000599007 001__ 599007
000599007 005__ 20250724132454.0
000599007 0247_ $$2doi$$a10.3847/1538-3881/ace347
000599007 0247_ $$2INSPIRETeX$$aVERITAS:2023kim
000599007 0247_ $$2inspire$$ainspire:2673686
000599007 0247_ $$2ISSN$$a0004-6256
000599007 0247_ $$2ISSN$$a1538-3881
000599007 0247_ $$2arXiv$$aarXiv:2306.17680
000599007 0247_ $$2datacite_doi$$a10.3204/PUBDB-2023-07091
000599007 0247_ $$2WOS$$aWOS:001041274700001
000599007 0247_ $$2altmetric$$aaltmetric:150918597
000599007 0247_ $$2openalex$$aopenalex:W4385460139
000599007 037__ $$aPUBDB-2023-07091
000599007 041__ $$aEnglish
000599007 082__ $$a520
000599007 088__ $$2arXiv$$aarXiv:2306.17680
000599007 1001_ $$00000-0002-2028-9230$$aAcharyya, Atreya$$b0
000599007 245__ $$aA VERITAS/Breakthrough Listen Search for Optical Technosignatures
000599007 260__ $$aChicago, Ill.$$bUniv. of Chicago Press, Journals Division$$c2023
000599007 3367_ $$2DRIVER$$aarticle
000599007 3367_ $$2DataCite$$aOutput Types/Journal article
000599007 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1704808382_313859
000599007 3367_ $$2BibTeX$$aARTICLE
000599007 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000599007 3367_ $$00$$2EndNote$$aJournal Article
000599007 500__ $$aISSN 1538-3881 not unique: **2 hits**.15 pages, 7 figures
000599007 520__ $$aThe Breakthrough Listen Initiative is conducting a program using multiple telescopes around the world to search for “technosignatures”: artificial transmitters of extraterrestrial origin from beyond our solar system. The Very Energetic Radiation Imaging Telescope Array System (VERITAS) Collaboration joined this program in 2018 and provides the capability to search for one particular technosignature: optical pulses of a few nanoseconds in duration detectable over interstellar distances. We report here on the analysis and results of dedicated VERITAS observations of Breakthrough Listen targets conducted in 2019 and 2020 and of archival VERITAS data collected since 2012. Thirty hours of dedicated observations of 136 targets and 249 archival observations of 140 targets were analyzed and did not reveal any signals consistent with a technosignature. The results are used to place limits on the fraction of stars hosting transmitting civilizations. We also discuss the minimum pulse sensitivity of our observations and present VERITAS observations of CALIOP: a space-based pulsed laser on board the Cloud-Aerosol Lidar and Infrared Pathfinder Satellite Observations. The detection of these pulses with VERITAS, using the analysis techniques developed for our technosignature search, allows a test of our analysis efficiency and serves as an important proof of principle.
