The Mark II detector for the SLC

G. Abrams; C. E. Adolphsen; C. Akerlof; J. P. Alexander; M. Alvarez; D. Averill; A. R. Baden; J. Ballam; B. C. Barish; T. Barklow; B. A. Barnett; J. Bartelt; D. Blockus; W. De Boer; G. Bonvicini; C. Boswell; A. Boyarski; J. Boyer; B. Brabson; K. Braune; A. Breakstone; J. M. Brom; F. Bulos; P. R. Burchat; D. L. Burke; F. Butler; F. Calvino; R. J. Cence; J. Chapman; M. Chmeissani; D. Cords; D. P. Coupal; P. Dauncey; H. C. Destaebler; D. E. Dorfan; J. M. Dorfan; P. S. Drell; D. C. Drewer; J. Fay; G. J. Feldman; D. Fernandes; E. Fernandez; R. C. Field; W. T. Ford; C. Fordham; R. Frey; D. Fujino; K. K. Gan; C. Gatto; E. Gero; G. Gidal; T. Glanzman; G. Goldhaber; J. J. Gomez Cadenas; X. Gong; G. Gratta; A. Green; P. Grosse-Wiesmann; J. Haggerty; G. Hanson; R. Harr; B. Harral; F. A. Harris; C. M. Hawkes; K. Hayes; C. Hearty; D. Herrup; C. A. Heusch; T. Himel; D. A. Hinshaw; M. Hoenk; S. O. Holmgren; S. J. Hong; D. Hutchinson; J. Hylen; W. R. Innes; R. G. Jacobsen; M. Jaffre; J. A. Jaros; C. K. Jung; I. Juricic; J. A. Kadyk; D. Karlen; J. Kent; M. King; S. R. Klein; L. Koepke; D. Koetke; A. Koide; S. Komamiya; W. Koska; L. A. Kowalski; W. Kozanecki; J. F. Kral; M. Kuhlen; L. Labarga; A. J. Lankford; R. R. Larsen; M. E. Levi; Z. Li; A. M. Litke; V. Lüth; G. R. Lynch; J. A. McKenna; J. A.J. Matthews; T. Mattison; B. D. Milliken; K. C. Moffeit; L. Müller; C. T. Munger; W. N. Murray; J. Nash; M. E. Nelson; D. Nitz; H. Ogren; R. A. Ong; K. F. O'Shaughnessy; S. I. Parker; C. Peck; J. Perl; M. L. Perl; F. Perrier; A. Petersen; M. Petradza; R. Pitthan; F. C. Porter; P. Rankin; J. D. Richman; K. Riles; F. R. Rouse; D. R. Rust; H. F.W. Sadrozinski; M. W. Schaad; W. B. Schmidke; B. A. Schumm; A. S. Schwarz; A. Seiden; J. G. Smith; A. Snyder; E. Soderstrom; D. P. Stoker; R. Stroynowski; M. Swartz; R. E. Taylor; R. Thun; G. H. Trilling; R. Tschirhart; M. Turala; R. Van Kooten; S. Vejcik; H. Veltman; P. Voruganti; S. R. Wagner; S. Watson; P. Weber; A. Weigend; A. J. Weinstein; A. J. Weir; S. Weisz; S. L. White; E. Wicklund; R. C. Wolf; D. R. Wood; M. Woods; G. Wormser; R. Wright; D. Y. Wu; M. Yurko; C. Zaccardelli; C. Von Zanthier

