Journal
CHINESE PHYSICS C
Volume 44, Issue 2, Pages -Publisher
IOP PUBLISHING LTD
DOI: 10.1088/1674-1137/44/2/021001
Keywords
luminosity; Bhabha; digamma; Belle II
Categories
Funding
- Science Committee of the Republic of Armenia [18T-1C180]
- Australian Research Council [DP180102629, DP170102389, DP170102204, DP150103061, FT130100303, FT130100018]
- Austrian Federal Ministry of Education, Science and Research [P 31361-N36]
- Austrian Science Fund [P 31361-N36]
- Natural Sciences and Engineering Research Council of Canada
- Chinese Academy of Sciences [QYZDJ-SSW-SLH011]
- National Natural Science Foundation of China [11521505, 11575017, 11675166, 11761141009, 11705209, 11975076]
- LiaoNing Revitalization Talents Program [XLYC1807135]
- Shanghai Municipal Science and Technology Committee [19ZR1403000]
- Shanghai Pujiang Program [18PJ1401000]
- CAS Center for Excellence in Particle Physics (CCEPP)
- Ministry of Education, Youth and Sports of the Czech Republic [LTT17020]
- Charles University grants [SVV 260448, GAUK 404316]
- European Research Council [PIEF-GA-2013-622527, 700525, 644294, 267104, 638528]
- L'Institut National de Physique Nucleaire et de Physique des Particules (IN2P3) du CNRS (France)
- BMBF (Germany)
- DFG (Germany)
- AvH Foundation (Germany)
- Department of Science and Technology (India)
- Israel Science Foundation [2476/17]
- United States-Israel Binational Science Foundation [2016113]
- Istituto Nazionale di Fisica Nucleare [BELLE2]
- Japan Society for the Promotion of Science [16H03968, 16H03993, 16H06492, 16K05323, 17H01133, 17H05405, 18K03621, 18H05226, 19H00682, 26220706, 26400255]
- National Institute of Informatics, and Science Information NETwork 5 (SINET5) of Japan
- Ministry of Education, Culture, Sports, Science, and Technology (MEXT) of Japan
- National Research Foundation (NRF) of Korea [2016R1D1A1B01010135, 2016R1D1A1B02012900, 2018R1A2B3003643, 2018R1A6A1A06024970, 2018R1D1A1B07047294, 2019K1A3A7A09033840, 2019R1I1A3A01058933]
- Universiti Malaya RU grant
- Akademi Sains Malaysia
- Ministry of Education Malaysia
- Frontiers of Science Program [FOINS-296, CB-221329, CB-236394, CB-254409, CB-180023]
- Thematic Networks program (Mexico)
- Polish Ministry of Science and Higher Education
- National Science Center
- Ministry of Science and Higher Education of the Russian Federation [14.W03.31.0026]
- Slovenian Research Agency [J1-9124, P1-0135]
- Agencia Estatal de Investigacion, Spain [FPA2014-55613-P, FPA2017-84445-P]
- Generalitat Valenciana [CIDEGENT/2018/020]
- Ministry of Science and Technology (Taiwan) [MOST106-2112-M-002-005MY3, MOST107-2119-M-002-035-MY3]
- Ministry of Education (Taiwan)
- Thailand Center of Excellence in Physics
- TUBITAK ULAKBIM (Turkey)
- Min-istry of Education and Science of Ukraine
- US National Science Foundation [PHY-1807007, PHY-1913789]
- US Department of Energy [DE-AC06-76RLO1830, DE-SC0007983, DE-SC0009824, DE-SC0009973, DE-SC0010073, DE-SC0010118, DE-SC0010504, DE-SC0011784, DE-SC0012704]
- National Foundation for Science and Technology Development (NAFOSTED) of Vietnam [103.99-2018.45]
- Compute Canada
- CANARIE
- HGF (Germany)
- MPG (Germany)
- Department of Atomic Energy (India)
- Radiation Science Research Institute
- Foreign Large-size Research Facility Application Supporting project
- Global Science Experimental Data Hub Center of the Korea Institute of Science and Technology Information
- KREONET/GLORIAD
- Grants-in-Aid for Scientific Research [16H03968, 16K05323, 19H00682, 18H05226, 17H01133, 17H05405, 16H03993, 18K03621] Funding Source: KAKEN
- U.S. Department of Energy (DOE) [DE-SC0009973, DE-SC0009824, DE-SC0010073, DE-SC0010118, DE-SC0011784] Funding Source: U.S. Department of Energy (DOE)
Ask authors/readers for more resources
From April to July 2018, a data sample at the peak energy of the resonance was collected with the Belle II detector at the SuperKEKB electron-positron collider. This is the first data sample of the Belle II experiment. Using Bhabha and digamma events, we measure the integrated luminosity of the data sample to be (, where the first uncertainty is statistical and the second is systematic. This work provides a basis for future luminosity measurements at Belle II.
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