000599007 536__ $$0G:(DE-HGF)POF4-613$$a613 - Matter and Radiation from the Universe (POF4-613)$$cPOF4-613$$fPOF IV$$x0
000599007 588__ $$aDataset connected to CrossRef, INSPIRE, Journals: bib-pubdb1.desy.de
000599007 693__ $$0EXP:(DE-H253)CTA-20150101$$5EXP:(DE-H253)CTA-20150101$$eCherenkov Telescope Array$$x0
000599007 693__ $$0EXP:(DE-H253)VERITAS-20170101$$5EXP:(DE-H253)VERITAS-20170101$$eVery Energetic Radiation Imaging Telescope Array System$$x1
000599007 7001_ $$00000-0002-9021-6192$$aAdams, Colin$$b1
000599007 7001_ $$aArcher, Avery$$b2
000599007 7001_ $$00000-0002-3886-3739$$aBangale, Priyadarshini$$b3
000599007 7001_ $$00000-0001-8138-1391$$aBatista, Pedro$$b4
000599007 7001_ $$00000-0003-2098-170X$$aBenbow, Wystan$$b5
000599007 7001_ $$00000-0002-6208-5244$$aBrill, Aryeh$$b6
000599007 7001_ $$00000-0002-8136-9461$$aCapasso, M.$$b7
000599007 7001_ $$00000-0002-1853-863X$$aErrando, Manel$$b8
000599007 7001_ $$00000-0002-5068-7344$$aFalcone, Abraham$$b9
000599007 7001_ $$aFeng, Qi$$b10
000599007 7001_ $$aFinley, John$$b11
000599007 7001_ $$00000-0002-2944-6060$$aFoote, Gregory$$b12$$eCorresponding author
000599007 7001_ $$00000-0002-1067-8558$$aFortson, Lucy$$b13
000599007 7001_ $$00000-0003-1614-1273$$aFurniss, Amy$$b14
000599007 7001_ $$aGriffin, Sean$$b15
000599007 7001_ $$00000-0002-0109-4737$$aHanlon, William$$b16
000599007 7001_ $$00000-0002-8513-5603$$aHanna, David$$b17
000599007 7001_ $$00000-0003-3878-1677$$aHervet, Olivier$$b18
000599007 7001_ $$00000-0001-6951-2299$$aHinrichs, Claire$$b19
000599007 7001_ $$aHoang, John$$b20
000599007 7001_ $$00000-0002-6833-0474$$aHolder, Jamie$$b21
000599007 7001_ $$00000-0002-1432-7771$$aHumensky, T. B.$$b22
000599007 7001_ $$00000-0002-1089-1754$$aJin, Weidong$$b23
000599007 7001_ $$00000-0002-3638-0637$$aKaaret, Philip$$b24
000599007 7001_ $$aKertzman, Mary P.$$b25
000599007 7001_ $$0P:(DE-H253)PIP1084929$$aKherlakian, Maria$$b26
000599007 7001_ $$00000-0003-4785-0101$$aKieda, David$$b27
000599007 7001_ $$0P:(DE-H253)PIP1093214$$aKleiner, Tobias$$b28
000599007 7001_ $$aKorzoun, Nikolas$$b29
000599007 7001_ $$aKumar, Sajan$$b30
000599007 7001_ $$00000-0003-4641-4201$$aLang, Mark$$b31
000599007 7001_ $$00000-0003-3802-1619$$aLundy, Matthew$$b32
000599007 7001_ $$0P:(DE-H253)PIP1011664$$aMaier, Gernot$$b33
000599007 7001_ $$aMcGrath, Conor$$b34
000599007 7001_ $$00000-0001-7106-8502$$aMillard, Matthew$$b35
000599007 7001_ $$aMiller, Hayden$$b36
000599007 7001_ $$aMillis, John$$b37
000599007 7001_ $$00000-0001-5937-446X$$aMooney, Connor$$b38
000599007 7001_ $$00000-0002-1499-2667$$aMoriarty, Patrick$$b39
000599007 7001_ $$00000-0002-3223-0754$$aMukherjee, Reshmi$$b40
000599007 7001_ $$00000-0002-9296-2981$$aO'Brien, Stephan$$b41
000599007 7001_ $$00000-0002-4837-5253$$aOng, Rene A.$$b42
000599007 7001_ $$0P:(DE-H253)PIP1010085$$aPohl, Martin$$b43
000599007 7001_ $$0P:(DE-H253)PIP1031007$$aPueschel, Elisa$$b44
000599007 7001_ $$00000-0002-4855-2694$$aQuinn, John$$b45
000599007 7001_ $$aRagan, Kenneth J.$$b46
000599007 7001_ $$aReynolds, Paul$$b47
000599007 7001_ $$00000-0002-7523-7366$$aRibeiro, Deivid$$b48
000599007 7001_ $$aRoache, Emmet Thomas$$b49
000599007 7001_ $$00000-0001-6662-5925$$aRyan, Jamie$$b50
000599007 7001_ $$0P:(DE-H253)PIP1006066$$aSadeh, Iftach$$b51
000599007 7001_ $$00000-0002-3171-5039$$aSaha, Lab$$b52
000599007 7001_ $$00000-0001-7297-8217$$aSantander, Marcos$$b53
000599007 7001_ $$aSembroski, Glenn H.$$b54
