s=3.650 GeV during May 2009 and at √s=3.773 GeV from January 2010 to May 2011. By analyzing the large angle Bhabha scattering events, the integrated luminosities of the two data sets are measured to be (44.49±0.02±0.44) pb-1 and (2916.94±0.18±29.17) pb-1, respectively, where the first error is statistical and the second error is systematic."> Measurement of the integrated luminosities of the data taken by BESⅢ at <I>s</I>=3.650 and 3.773 GeV -
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    Ablikim M et al. (BESⅢ collaboration). Nucl. Instrum. Methods A, 2004, 614: 345[2] BAI J Z et al. (BESⅢ collaboration). Nucl. Instrum. Methods A, 1994. 344: 319; 2001, 458: 627[3] Calame C M C, Montagna G, Nicrosini O, Piccinini F. Nucl. Phys. Proc. Suppl., 2004, 131: 48-55[4] Berger N, ZHU Kai et al. Chinese Physics C (HEP NP), 2010, 34(12): 1779-1784

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