doi:10.1016/0168-9002(89)91217-5

The Mark II detector for the SLC

G. Abrams^*, C. E. Adolphsen, C. Akerlof, J. P. Alexander, M. Alvarez, D. Averill, A. R. Baden, J. Ballam, B. C. Barish, T. Barklow, B. A. Barnett, J. Bartelt, D. Blockus, W. De Boer, G. Bonvicini, C. Boswell, A. Boyarski, J. Boyer, B. Brabson, K. BrauneA. Breakstone, J. M. Brom, F. Bulos, P. R. Burchat, D. L. Burke, F. Butler, F. Calvino, R. J. Cence, J. Chapman, M. Chmeissani, D. Cords, D. P. Coupal, P. Dauncey, H. C. Destaebler, D. E. Dorfan, J. M. Dorfan, P. S. Drell, D. C. Drewer, J. Fay, G. J. Feldman, D. Fernandes, E. Fernandez, R. C. Field, W. T. Ford, C. Fordham, R. Frey, D. Fujino, K. K. Gan, C. Gatto, E. Gero, G. Gidal, T. Glanzman, G. Goldhaber, J. J. Gomez Cadenas, X. Gong, G. Gratta, A. Green, P. Grosse-Wiesmann, J. Haggerty, G. Hanson, R. Harr, B. Harral, F. A. Harris, C. M. Hawkes, K. Hayes, C. Hearty, D. Herrup, C. A. Heusch, T. Himel, D. A. Hinshaw, M. Hoenk, S. O. Holmgren, S. J. Hong, D. Hutchinson, J. Hylen, W. R. Innes, R. G. Jacobsen, M. Jaffre, J. A. Jaros, C. K. Jung, I. Juricic, J. A. Kadyk, D. Karlen, J. Kent, M. King, S. R. Klein, L. Koepke, D. Koetke, A. Koide, S. Komamiya, W. Koska, L. A. Kowalski, W. Kozanecki, J. F. Kral, M. Kuhlen, L. Labarga, A. J. Lankford, R. R. Larsen, M. E. Levi, Z. Li, A. M. Litke, V. Lüth, G. R. Lynch, J. A. McKenna, J. A.J. Matthews, T. Mattison, B. D. Milliken, K. C. Moffeit, L. Müller, C. T. Munger, W. N. Murray, J. Nash, M. E. Nelson, D. Nitz, H. Ogren, R. A. Ong, K. F. O'Shaughnessy, S. I. Parker, C. Peck, J. Perl, M. L. Perl, F. Perrier, A. Petersen, M. Petradza, R. Pitthan, F. C. Porter, P. Rankin, J. D. Richman, K. Riles, F. R. Rouse, D. R. Rust, H. F.W. Sadrozinski, M. W. Schaad, W. B. Schmidke, B. A. Schumm, A. S. Schwarz, A. Seiden, J. G. Smith, A. Snyder, E. Soderstrom, D. P. Stoker, R. Stroynowski, M. Swartz, R. E. Taylor, R. Thun, G. H. Trilling, R. Tschirhart, M. Turala, R. Van Kooten, S. Vejcik, H. Veltman, P. Voruganti, S. R. Wagner, S. Watson, P. Weber, A. Weigend, A. J. Weinstein, A. J. Weir, S. Weisz, S. L. White, E. Wicklund, R. C. Wolf, D. R. Wood, M. Woods, G. Wormser, R. Wright, D. Y. Wu, M. Yurko, C. Zaccardelli, C. Von Zanthier

^*この研究の対応する著者

研究成果: Article › 査読

30 被引用数 (Scopus)

抄録

The Mark II detector has been upgraded in preparation for its role as the first detector to take data at the Stanford Linear Collider. The new detector components include the central drift chamber, the time-of-flight system, the coil, the endcap electromagnetic calorimeters and the beam energy and luminosity measuring devices. There have also been improvements in detector hermeticity. All of the major components were installed for a test run at the PEP storage ring (√s = 29 GeV) in 1985. This paper describes the upgraded detector, including its trigger and data acquisition systems, and gives performance figures for its components. Future improvements are also discussed.