000599007 7001_ $$00000-0002-9856-989X$$aShang, Ruo$$b55
000599007 7001_ $$0P:(DE-H253)PIP1094637$$aTak, Donggeun$$b56
000599007 7001_ $$aTalluri, Anjana$$b57
000599007 7001_ $$aTucci, James$$b58
000599007 7001_ $$aVazquez, Nico$$b59
000599007 7001_ $$00000-0003-2740-9714$$aWilliams, David$$b60
000599007 7001_ $$0P:(DE-H253)PIP1102426$$aWong, S. L.$$b61
000599007 7001_ $$00009-0001-6471-1405$$aWoo, Jooyun$$b62
000599007 7001_ $$00000-0003-3197-2294$$aDeBoer, David$$b63
000599007 7001_ $$00000-0002-0531-1073$$aIsaacson, Howard$$b64
000599007 7001_ $$00000-0002-4278-3168$$ade Pater, Imke$$b65
000599007 7001_ $$00000-0003-2783-1608$$aPrice, Danny$$b66
000599007 7001_ $$00000-0003-2828-7720$$aSiemion, Andrew$$b67
000599007 7001_ $$0P:(DE-HGF)0$$aVERITAS Collaboration$$b68$$eCollaboration author
000599007 773__ $$0PERI:(DE-600)2207625-6$$a10.3847/1538-3881/ace347$$gVol. 166, no. 3, p. 84 -$$n3$$p84$$tThe astronomical journal$$v166$$x0004-6256$$y2023
000599007 8564_ $$uhttps://bib-pubdb1.desy.de/record/599007/files/Acharyya_2023_AJ_166_84.pdf$$yOpenAccess
000599007 8564_ $$uhttps://bib-pubdb1.desy.de/record/599007/files/Acharyya_2023_AJ_166_84.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000599007 909CO $$ooai:bib-pubdb1.desy.de:599007$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000599007 9101_ $$0I:(DE-588b)2008985-5$$60000-0001-8138-1391$$aDeutsches Elektronen-Synchrotron$$b4$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1084929$$aDeutsches Elektronen-Synchrotron$$b26$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1093214$$aDeutsches Elektronen-Synchrotron$$b28$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1011664$$aDeutsches Elektronen-Synchrotron$$b33$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1010085$$aDeutsches Elektronen-Synchrotron$$b43$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1031007$$aDeutsches Elektronen-Synchrotron$$b44$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1006066$$aDeutsches Elektronen-Synchrotron$$b51$$kDESY
000599007 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1094637$$aDeutsches Elektronen-Synchrotron$$b56$$kDESY
000599007 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1102426$$aExternal Institute$$b61$$kExtern
000599007 9131_ $$0G:(DE-HGF)POF4-613$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vMatter and Radiation from the Universe$$x0
000599007 9141_ $$y2023
000599007 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2021-02-02
000599007 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000599007 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bASTRON J : 2019$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bASTRON J : 2019$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)0700$$2StatID$$aFees$$d2023-08-23
000599007 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000599007 915__ $$0StatID:(DE-HGF)0561$$2StatID$$aArticle Processing Charges$$d2023-08-23
000599007 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2021-02-02
000599007 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2021-02-02
000599007 9201_ $$0I:(DE-H253)Z_CTA-20210408$$kZ_CTA$$lCherenkov Telescope Array$$x0
000599007 9201_ $$0I:(DE-H253)Z_VER-20210408$$kZ_VER$$lVERITAS$$x1
000599007 980__ $$ajournal
000599007 980__ $$aVDB
000599007 980__ $$aUNRESTRICTED
000599007 980__ $$aI:(DE-H253)Z_CTA-20210408
000599007 980__ $$aI:(DE-H253)Z_VER-20210408
000599007 9801_ $$aFullTexts