A high resolution imaging detector for TeV gamma-ray astronomy
Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Cawley, M. F. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
1990 |
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| Schlagwörter: |
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| Anmerkung: |
© Kluwer Academic Publishers 1990 |
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| Übergeordnetes Werk: |
Enthalten in: Experimental astronomy - Kluwer Academic Publishers, 1989, 1(1990), 3 vom: Mai, Seite 173-193 |
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| Übergeordnetes Werk: |
volume:1 ; year:1990 ; number:3 ; month:05 ; pages:173-193 |
| Links: |
|---|
| DOI / URN: |
10.1007/BF00462039 |
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| Katalog-ID: |
OLC2042935980 |
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| 245 | 1 | 0 | |a A high resolution imaging detector for TeV gamma-ray astronomy |
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| 520 | |a Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. | ||
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| 700 | 1 | |a Fegan, D. J. |4 aut | |
| 700 | 1 | |a Harris, K. |4 aut | |
| 700 | 1 | |a Hillas, A. M. |4 aut | |
| 700 | 1 | |a Kwok, P. W. |4 aut | |
| 700 | 1 | |a Lamb, R. C. |4 aut | |
| 700 | 1 | |a Lang, M. J. |4 aut | |
| 700 | 1 | |a Lewis, D. A. |4 aut | |
| 700 | 1 | |a Macomb, D. |4 aut | |
| 700 | 1 | |a Reynolds, P. T. |4 aut | |
| 700 | 1 | |a Schmid, D. J. |4 aut | |
| 700 | 1 | |a Vacanti, G. |4 aut | |
| 700 | 1 | |a Weekes, T. C. |4 aut | |
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10.1007/BF00462039 doi (DE-627)OLC2042935980 (DE-He213)BF00462039-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Cawley, M. F. verfasserin aut A high resolution imaging detector for TeV gamma-ray astronomy 1990 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1990 Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. High Resolution Resolution Imaging Photomultiplier Tube High Resolution Imaging Imaging Detector Fegan, D. J. aut Harris, K. aut Hillas, A. M. aut Kwok, P. W. aut Lamb, R. C. aut Lang, M. J. aut Lewis, D. A. aut Macomb, D. aut Reynolds, P. T. aut Schmid, D. J. aut Vacanti, G. aut Weekes, T. C. aut Enthalten in Experimental astronomy Kluwer Academic Publishers, 1989 1(1990), 3 vom: Mai, Seite 173-193 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:1 year:1990 number:3 month:05 pages:173-193 https://doi.org/10.1007/BF00462039 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2012 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 39.00 VZ AR 1 1990 3 05 173-193 |
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10.1007/BF00462039 doi (DE-627)OLC2042935980 (DE-He213)BF00462039-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Cawley, M. F. verfasserin aut A high resolution imaging detector for TeV gamma-ray astronomy 1990 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1990 Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. High Resolution Resolution Imaging Photomultiplier Tube High Resolution Imaging Imaging Detector Fegan, D. J. aut Harris, K. aut Hillas, A. M. aut Kwok, P. W. aut Lamb, R. C. aut Lang, M. J. aut Lewis, D. A. aut Macomb, D. aut Reynolds, P. T. aut Schmid, D. J. aut Vacanti, G. aut Weekes, T. C. aut Enthalten in Experimental astronomy Kluwer Academic Publishers, 1989 1(1990), 3 vom: Mai, Seite 173-193 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:1 year:1990 number:3 month:05 pages:173-193 https://doi.org/10.1007/BF00462039 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2012 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 39.00 VZ AR 1 1990 3 05 173-193 |
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10.1007/BF00462039 doi (DE-627)OLC2042935980 (DE-He213)BF00462039-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Cawley, M. F. verfasserin aut A high resolution imaging detector for TeV gamma-ray astronomy 1990 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1990 Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. High Resolution Resolution Imaging Photomultiplier Tube High Resolution Imaging Imaging Detector Fegan, D. J. aut Harris, K. aut Hillas, A. M. aut Kwok, P. W. aut Lamb, R. C. aut Lang, M. J. aut Lewis, D. A. aut Macomb, D. aut Reynolds, P. T. aut Schmid, D. J. aut Vacanti, G. aut Weekes, T. C. aut Enthalten in Experimental astronomy Kluwer Academic Publishers, 1989 1(1990), 3 vom: Mai, Seite 173-193 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:1 year:1990 number:3 month:05 pages:173-193 https://doi.org/10.1007/BF00462039 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2012 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 39.00 VZ AR 1 1990 3 05 173-193 |