本文言語	English
ページ（範囲）	55-80
ページ数	26
ジャーナル	Nuclear Inst. and Methods in Physics Research, A
巻	281
号	1
DOI	https://doi.org/10.1016/0168-9002(89)91217-5
出版ステータス	Published - 1989 8月 20
外部発表	はい

ASJC Scopus subject areas

核物理学および高エネルギー物理学
器械工学

文献へのアクセス

10.1016/0168-9002(89)91217-5

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引用スタイル

Abrams, G., Adolphsen, C. E., Akerlof, C., Alexander, J. P., Alvarez, M., Averill, D., Baden, A. R., Ballam, J., Barish, B. C., Barklow, T., Barnett, B. A., Bartelt, J., Blockus, D., De Boer, W., Bonvicini, G., Boswell, C., Boyarski, A., Boyer, J., Brabson, B., ... Von Zanthier, C. (1989). The Mark II detector for the SLC. Nuclear Inst. and Methods in Physics Research, A, 281(1), 55-80. https://doi.org/10.1016/0168-9002(89)91217-5

Abrams, G, Adolphsen, CE, Akerlof, C, Alexander, JP, Alvarez, M, Averill, D, Baden, AR, Ballam, J, Barish, BC, Barklow, T, Barnett, BA, Bartelt, J, Blockus, D, De Boer, W, Bonvicini, G, Boswell, C, Boyarski, A, Boyer, J, Brabson, B, Braune, K, Breakstone, A, Brom, JM, Bulos, F, Burchat, PR, Burke, DL, Butler, F, Calvino, F, Cence, RJ, Chapman, J, Chmeissani, M, Cords, D, Coupal, DP, Dauncey, P, Destaebler, HC, Dorfan, DE, Dorfan, JM, Drell, PS, Drewer, DC, Fay, J, Feldman, GJ, Fernandes, D, Fernandez, E, Field, RC, Ford, WT, Fordham, C, Frey, R, Fujino, D, Gan, KK, Gatto, C, Gero, E, Gidal, G, Glanzman, T, Goldhaber, G, Gomez Cadenas, JJ, Gong, X, Gratta, G, Green, A, Grosse-Wiesmann, P, Haggerty, J, Hanson, G, Harr, R, Harral, B, Harris, FA, Hawkes, CM, Hayes, K, Hearty, C, Herrup, D, Heusch, CA, Himel, T, Hinshaw, DA, Hoenk, M, Holmgren, SO, Hong, SJ, Hutchinson, D, Hylen, J, Innes, WR, Jacobsen, RG, Jaffre, M, Jaros, JA, Jung, CK, Juricic, I, Kadyk, JA, Karlen, D, Kent, J, King, M, Klein, SR, Koepke, L, Koetke, D, Koide, A, Komamiya, S, Koska, W, Kowalski, LA, Kozanecki, W, Kral, JF, Kuhlen, M, Labarga, L, Lankford, AJ, Larsen, RR, Levi, ME, Li, Z, Litke, AM, Lüth, V, Lynch, GR, McKenna, JA, Matthews, JAJ, Mattison, T, Milliken, BD, Moffeit, KC, Müller, L, Munger, CT, Murray, WN, Nash, J, Nelson, ME, Nitz, D, Ogren, H, Ong, RA, O'Shaughnessy, KF, Parker, SI, Peck, C, Perl, J, Perl, ML, Perrier, F, Petersen, A, Petradza, M, Pitthan, R, Porter, FC, Rankin, P, Richman, JD, Riles, K, Rouse, FR, Rust, DR, Sadrozinski, HFW, Schaad, MW, Schmidke, WB, Schumm, BA, Schwarz, AS, Seiden, A, Smith, JG, Snyder, A, Soderstrom, E, Stoker, DP, Stroynowski, R, Swartz, M, Taylor, RE, Thun, R, Trilling, GH, Tschirhart, R, Turala, M, Van Kooten, R, Vejcik, S, Veltman, H, Voruganti, P, Wagner, SR, Watson, S, Weber, P, Weigend, A, Weinstein, AJ, Weir, AJ, Weisz, S, White, SL, Wicklund, E, Wolf, RC, Wood, DR, Woods, M, Wormser, G, Wright, R, Wu, DY, Yurko, M, Zaccardelli, C & Von Zanthier, C 1989, 'The Mark II detector for the SLC', Nuclear Inst. and Methods in Physics Research, A, vol. 281, no. 1, pp. 55-80. https://doi.org/10.1016/0168-9002(89)91217-5

