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		题名	作者	年代	出处	被引量
	1	Collective bands in 106 Ag and 107 Ag显示文摘	JERRESTAM D KLAMRA W GIZON J	1994	Nu-clear Physics A1994，577，：	1
	2	Structure of high-spin states in 100 Pd显示文摘	G.E. Perez D. Sohler A. Algora Zs. Dombrádi B.M. Nyakó J. Timár L. Zolnai R. Wyss J. Cederk?ll A. Johnson A. Kerek W. Klamra L.-O. Norlin M. Lipoglavs?ek C. Fahlander A. Likar M. Palacz A. Atac J. Nyberg J. Persson A. Gizon J. Gizon A.J. Boston E.S. Paul	2001	Nuclear Physics Section A2001，，1：	1
	3	High spin bands in 102 Pd显示文摘	Dan Jerrestam W. Klamra B. Fogelberg R. Bark A. Gizon J. Gizon E. Ideguchi S. Mitarai M. Piiparinen G. Sletten	1996	Nuclear Physics Section A1996，，2：	1
	4	Alignments and band termination in99,100Ru显示文摘	J. Gizon D. Jerrestam A. Gizon M. Jozsa R. Bark B. Fogelberg E. Ideguchi W. Klamra T. Lindblad S. Mitarai J. Nyberg M. Piiparinen G. Sletten	1993	Zeitschrift für Physik A Hadrons and Nuclei1993，，3：	1
	5	BESTP——An automated Bayesian modeling tool for asteroseismology显示文摘Asteroseismic observations are crucial to constrain stellar models with precision.Bayesian Estimation of STellar Parameters(BESTP)is a tool that utilizes Bayesian statistics and nested sampling Monte Carlo algorithm to search for the stellar models that best match a given set of classical and asteroseismic constraints from observations.The computation and evaluation of models are efficiently performed in an automated and multi-threaded way.To illustrate the capabilities of BESTP,we estimate fundamental stellar properties for the Sun and the red-giant star HD 222076.In both cases,we find models that are consistent with observations.We also evaluate the improvement in the precision of stellar parameters when the oscillation frequencies of individual modes are included as constraints,compared to the case when only the large frequency separation is included.For the solar case,the uncertainties of estimated masses,radii and ages are reduced by 0.7%,0.3%and 8%respectively.For HD 222076,they are reduced even more noticeably by 2%,0.5%and 4.7%respectively.We also note an improvement of 10%for the age of HD 222076 when the Gaia parallax is included as a constraint compared to the case when only the large separation is included as a constraint.	姜晨 Laurent Gizon	2021	Research in Astronomy and Astrophysics2021，21，9：	0

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