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@ARTICLE{Ablikim:208662,
author = {Ablikim, M. and Achasov, M. N. and Ahmed, S. and Ai, X. C.
and Albayrak, O. and Albrecht, M. and Ambrose, D. J. and
Amoroso, A. and An, F. F. and An, Q. and Bai, J. Z. and
Ferroli, R. Baldini and Ban, Y. and Bennett, D. W. and
Bennett, J. V. and Berger, N. and Bertani, M. and Bettoni,
D. and Bian, J. M. and Bianchi, F. and Boger, E. and Boyko,
I. and Briere, R. A. and Cai, H. and Cai, X. and Cakir, O.
and Calcaterra, A. and Cao, G. F. and Cetin, S. A. and Chai,
J. and Chang, J. F. and Chelkov, G. and Chen, G. and Chen,
H. S. and Chen, J. C. and Chen, M. L. and Chen, S. and Chen,
S. J. and Chen, X. and Chen, X. R. and Chen, Y. B. and
Cheng, H. P. and Chu, X. K. and Cibinetto, G. and Dai, H. L.
and Dai, J. P. and Dbeyssi, A. and Dedovich, D. and Deng, Z.
Y. and Denig, A. and Denysenko, I. and Destefanis, M. and De
Mori, F. and Ding, Y. and Dong, C. and Dong, J. and Dong, L.
Y. and Dong, M. Y. and Dou, Z. L. and Du, S. X. and Duan, P.
F. and Fan, J. Z. and Fang, J. and Fang, S. S. and Fang, X.
and Fang, Y. and Farinelli, R. and Fava, L. and Fedorov, O.
and Feldbauer, F. and Felici, G. and Feng, C. Q. and
Fioravanti, E. and Fritsch, M. and Fu, C. D. and Gao, Q. and
Gao, X. L. and Gao, Y. and Gao, Z. and Garzia, I. and
Goetzen, K. and Gong, L. and Gong, W. X. and Gradl, W. and
Greco, M. and Gu, M. H. and Gu, Y. T. and Guan, Y. H. and
Guo, A. Q. and Guo, L. B. and Guo, R. P. and Guo, Y. and
Guo, Y. P. and Haddadi, Z. and Hafner, A. and Han, S. and
Hao, X. Q. and Harris, F. A. and He, K. L. and Heinsius, F.
H. and Held, T. and Heng, Y. K. and Holtmann, T. and Hou, Z.
L. and Hu, C. and Hu, H. M. and Hu, J. F. and Hu, T. and Hu,
Y. and Huang, G. S. and Huang, J. S. and Huang, X. T. and
Huang, X. Z. and Huang, Y. and Huang, Z. L. and Hussain, T.
and Ji, Q. and Ji, Q. P. and Ji, X. B. and Ji, X. L. and
Jiang, L. W. and Jiang, X. S. and Jiang, X. Y. and Jiao, J.
B. and Jiao, Z. and Jin, D. P. and Jin, S. and Johansson, T.
and Julin, A. and Kalantar-Nayestanaki, N. and Kang, X. L.
and Kang, X. S. and Kavatsyuk, M. and Ke, B. C. and Kiese,
P. and Kliemt, R. and Kloss, B. and Kolcu, O. B. and Kopf,
B. and Kornicer, M. and Kupsc, A. and Kühn, W. and Lange,
J. S. and Lara, M. and Larin, P. and Leithoff, H. and Leng,
C. and Li, C. and Li, Cheng and Li, D. M. and Li, F. and Li,
F. Y. and Li, G. and Li, H. B. and Li, H. J. and Li, J. C.
and Li, Jin and Li, K. and Li, K. and Li, Lei and Li, P. R.
and Li, Q. Y. and Li, T. and Li, W. D. and Li, W. G. and Li,
X. L. and Li, X. N. and Li, X. Q. and Li, Y. B. and Li, Z.
B. and Liang, H. and Liang, Y. F. and Liang, Y. T. and Liao,
G. R. and Lin, D. X. and Liu, B. and Liu, B. J. and Liu, C.
X. and Liu, D. and Liu, F. H. and Liu, Fang and Liu, Feng
and Liu, H. B. and Liu, H. H. and Liu, H. H. and Liu, H. M.
and Liu, J. and Liu, J. B. and Liu, J. P. and Liu, J. Y. and
Liu, K. and Liu, K. Y. and Liu, L. D. and Liu, P. L. and
Liu, Q. and Liu, S. B. and Liu, X. and Liu, Y. B. and Liu,
Y. Y. and Liu, Z. A. and Liu, Zhiqing and Loehner, H. and
Long, Y. F. and Lou, X. C. and Lu, H. J. and Lu, J. G. and
Lu, Y. and Lu, Y. P. and Luo, C. L. and Luo, M. X. and Luo,
T. and Luo, X. L. and Lyu, X. R. and Ma, F. C. and Ma, H. L.
and Ma, L. L. and Ma, M. M. and Ma, Q. M. and Ma, T. and Ma,
X. N. and Ma, X. Y. and Ma, Y. M. and Maas, F. E. and
Maggiora, M. and Malik, Q. A. and Mao, Y. J. and Mao, Z. P.
