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@ARTICLE{Adams:455779,
      author       = {Adams, C. B. and Alfaro, R. and Ambrosi, G. and Ambrosio,
                      M. and Aramo, C. and Arlen, T. and Batista, P. I. and
                      Benbow, W. and Bertucci, B. and Bissaldi, E. and Biteau, J.
                      and Bitossi, M. and Boiano, A. and Bonavolontà, C. and
                      Bose, R. and Bouvier, A. and Brill, A. and Brown, A. M. and
                      Buckley, J. H. and Byrum, K. and Cameron, R. A. and
                      Canestrari, R. and Capasso, M. and Caprai, M. and Covault,
                      C. E. and Depaoli, D. and Errando, M. and Fegan, S. and
                      Feng, Q. and Fiandrini, E. and Foote, G. and Fortin, P. and
                      Funk, S. and Furniss, A. and Garfias, F. and Gent, A. and
                      Giglietto, N. and Giordano, F. and Giro, E. and González,
                      M. M. and Guarino, V. and Halliday, R. and Hervet, O. and
                      Holder, J. and Hughes, G. and Humensky, T. B. and Ionica, M.
                      and Iriarte, A. and Jin, W. and Johnson, C. A. and Kaaret,
                      P. and Kieda, D. and Kim, B. and Kuznetsov, A. and
                      Lapington, J. S. and Licciulli, F. and Loporchio, S. and
                      Masone, V. and Meagher, K. and Meures, T. and Mode, B. A. W.
                      and Mognet, S. A. I. and Mukherjee, R. and Nguyen, T. and
                      Nieto, D. and Okumura, A. and Otte, N. and La Palombara, N.
                      and Pantaleo, F. R. and Paoletti, R. and Pareschi, G. and
                      Petrashyk, A. and Di Pierro, F. and Pueschel, Elisa and
                      Reynolds, P. T. and Ribeiro, D. and Richards, G. and Roache,
                      E. and Ross, D. and Rousselle, J. and Rugliancich, A. and
                      Ruíz-Díaz-Soto, J. and Santander, M. and Schlenstedt,
                      Stefan and Schneider, M. and Scuderi, S. and Shang, R. and
                      Sironi, G. and Stevenson, B. and Stiaccini, L. and Tajima,
                      H. and Taylor, L. P. and Thornhill, J. and Tosti, L. and
                      Tovmassian, G. and Vagelli, V. and Valentino, M. and
                      Vandenbroucke, J. and Vassiliev, V. V. and Di Venere, L. and
                      Wakely, S. P. and Watson, J. J. and White, R. and Wilcox, P.
                      and Williams, D. A. and Wood, M. and Yu, P. and Zink, A.},
      title        = {{D}etection of the {C}rab {N}ebula with the 9.7 m
                      prototype {S}chwarzschild-{C}ouder telescope},
      journal      = {Astroparticle physics},
      volume       = {128},
      issn         = {0927-6505},
      address      = {Amsterdam [u.a.]},
      publisher    = {Elsevier Science},
      reportid     = {PUBDB-2021-01213, arXiv:2012.08448},
      pages        = {102562},
      year         = {2021},
      note         = {13 pages, 12 figures, 3 tableskein journal fulltext trotz
                      Anfrage, nur arXiv Waiting for fulltext},
      abstract     = {The Schwarzschild-Couder Telescope (SCT) is a telescope
                      concept proposed for the Cherenkov Telescope Array. It
                      employs a dual-mirror optical design to remove comatic
                      aberrations over an 8∘ field of view, and a high-density
                      silicon photomultiplier camera (with a pixel resolution of
                      4 arcmin) to record Cherenkov emission from cosmic ray and
                      gamma-ray initiated particle cascades in the atmosphere. The
                      prototype SCT (pSCT), comprising a 9.7 m diameter primary
                      mirror and a partially instrumented camera with
                      1536 pixels, has been constructed at the Fred Lawrence
                      Whipple Observatory. The telescope was inaugurated in
                      January 2019, with commissioning continuing throughout 2019.
                      We describe the first campaign of observations with the
                      pSCT, conducted in January and February of 2020, and
                      demonstrate the detection of gamma-ray emission from the
                      Crab Nebula with a statistical significance of 8.6σ .},
      keywords     = {gamma ray: emission (INSPIRE) / photomultiplier: silicon
                      (INSPIRE) / pixel (INSPIRE) / Cherenkov Telescope Array
                      (INSPIRE) / cosmic radiation (INSPIRE) / observatory
                      (INSPIRE) / statistical (INSPIRE) / atmosphere (INSPIRE) /
                      aberration (INSPIRE) / resolution (INSPIRE) / radiation:
                      Cherenkov (INSPIRE) / cascade (INSPIRE) / optical (INSPIRE)
                      / mirror (INSPIRE)},
      cin          = {ZEU-CTA},
      ddc          = {540},
      cid          = {I:(DE-H253)ZEU-CTA-20120731},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)CTA-20150101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2012.08448},
      howpublished = {arXiv:2012.08448},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2012.08448;\%\%$},
      UT           = {WOS:000621632600012},
      doi          = {10.1016/j.astropartphys.2021.102562},
      url          = {https://bib-pubdb1.desy.de/record/455779},
}