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@ARTICLE{Acharyya:599007,
      author       = {Acharyya, Atreya and Adams, Colin and Archer, Avery and
                      Bangale, Priyadarshini and Batista, Pedro and Benbow, Wystan
                      and Brill, Aryeh and Capasso, M. and Errando, Manel and
                      Falcone, Abraham and Feng, Qi and Finley, John and Foote,
                      Gregory and Fortson, Lucy and Furniss, Amy and Griffin, Sean
                      and Hanlon, William and Hanna, David and Hervet, Olivier and
                      Hinrichs, Claire and Hoang, John and Holder, Jamie and
                      Humensky, T. B. and Jin, Weidong and Kaaret, Philip and
                      Kertzman, Mary P. and Kherlakian, Maria and Kieda, David and
                      Kleiner, Tobias and Korzoun, Nikolas and Kumar, Sajan and
                      Lang, Mark and Lundy, Matthew and Maier, Gernot and McGrath,
                      Conor and Millard, Matthew and Miller, Hayden and Millis,
                      John and Mooney, Connor and Moriarty, Patrick and Mukherjee,
                      Reshmi and O'Brien, Stephan and Ong, Rene A. and Pohl,
                      Martin and Pueschel, Elisa and Quinn, John and Ragan,
                      Kenneth J. and Reynolds, Paul and Ribeiro, Deivid and
                      Roache, Emmet Thomas and Ryan, Jamie and Sadeh, Iftach and
                      Saha, Lab and Santander, Marcos and Sembroski, Glenn H. and
                      Shang, Ruo and Tak, Donggeun and Talluri, Anjana and Tucci,
                      James and Vazquez, Nico and Williams, David and Wong, S. L.
                      and Woo, Jooyun and DeBoer, David and Isaacson, Howard and
                      de Pater, Imke and Price, Danny and Siemion, Andrew},
      collaboration = {{VERITAS Collaboration}},
      title        = {{A} {VERITAS}/{B}reakthrough {L}isten {S}earch for
                      {O}ptical {T}echnosignatures},
      journal      = {The astronomical journal},
      volume       = {166},
      number       = {3},
      issn         = {0004-6256},
      address      = {Chicago, Ill.},
      publisher    = {Univ. of Chicago Press, Journals Division},
      reportid     = {PUBDB-2023-07091, arXiv:2306.17680},
      pages        = {84},
      year         = {2023},
      note         = {ISSN 1538-3881 not unique: **2 hits**.15 pages, 7 figures},
      abstract     = {The Breakthrough Listen Initiative is conducting a program
                      using multiple telescopes around the world to search for
                      “technosignatures”: artificial transmitters of
                      extraterrestrial origin from beyond our solar system. The
                      Very Energetic Radiation Imaging Telescope Array System
                      (VERITAS) Collaboration joined this program in 2018 and
                      provides the capability to search for one particular
                      technosignature: optical pulses of a few nanoseconds in
                      duration detectable over interstellar distances. We report
                      here on the analysis and results of dedicated VERITAS
                      observations of Breakthrough Listen targets conducted in
                      2019 and 2020 and of archival VERITAS data collected since
                      2012. Thirty hours of dedicated observations of 136 targets
                      and 249 archival observations of 140 targets were analyzed
                      and did not reveal any signals consistent with a
                      technosignature. The results are used to place limits on the
                      fraction of stars hosting transmitting civilizations. We
                      also discuss the minimum pulse sensitivity of our
                      observations and present VERITAS observations of CALIOP: a
                      space-based pulsed laser on board the Cloud-Aerosol Lidar
                      and Infrared Pathfinder Satellite Observations. The
                      detection of these pulses with VERITAS, using the analysis
                      techniques developed for our technosignature search, allows
                      a test of our analysis efficiency and serves as an important
                      proof of principle.},
      cin          = {$Z_CTA$ / $Z_VER$},
      ddc          = {520},
      cid          = {$I:(DE-H253)Z_CTA-20210408$ / $I:(DE-H253)Z_VER-20210408$},
      pnm          = {613 - Matter and Radiation from the Universe (POF4-613)},
      pid          = {G:(DE-HGF)POF4-613},
      experiment   = {EXP:(DE-H253)CTA-20150101 / EXP:(DE-H253)VERITAS-20170101},
      typ          = {PUB:(DE-HGF)16},
      eprint       = {2306.17680},
      howpublished = {arXiv:2306.17680},
      archivePrefix = {arXiv},
      SLACcitation = {$\%\%CITATION$ = $arXiv:2306.17680;\%\%$},
      UT           = {WOS:001041274700001},
      doi          = {10.3847/1538-3881/ace347},
      url          = {https://bib-pubdb1.desy.de/record/599007},
}