Precision measurement of the integrated luminosity of the data taken by BESIII at center-of-mass energies between 3.810 GeV and 4.600 GeV

BESIII Collaboration

doi:10.1088/1674-1137/39/9/093001

Precision measurement of the integrated luminosity of the data taken by BESIII at center-of-mass energies between 3.810 GeV and 4.600 GeV

BESIII Collaboration

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Abstract

From December 2011 to May 2014, about 5 fb(-1) of data were taken with the BESIII detector at center-ofmass energies between 3.810 GeV and 4.600 GeV to study the charmonium-like states and higher excited charmonium states. The time-integrated luminosity of the collected data sample is measured to a precision of 1% by analyzing events produced by the large-angle Bhabha scattering process.

Original language	English
Article number	093001
Number of pages	7
Journal	Chinese Physics C
Volume	39
Issue number	3
DOIs	https://doi.org/10.1088/1674-1137/39/9/093001
Publication status	Published - Sept-2015

Keywords

precision measurement
luminosity
Bhabha scattering
charmonium

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10.1088/1674-1137/39/9/093001Licence: CC BY

Precision measurement of the integrated luminosity of the data taken by BESIII at center-of-mass energies between 3.810 GeV and 4.600 GeVFinal publisher's version, 1.68 MBLicence: CC BY

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@article{4b0eec8aafd1492986b0d57e4fe8459f,

title = "Precision measurement of the integrated luminosity of the data taken by BESIII at center-of-mass energies between 3.810 GeV and 4.600 GeV",

abstract = "From December 2011 to May 2014, about 5 fb(-1) of data were taken with the BESIII detector at center-ofmass energies between 3.810 GeV and 4.600 GeV to study the charmonium-like states and higher excited charmonium states. The time-integrated luminosity of the collected data sample is measured to a precision of 1\% by analyzing events produced by the large-angle Bhabha scattering process.",

keywords = "precision measurement, luminosity, Bhabha scattering, charmonium",

author = "M. Ablikim and Achasov, \{M. N.\} and X.C. Ai and O. Albayrak and M. Albrecht and D.J. Ambrose and A. Amoroso and Olga Bondarenko and Z. Haddadi and N. Kalantar-Nayestanaki and M. Kavatsyuk and H. Loehner and J.G. Messchendorp and M. Tiemens and \{BESIII Collaboration\}",

year = "2015",

month = sep,

doi = "10.1088/1674-1137/39/9/093001",

language = "English",

volume = "39",

journal = "Chinese Physics C",

issn = "1674-1137",

publisher = "CHINESE PHYSICAL SOC",

number = "3",

}

TY - JOUR

T1 - Precision measurement of the integrated luminosity of the data taken by BESIII at center-of-mass energies between 3.810 GeV and 4.600 GeV

AU - Ablikim, M.

AU - Achasov, M. N.

AU - Ai, X.C.

AU - Albayrak, O.

AU - Albrecht, M.

AU - Ambrose, D.J.

AU - Amoroso, A.

AU - Bondarenko, Olga

AU - Haddadi, Z.

AU - Kalantar-Nayestanaki, N.

AU - Kavatsyuk, M.

AU - Loehner, H.

AU - Messchendorp, J.G.

AU - Tiemens, M.

AU - BESIII Collaboration

PY - 2015/9

Y1 - 2015/9

N2 - From December 2011 to May 2014, about 5 fb(-1) of data were taken with the BESIII detector at center-ofmass energies between 3.810 GeV and 4.600 GeV to study the charmonium-like states and higher excited charmonium states. The time-integrated luminosity of the collected data sample is measured to a precision of 1% by analyzing events produced by the large-angle Bhabha scattering process.

AB - From December 2011 to May 2014, about 5 fb(-1) of data were taken with the BESIII detector at center-ofmass energies between 3.810 GeV and 4.600 GeV to study the charmonium-like states and higher excited charmonium states. The time-integrated luminosity of the collected data sample is measured to a precision of 1% by analyzing events produced by the large-angle Bhabha scattering process.

KW - precision measurement

KW - luminosity

KW - Bhabha scattering

KW - charmonium

U2 - 10.1088/1674-1137/39/9/093001

DO - 10.1088/1674-1137/39/9/093001

M3 - Article

SN - 1674-1137

VL - 39

JO - Chinese Physics C

JF - Chinese Physics C

IS - 3

M1 - 093001

ER -

Precision measurement of the integrated luminosity of the data taken by BESIII at center-of-mass energies between 3.810 GeV and 4.600 GeV

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Keywords

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