and Marcello, S. and Messchendorp, J. G. and Mezzadri, G.
and Min, J. and Min, T. J. and Mitchell, R. E. and Mo, X. H.
and Mo, Y. J. and Morales, C. Morales and Muchnoi, N. Yu.
and Muramatsu, H. and Musiol, P. and Nefedov, Y. and
Nerling, F. and Nikolaev, I. B. and Ning, Z. and Nisar, S.
and Niu, S. L. and Niu, X. Y. and Olsen, S. L. and Ouyang,
Q. and Pacetti, S. and Pan, Y. and Patteri, P. and
Pelizaeus, M. and Peng, H. P. and Peters, K. and Pettersson,
J. and Ping, J. L. and Ping, R. G. and Poling, R. and
Prasad, V. and Qi, H. R. and Qi, M. and Qian, S. and Qiao,
C. F. and Qin, L. Q. and Qin, N. and Qin, X. S. and Qin, Z.
H. and Qiu, J. F. and Rashid, K. H. and Redmer, C. F. and
Ripka, M. and Rong, G. and Rosner, Ch. and Ruan, X. D. and
Sarantsev, A. and Savrié, M. and Schnier, C. and
Schoenning, K. and Schumann, S. and Shan, W. and Shao, M.
and Shen, C. P. and Shen, P. X. and Shen, X. Y. and Sheng,
H. Y. and Shi, M. and Song, W. M. and Song, X. Y. and Sosio,
S. and Spataro, S. and Sun, G. X. and Sun, J. F. and Sun, S.
S. and Sun, X. H. and Sun, Y. J. and Sun, Y. Z. and Sun, Z.
J. and Sun, Z. T. and Tang, C. J. and Tang, X. and Tapan, I.
and Thorndike, E. H. and Tiemens, M. and Uman, I. and
Varner, G. S. and Wang, B. and Wang, B. L. and Wang, D. and
Wang, D. Y. and Wang, K. and Wang, L. L. and Wang, L. S. and
Wang, M. and Wang, P. and Wang, P. L. and Wang, W. and Wang,
W. P. and Wang, X. F. and Wang, Y. and Wang, Y. D. and Wang,
Y. F. and Wang, Y. Q. and Wang, Z. and Wang, Z. G. and Wang,
Z. H. and Wang, Z. Y.},
collaboration = {{BESIII Collaboration}},
title = {{M}easurement of integrated luminosity and center-of-mass
energy of data taken by {BESIII} at},
journal = {Chinese physics / C},
volume = {41},
number = {11},
issn = {1674-1137},
address = {Bristol [u.a.]},
publisher = {IOP Publ.},
reportid = {GSI-2018-00050},
pages = {113001},
year = {2017},
note = {Content from this work may be used under the terms of the
Creative Commons Attribution 3.0 licence. Any
furtherdistribution of this work must maintain attribution
to the author(s) and the title of the work, journal citation
and DOI. Article fundedby SCOAP3 and published under licence
by Chinese Physical Society and the Institute of High Energy
Physics of the Chinese Academyof Sciences and the Institute
of Modern Physics of the Chinese Academy of Sciences and IOP
Publishing Ltd},
abstract = {To study the nature of the state $Y(2175)$, a dedicated
data set of $e^+e^-$ collision data was collected at the
center-of-mass energy of 2.125 GeV with the BESIII detector
at the BEPCII collider. By analyzing large-angle Bhabha
scattering events, the integrated luminosity of this data
set is determined to be $108.49\pm0.02\pm0.85$ pb$^{-1}$,
where the first uncertainty is statistical and the second
one is systematic. In addition, the center-of-mass energy of
the data set is determined with radiative dimuon events to
be $2126.55\pm0.03\pm0.85$ MeV, where the first uncertainty
is statistical and the second one is systematic.},
cin = {HSP / HIM},
ddc = {530},
cid = {I:(DE-Ds200)HSP-20080821OR101 /
I:(DE-Ds200)HIM-20110223OR116},
pnm = {612 - Cosmic Matter in the Laboratory (POF3-612) / OAGSI -
Open Access Publikation mit Unterstützung des GSI
Helmholtzzentrums für Schwerionenforschung (OAGSI) /
HGF-IVF-VH-GS-201 - HGS-HIRe : (HGF-IVF-VH-GS-201) /
SUC-GSI-Frankfurt - Strategic university cooperation GSI-U
Frankfurt/M (SUC-GSI-FR)},
pid = {G:(DE-HGF)POF3-612 / G:(DE-Ds200)OAGSI /
G:(DE-Ds200)HGF-IVF-VH-GS-201 / G:(DE-Ds200)SUC-GSI-FR},
typ = {PUB:(DE-HGF)16},
UT = {WOS:000414482100001},
doi = {10.1088/1674-1137/41/11/113001},
url = {https://repository.gsi.de/record/208662},
}
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