Cargando…

Track-based alignment for the BESIII CGEM detector in the cosmic-ray test

The Beijing Electron Spectrometer III (BESIII) is a multipurpose detector operating on the Beijing Electron Positron Collider II (BEPCII). After more than ten year's operation, the efficiency of the inner layers of the Main Drift Chamber (MDC) decreased significantly. To solve this issue, the B...

Descripción completa

Detalles Bibliográficos
Autores principales: Guo, A.Q., Wu, L.H., Wang, L.L., Mitchell, R.E., Amoroso, A., Ferroli, R. Baldini, Balossino, I., Bertani, M., Bettoni, D., Bortone, A., Calcaterra, A., Cheng, W., Cibinetto, G., Cotta Ramusino, A., Cossio, F., Dong, M.Y., Da Rocha Rolo, M., De Mori, F., Destefanis, M., Dong, J., Evangelisti, F., Farinelli, R., Fava, L., Felici, G., Garzia, I., Gatta, M., Giraudo, G., Gramigna, S., Greco, M., Huang, Z., Hou, Y.R., Imoehl, W., Lavezzi, L., Lu, X.L., Maggiora, M., Malaguti, R., Mangoni, A., Marcello, S., Melchiorri, M., Mezzadri, G., Ouyang, Q., Pace, E., Pacetti, S., Patteri, P., Pellegrino, J., Rivetti, A., Shi, R.S., Scodeggio, M., Sosio, S., Spataro, S., Wang, H.P., Zhao, J.Y.
Lenguaje:eng
Publicado: 2022
Materias:
Acceso en línea:http://cds.cern.ch/record/2839589
_version_ 1780975973763645440
author Guo, A.Q.
Wu, L.H.
Wang, L.L.
Mitchell, R.E.
Amoroso, A.
Ferroli, R. Baldini
Balossino, I.
Bertani, M.
Bettoni, D.
Bortone, A.
Calcaterra, A.
Cheng, W.
Cibinetto, G.
Cotta Ramusino, A.
Cossio, F.
Dong, M.Y.
Da Rocha Rolo, M.
De Mori, F.
Destefanis, M.
Dong, J.
Evangelisti, F.
Farinelli, R.
Fava, L.
Felici, G.
Garzia, I.
Gatta, M.
Giraudo, G.
Gramigna, S.
Greco, M.
Huang, Z.
Hou, Y.R.
Imoehl, W.
Lavezzi, L.
Lu, X.L.
Maggiora, M.
Malaguti, R.
Mangoni, A.
Marcello, S.
Melchiorri, M.
Mezzadri, G.
Ouyang, Q.
Pace, E.
Pacetti, S.
Patteri, P.
Pellegrino, J.
Rivetti, A.
Shi, R.S.
Scodeggio, M.
Sosio, S.
Spataro, S.
Wang, H.P.
Zhao, J.Y.
author_facet Guo, A.Q.
Wu, L.H.
Wang, L.L.
Mitchell, R.E.
Amoroso, A.
Ferroli, R. Baldini
Balossino, I.
Bertani, M.
Bettoni, D.
Bortone, A.
Calcaterra, A.
Cheng, W.
Cibinetto, G.
Cotta Ramusino, A.
Cossio, F.
Dong, M.Y.
Da Rocha Rolo, M.
De Mori, F.
Destefanis, M.
Dong, J.
Evangelisti, F.
Farinelli, R.
Fava, L.
Felici, G.
Garzia, I.
Gatta, M.
Giraudo, G.
Gramigna, S.
Greco, M.
Huang, Z.
Hou, Y.R.
Imoehl, W.
Lavezzi, L.
Lu, X.L.
Maggiora, M.
Malaguti, R.
Mangoni, A.
Marcello, S.
Melchiorri, M.
Mezzadri, G.
Ouyang, Q.
Pace, E.
Pacetti, S.
Patteri, P.
Pellegrino, J.
Rivetti, A.
Shi, R.S.
Scodeggio, M.
Sosio, S.
Spataro, S.
Wang, H.P.
Zhao, J.Y.
author_sort Guo, A.Q.
collection CERN
description The Beijing Electron Spectrometer III (BESIII) is a multipurpose detector operating on the Beijing Electron Positron Collider II (BEPCII). After more than ten year's operation, the efficiency of the inner layers of the Main Drift Chamber (MDC) decreased significantly. To solve this issue, the BESIII collaboration is planning to replace the inner part of the MDC with three layers of Cylindrical triple-Gas Electron Multipliers (CGEM). The new features of the CGEM detector will improve the spatial resolution to 130 $\mu$m. To meet this goal, a careful calibration of the detector is necessary to fully exploit the potential of the CGEM detector. In all the calibrations, the detector alignment plays an important role to improve the detector precision. The track-based alignment for the CGEM detector with the Millepede algorithm is implemented to reduce the uncertainties of the hit position measurement. Using the cosmic-ray data taken in 2020 with the two layers setup, the displacement of the outer layer with respect to the inner layer is determined by a simultaneous fit applied to more than 160000 tracks. A good alignment precision has been achieved that guarantees the design request could be satisfied in the future. A further alignment will be performed using the combined information of tracks from cosmic-ray and collisions after the CGEM is installed into the BESIII detector.
id cern-2839589
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2022
record_format invenio
spelling cern-28395892022-11-08T22:14:31Zhttp://cds.cern.ch/record/2839589engGuo, A.Q.Wu, L.H.Wang, L.L.Mitchell, R.E.Amoroso, A.Ferroli, R. BaldiniBalossino, I.Bertani, M.Bettoni, D.Bortone, A.Calcaterra, A.Cheng, W.Cibinetto, G.Cotta Ramusino, A.Cossio, F.Dong, M.Y.Da Rocha Rolo, M.De Mori, F.Destefanis, M.Dong, J.Evangelisti, F.Farinelli, R.Fava, L.Felici, G.Garzia, I.Gatta, M.Giraudo, G.Gramigna, S.Greco, M.Huang, Z.Hou, Y.R.Imoehl, W.Lavezzi, L.Lu, X.L.Maggiora, M.Malaguti, R.Mangoni, A.Marcello, S.Melchiorri, M.Mezzadri, G.Ouyang, Q.Pace, E.Pacetti, S.Patteri, P.Pellegrino, J.Rivetti, A.Shi, R.S.Scodeggio, M.Sosio, S.Spataro, S.Wang, H.P.Zhao, J.Y.Track-based alignment for the BESIII CGEM detector in the cosmic-ray testphysics.ins-dethep-exThe Beijing Electron Spectrometer III (BESIII) is a multipurpose detector operating on the Beijing Electron Positron Collider II (BEPCII). After more than ten year's operation, the efficiency of the inner layers of the Main Drift Chamber (MDC) decreased significantly. To solve this issue, the BESIII collaboration is planning to replace the inner part of the MDC with three layers of Cylindrical triple-Gas Electron Multipliers (CGEM). The new features of the CGEM detector will improve the spatial resolution to 130 $\mu$m. To meet this goal, a careful calibration of the detector is necessary to fully exploit the potential of the CGEM detector. In all the calibrations, the detector alignment plays an important role to improve the detector precision. The track-based alignment for the CGEM detector with the Millepede algorithm is implemented to reduce the uncertainties of the hit position measurement. Using the cosmic-ray data taken in 2020 with the two layers setup, the displacement of the outer layer with respect to the inner layer is determined by a simultaneous fit applied to more than 160000 tracks. A good alignment precision has been achieved that guarantees the design request could be satisfied in the future. A further alignment will be performed using the combined information of tracks from cosmic-ray and collisions after the CGEM is installed into the BESIII detector.oai:cds.cern.ch:28395892022-11-02