@article{7ca2f232bc3c43df98ba4cd7c1de5159,

title = "The Mark II detector for the SLC",

abstract = "The Mark II detector has been upgraded in preparation for its role as the first detector to take data at the Stanford Linear Collider. The new detector components include the central drift chamber, the time-of-flight system, the coil, the endcap electromagnetic calorimeters and the beam energy and luminosity measuring devices. There have also been improvements in detector hermeticity. All of the major components were installed for a test run at the PEP storage ring (√s = 29 GeV) in 1985. This paper describes the upgraded detector, including its trigger and data acquisition systems, and gives performance figures for its components. Future improvements are also discussed.",

author = "G. Abrams and Adolphsen, {C. E.} and C. Akerlof and Alexander, {J. P.} and M. Alvarez and D. Averill and Baden, {A. R.} and J. Ballam and Barish, {B. C.} and T. Barklow and Barnett, {B. A.} and J. Bartelt and D. Blockus and {De Boer}, W. and G. Bonvicini and C. Boswell and A. Boyarski and J. Boyer and B. Brabson and K. Braune and A. Breakstone and Brom, {J. M.} and F. Bulos and Burchat, {P. R.} and Burke, {D. L.} and F. Butler and F. Calvino and Cence, {R. J.} and J. Chapman and M. Chmeissani and D. Cords and Coupal, {D. P.} and P. Dauncey and Destaebler, {H. C.} and Dorfan, {D. E.} and Dorfan, {J. M.} and Drell, {P. S.} and Drewer, {D. C.} and J. Fay and Feldman, {G. J.} and D. Fernandes and E. Fernandez and Field, {R. C.} and Ford, {W. T.} and C. Fordham and R. Frey and D. Fujino and Gan, {K. K.} and C. Gatto and E. Gero and G. Gidal and T. Glanzman and G. Goldhaber and {Gomez Cadenas}, {J. J.} and X. Gong and G. Gratta and A. Green and P. Grosse-Wiesmann and J. Haggerty and G. Hanson and R. Harr and B. Harral and Harris, {F. A.} and Hawkes, {C. M.} and K. Hayes and C. Hearty and D. Herrup and Heusch, {C. A.} and T. Himel and Hinshaw, {D. A.} and M. Hoenk and Holmgren, {S. O.} and Hong, {S. J.} and D. Hutchinson and J. Hylen and Innes, {W. R.} and Jacobsen, {R. G.} and M. Jaffre and Jaros, {J. A.} and Jung, {C. K.} and I. Juricic and Kadyk, {J. A.} and D. Karlen and J. Kent and M. King and Klein, {S. R.} and L. Koepke and D. Koetke and A. Koide and S. Komamiya and W. Koska and Kowalski, {L. A.} and W. Kozanecki and Kral, {J. F.} and M. Kuhlen and L. Labarga and Lankford, {A. J.} and Larsen, {R. R.} and Levi, {M. E.} and Z. Li and Litke, {A. M.} and V. L{\"u}th and Lynch, {G. R.} and McKenna, {J. A.} and Matthews, {J. A.J.} and T. Mattison and Milliken, {B. D.} and Moffeit, {K. C.} and L. M{\"u}ller and Munger, {C. T.} and Murray, {W. N.} and J. Nash and Nelson, {M. E.} and D. Nitz and H. Ogren and Ong, {R. A.} and O'Shaughnessy, {K. F.} and Parker, {S. I.} and C. Peck and J. Perl and Perl, {M. L.} and F. Perrier and A. Petersen and M. Petradza and R. Pitthan and Porter, {F. C.} and P. Rankin and Richman, {J. D.} and K. Riles and Rouse, {F. R.} and Rust, {D. R.} and Sadrozinski, {H. F.W.} and Schaad, {M. W.} and Schmidke, {W. B.} and Schumm, {B. A.} and Schwarz, {A. S.} and A. Seiden and Smith, {J. G.} and A. Snyder and E. Soderstrom and Stoker, {D. P.} and R. Stroynowski and M. Swartz and Taylor, {R. E.} and R. Thun and Trilling, {G. H.} and R. Tschirhart and M. Turala and {Van Kooten}, R. and S. Vejcik and H. Veltman and P. Voruganti and Wagner, {S. R.} and S. Watson and P. Weber and A. Weigend and Weinstein, {A. J.} and Weir, {A. J.} and S. Weisz and White, {S. L.} and E. Wicklund and Wolf, {R. C.} and Wood, {D. R.} and M. Woods and G. Wormser and R. Wright and Wu, {D. Y.} and M. Yurko and C. Zaccardelli and {Von Zanthier}, C.",

