z elements are remarkably deficient compared to their adjacent even-Z elements[2]. Astronomers are searching for long-lived, low mass stars with the unique nucleosynthetic pattern matching the predicted yields[3].	Tang Xiaodong B. Bucher X. Fang A. Heger S. Almaraz-Calderon A. Alongi A.D. Ayangeakaa M. Beard A. Best J. Browne C. Cahillane M. Couder R.J. deBoer A. Kontos L. Lamm Y.J. Li A. Long W. Lu S. Lyons M. Notani D. Patel N. Paul M. Pignatari A. Roberts D. Robertson K. Smith E. Stech R. Talwar W.P. Tan M. Wiescher S.E. Woosley	2015	IMP & HIRFL Annual Report2015，，1：	0

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