spellingShingle physics.ins-det
hep-ex
Guo, A.Q.
Wu, L.H.
Wang, L.L.
Mitchell, R.E.
Amoroso, A.
Ferroli, R. Baldini
Balossino, I.
Bertani, M.
Bettoni, D.
Bortone, A.
Calcaterra, A.
Cheng, W.
Cibinetto, G.
Cotta Ramusino, A.
Cossio, F.
Dong, M.Y.
Da Rocha Rolo, M.
De Mori, F.
Destefanis, M.
Dong, J.
Evangelisti, F.
Farinelli, R.
Fava, L.
Felici, G.
Garzia, I.
Gatta, M.
Giraudo, G.
Gramigna, S.
Greco, M.
Huang, Z.
Hou, Y.R.
Imoehl, W.
Lavezzi, L.
Lu, X.L.
Maggiora, M.
Malaguti, R.
Mangoni, A.
Marcello, S.
Melchiorri, M.
Mezzadri, G.
Ouyang, Q.
Pace, E.
Pacetti, S.
Patteri, P.
Pellegrino, J.
Rivetti, A.
Shi, R.S.
Scodeggio, M.
Sosio, S.
Spataro, S.
Wang, H.P.
Zhao, J.Y.
Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
title Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
title_full Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
title_fullStr Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
title_full_unstemmed Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
title_short Track-based alignment for the BESIII CGEM detector in the cosmic-ray test
title_sort track-based alignment for the besiii cgem detector in the cosmic-ray test
topic physics.ins-det
hep-ex
url http://cds.cern.ch/record/2839589
work_keys_str_mv AT guoaq trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT wulh trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT wangll trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT mitchellre trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT amorosoa trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT ferrolirbaldini trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT balossinoi trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT bertanim trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT bettonid trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT bortonea trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT calcaterraa trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT chengw trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT cibinettog trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT cottaramusinoa trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT cossiof trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT dongmy trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT darocharolom trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT demorif trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT destefanism trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT dongj trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT evangelistif trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT farinellir trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT faval trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT felicig trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT garziai trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT gattam trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT giraudog trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT gramignas trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT grecom trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT huangz trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT houyr trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT imoehlw trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT lavezzil trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT luxl trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT maggioram trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT malagutir trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT mangonia trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT marcellos trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT melchiorrim trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT mezzadrig trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT ouyangq trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT pacee trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT pacettis trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT patterip trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT pellegrinoj trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT rivettia trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT shirs trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT scodeggiom trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT sosios trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT spataros trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT wanghp trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest
AT zhaojy trackbasedalignmentforthebesiiicgemdetectorinthecosmicraytest