note = "Funding Information: There are many people who have contributed to the design, construction and operation of the Mark II detector over the past 12 years. The fact that several components of the original detector built at SPEAR are in use today is a tribute to the skill of those involved . We gratefully acknowledge all of the physicists, engineers and technicians who have helped us over the years. We also wish to acknowledge the important contributions of the following people to the design and engineering studies leading to the successful upgrade of the Mark II detector: R. Baggs, D. Bernstein, L. Barker, K. Bouldin, H. Brafman, D. Briggs, R. Cooper, D. Day, B. Denton, S. Dyer, R. Fuzesy, B. Gray, J. Hanson, C. Hoard, D. Horelick, R. Home, N. Hower, R. Jared, F. Kirsten, M. LaTeur, J. Mann, J. Mark, B. Martin, K. Mirk, T. Nakashima, W. Nilsson, J. Olsen, E. Ordinario, L. Paffrath, W. Pope, D. Porat, H. Rogers, W. Rowe, R. Stickley, M. Studzinski, Y.-Y. Sung, J. Tinsman, T. Walker, K. Warfield, and T. Webster. Several of us are supported by outside foundations. M.W . Schaad acknowledges the support received from the Swiss National Science Foundation . G. Gratta acknowledges the Italian INFN for their support. J.J. Gomez Cadenas and L. Labarga thank the Fulbright Foundation. M. Kuhlen acknowledges the Alexander von Humboldt Foundation for its support. This work was supported in part by Department of Energy contracts DE-AC03-81ER40050 (CIT), DE-AM03-76SF00010 (UCSC), DE-AC02-86ER40253 (Colorado), DE-AC03-83ER40103 (Hawaii), DE-AC02-84-ER40125 (Indiana), DE-AC03-76SF00098 (LBL), DE-AC02-84ER40125 (Michigan), and DE-AC03-76SF00515 (SLAC) ; and by the National Science Foundation (Johns Hopkins) .",

year = "1989",

month = aug,

day = "20",

doi = "10.1016/0168-9002(89)91217-5",

language = "English",

volume = "281",

pages = "55--80",

journal = "Nuclear Inst. and Methods in Physics Research, A",

issn = "0168-9002",

publisher = "Elsevier",

number = "1",

}

TY - JOUR

T1 - The Mark II detector for the SLC

AU - Abrams, G.

AU - Adolphsen, C. E.

AU - Akerlof, C.

AU - Alexander, J. P.

AU - Alvarez, M.

AU - Averill, D.

AU - Baden, A. R.

AU - Ballam, J.

AU - Barish, B. C.

AU - Barklow, T.

AU - Barnett, B. A.

AU - Bartelt, J.

AU - Blockus, D.

AU - De Boer, W.

AU - Bonvicini, G.

AU - Boswell, C.

AU - Boyarski, A.

AU - Boyer, J.

AU - Brabson, B.

AU - Braune, K.

AU - Breakstone, A.

AU - Brom, J. M.

AU - Bulos, F.

AU - Burchat, P. R.

AU - Burke, D. L.

AU - Butler, F.