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10.1007/BF00462039 doi (DE-627)OLC2042935980 (DE-He213)BF00462039-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Cawley, M. F. verfasserin aut A high resolution imaging detector for TeV gamma-ray astronomy 1990 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1990 Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. High Resolution Resolution Imaging Photomultiplier Tube High Resolution Imaging Imaging Detector Fegan, D. J. aut Harris, K. aut Hillas, A. M. aut Kwok, P. W. aut Lamb, R. C. aut Lang, M. J. aut Lewis, D. A. aut Macomb, D. aut Reynolds, P. T. aut Schmid, D. J. aut Vacanti, G. aut Weekes, T. C. aut Enthalten in Experimental astronomy Kluwer Academic Publishers, 1989 1(1990), 3 vom: Mai, Seite 173-193 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:1 year:1990 number:3 month:05 pages:173-193 https://doi.org/10.1007/BF00462039 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2012 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 39.00 VZ AR 1 1990 3 05 173-193 |
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10.1007/BF00462039 doi (DE-627)OLC2042935980 (DE-He213)BF00462039-p DE-627 ger DE-627 rakwb eng 520 530 VZ 16,12 ssgn 39.00 bkl Cawley, M. F. verfasserin aut A high resolution imaging detector for TeV gamma-ray astronomy 1990 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Kluwer Academic Publishers 1990 Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. High Resolution Resolution Imaging Photomultiplier Tube High Resolution Imaging Imaging Detector Fegan, D. J. aut Harris, K. aut Hillas, A. M. aut Kwok, P. W. aut Lamb, R. C. aut Lang, M. J. aut Lewis, D. A. aut Macomb, D. aut Reynolds, P. T. aut Schmid, D. J. aut Vacanti, G. aut Weekes, T. C. aut Enthalten in Experimental astronomy Kluwer Academic Publishers, 1989 1(1990), 3 vom: Mai, Seite 173-193 (DE-627)130767123 (DE-600)1001704-5 (DE-576)023036176 0922-6435 nnns volume:1 year:1990 number:3 month:05 pages:173-193 https://doi.org/10.1007/BF00462039 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OLC-AST SSG-OPC-AST GBV_ILN_11 GBV_ILN_22 GBV_ILN_31 GBV_ILN_40 GBV_ILN_47 GBV_ILN_70 GBV_ILN_2002 GBV_ILN_2012 GBV_ILN_4012 GBV_ILN_4046 GBV_ILN_4082 GBV_ILN_4103 GBV_ILN_4306 GBV_ILN_4700 39.00 VZ AR 1 1990 3 05 173-193 |
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Cawley, M. F. @@aut@@ Fegan, D. J. @@aut@@ Harris, K. @@aut@@ Hillas, A. M. @@aut@@ Kwok, P. W. @@aut@@ Lamb, R. C. @@aut@@ Lang, M. J. @@aut@@ Lewis, D. A. @@aut@@ Macomb, D. @@aut@@ Reynolds, P. T. @@aut@@ Schmid, D. J. @@aut@@ Vacanti, G. @@aut@@ Weekes, T. C. @@aut@@ |
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Cawley, M. F. |
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520 530 VZ 16,12 ssgn 39.00 bkl A high resolution imaging detector for TeV gamma-ray astronomy High Resolution Resolution Imaging Photomultiplier Tube High Resolution Imaging Imaging Detector |
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ddc 520 ssgn 16,12 bkl 39.00 misc High Resolution misc Resolution Imaging misc Photomultiplier Tube misc High Resolution Imaging misc Imaging Detector |
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A high resolution imaging detector for TeV gamma-ray astronomy |
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A high resolution imaging detector for TeV gamma-ray astronomy |
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Cawley, M. F. |
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Experimental astronomy |
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1990 |
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Cawley, M. F. Fegan, D. J. Harris, K. Hillas, A. M. Kwok, P. W. Lamb, R. C. Lang, M. J. Lewis, D. A. Macomb, D. Reynolds, P. T. Schmid, D. J. Vacanti, G. Weekes, T. C. |
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Cawley, M. F. |
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10.1007/BF00462039 |
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520 530 |
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a high resolution imaging detector for tev gamma-ray astronomy |
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A high resolution imaging detector for TeV gamma-ray astronomy |
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Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. © Kluwer Academic Publishers 1990 |
| abstractGer |
Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. © Kluwer Academic Publishers 1990 |
| abstract_unstemmed |
Abstract Details are presented of an atmospheric Cherenkov telescope for use in very high energy gamma-ray astronomy which consists of a cluster of 109 close-packed photomultiplier tubes at the focus of a 10 meter optical reflector. The images of the Cherenkov flashes generated both by gamma-ray and charged cosmic-ray events are digitized and recorded. Subsequent off-line analysis of the images improves the significance of the signal to noise ratio by a factor of 10 compared with non-imaging techniques. © Kluwer Academic Publishers 1990 |
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A high resolution imaging detector for TeV gamma-ray astronomy |
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https://doi.org/10.1007/BF00462039 |
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Fegan, D. J. Harris, K. Hillas, A. M. Kwok, P. W. Lamb, R. C. Lang, M. J. Lewis, D. A. Macomb, D. Reynolds, P. T. Schmid, D. J. Vacanti, G. Weekes, T. C. |
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Fegan, D. J. Harris, K. Hillas, A. M. Kwok, P. W. Lamb, R. C. Lang, M. J. Lewis, D. A. Macomb, D. Reynolds, P. T. Schmid, D. J. Vacanti, G. Weekes, T. C. |
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