AU - Calvino, F.

AU - Cence, R. J.

AU - Chapman, J.

AU - Chmeissani, M.

AU - Cords, D.

AU - Coupal, D. P.

AU - Dauncey, P.

AU - Destaebler, H. C.

AU - Dorfan, D. E.

AU - Dorfan, J. M.

AU - Drell, P. S.

AU - Drewer, D. C.

AU - Fay, J.

AU - Feldman, G. J.

AU - Fernandes, D.

AU - Fernandez, E.

AU - Field, R. C.

AU - Ford, W. T.

AU - Fordham, C.

AU - Frey, R.

AU - Fujino, D.

AU - Gan, K. K.

AU - Gatto, C.

AU - Gero, E.

AU - Gidal, G.

AU - Glanzman, T.

AU - Goldhaber, G.

AU - Gomez Cadenas, J. J.

AU - Gong, X.

AU - Gratta, G.

AU - Green, A.

AU - Grosse-Wiesmann, P.

AU - Haggerty, J.

AU - Hanson, G.

AU - Harr, R.

AU - Harral, B.

AU - Harris, F. A.

AU - Hawkes, C. M.

AU - Hayes, K.

AU - Hearty, C.

AU - Herrup, D.

AU - Heusch, C. A.

AU - Himel, T.

AU - Hinshaw, D. A.

AU - Hoenk, M.

AU - Holmgren, S. O.

AU - Hong, S. J.

AU - Hutchinson, D.

AU - Hylen, J.

AU - Innes, W. R.

AU - Jacobsen, R. G.

AU - Jaffre, M.

AU - Jaros, J. A.

AU - Jung, C. K.

AU - Juricic, I.

AU - Kadyk, J. A.

AU - Karlen, D.

AU - Kent, J.

AU - King, M.

AU - Klein, S. R.

AU - Koepke, L.

AU - Koetke, D.

AU - Koide, A.

AU - Komamiya, S.

AU - Koska, W.

AU - Kowalski, L. A.

AU - Kozanecki, W.

AU - Kral, J. F.

AU - Kuhlen, M.

AU - Labarga, L.

AU - Lankford, A. J.

AU - Larsen, R. R.

AU - Levi, M. E.

AU - Li, Z.

AU - Litke, A. M.

AU - Lüth, V.

AU - Lynch, G. R.

AU - McKenna, J. A.

AU - Matthews, J. A.J.

AU - Mattison, T.

AU - Milliken, B. D.

AU - Moffeit, K. C.

AU - Müller, L.

AU - Munger, C. T.

AU - Murray, W. N.

AU - Nash, J.

AU - Nelson, M. E.

AU - Nitz, D.

AU - Ogren, H.

AU - Ong, R. A.

AU - O'Shaughnessy, K. F.

AU - Parker, S. I.

AU - Peck, C.

AU - Perl, J.

AU - Perl, M. L.

AU - Perrier, F.

AU - Petersen, A.

AU - Petradza, M.

AU - Pitthan, R.

AU - Porter, F. C.

AU - Rankin, P.

AU - Richman, J. D.

AU - Riles, K.

AU - Rouse, F. R.

AU - Rust, D. R.

AU - Sadrozinski, H. F.W.

AU - Schaad, M. W.

AU - Schmidke, W. B.

AU - Schumm, B. A.

AU - Schwarz, A. S.

AU - Seiden, A.

AU - Smith, J. G.

AU - Snyder, A.

AU - Soderstrom, E.

AU - Stoker, D. P.

AU - Stroynowski, R.

AU - Swartz, M.

AU - Taylor, R. E.

AU - Thun, R.

AU - Trilling, G. H.

AU - Tschirhart, R.

AU - Turala, M.

AU - Van Kooten, R.

AU - Vejcik, S.

AU - Veltman, H.

AU - Voruganti, P.

AU - Wagner, S. R.

AU - Watson, S.

AU - Weber, P.

AU - Weigend, A.

AU - Weinstein, A. J.

AU - Weir, A. J.

AU - Weisz, S.

AU - White, S. L.

AU - Wicklund, E.

AU - Wolf, R. C.

AU - Wood, D. R.

AU - Woods, M.

AU - Wormser, G.

AU - Wright, R.

AU - Wu, D. Y.

AU - Yurko, M.

AU - Zaccardelli, C.

AU - Von Zanthier, C.

N1 - Funding Information: There are many people who have contributed to the design, construction and operation of the Mark II detector over the past 12 years. The fact that several components of the original detector built at SPEAR are in use today is a tribute to the skill of those involved . We gratefully acknowledge all of the physicists, engineers and technicians who have helped us over the years. We also wish to acknowledge the important contributions of the following people to the design and engineering studies leading to the successful upgrade of the Mark II detector: R. Baggs, D. Bernstein, L. Barker, K. Bouldin, H. Brafman, D. Briggs, R. Cooper, D. Day, B. Denton, S. Dyer, R. Fuzesy, B. Gray, J. Hanson, C. Hoard, D. Horelick, R. Home, N. Hower, R. Jared, F. Kirsten, M. LaTeur, J. Mann, J. Mark, B. Martin, K. Mirk, T. Nakashima, W. Nilsson, J. Olsen, E. Ordinario, L. Paffrath, W. Pope, D. Porat, H. Rogers, W. Rowe, R. Stickley, M. Studzinski, Y.-Y. Sung, J. Tinsman, T. Walker, K. Warfield, and T. Webster. Several of us are supported by outside foundations. M.W . Schaad acknowledges the support received from the Swiss National Science Foundation . G. Gratta acknowledges the Italian INFN for their support. J.J. Gomez Cadenas and L. Labarga thank the Fulbright Foundation. M. Kuhlen acknowledges the Alexander von Humboldt Foundation for its support. This work was supported in part by Department of Energy contracts DE-AC03-81ER40050 (CIT), DE-AM03-76SF00010 (UCSC), DE-AC02-86ER40253 (Colorado), DE-AC03-83ER40103 (Hawaii), DE-AC02-84-ER40125 (Indiana), DE-AC03-76SF00098 (LBL), DE-AC02-84ER40125 (Michigan), and DE-AC03-76SF00515 (SLAC) ; and by the National Science Foundation (Johns Hopkins) .

PY - 1989/8/20

Y1 - 1989/8/20

N2 - The Mark II detector has been upgraded in preparation for its role as the first detector to take data at the Stanford Linear Collider. The new detector components include the central drift chamber, the time-of-flight system, the coil, the endcap electromagnetic calorimeters and the beam energy and luminosity measuring devices. There have also been improvements in detector hermeticity. All of the major components were installed for a test run at the PEP storage ring (√s = 29 GeV) in 1985. This paper describes the upgraded detector, including its trigger and data acquisition systems, and gives performance figures for its components. Future improvements are also discussed.

AB - The Mark II detector has been upgraded in preparation for its role as the first detector to take data at the Stanford Linear Collider. The new detector components include the central drift chamber, the time-of-flight system, the coil, the endcap electromagnetic calorimeters and the beam energy and luminosity measuring devices. There have also been improvements in detector hermeticity. All of the major components were installed for a test run at the PEP storage ring (√s = 29 GeV) in 1985. This paper describes the upgraded detector, including its trigger and data acquisition systems, and gives performance figures for its components. Future improvements are also discussed.

UR - http://www.scopus.com/inward/record.url?scp=0024715377&partnerID=8YFLogxK

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U2 - 10.1016/0168-9002(89)91217-5

DO - 10.1016/0168-9002(89)91217-5

M3 - Article

AN - SCOPUS:0024715377

SN - 0168-9002

VL - 281

SP - 55

EP - 80

JO - Nuclear Inst. and Methods in Physics Research, A

JF - Nuclear Inst. and Methods in Physics Research, A

IS - 1

ER -

The Mark II detector for the SLC

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