VizieR Online Data Catalog: Five years of blazar observations with VERITAS (Archambault+, 2016)

S Archambault,A Archer,W Benbow,R Bird, J Biteau, M Buchovecky,JH Buckley,V Bugaev,K Byrum,M Cerruti, X Chen,L Ciupik,MP Connolly,W Cui,JD Eisch,M Errando,A Falcone,Q Feng,JP Finley,H Fleischhack,P Fortin,L Fortson, A Furniss,GH Gillanders,S Griffin, J Grube, G Gyuk, M Hutten,N Hakansson, D Hanna,J Holder,TB Humensky,CA Johnson,P Kaaret, P Kar,N Kelley-Hoskins,M Kertzman,D Kieda,M Krause, F Krennrich,S Kumar,MJ Lang, G Maier,S McArthur,A McCann,K Meagher,P Moriarty,R Mukherjee,T Nguyen,D Nieto, A O'Faolain de Bhroithe,RA Ong,AN Otte,N Park,JS Perkins, A Pichel, M Pohl, A Popkow,E Pueschel,J Quinn,K Ragan,PT Reynolds, GT Richards, E Roache,AC Rovero,M Santander,GH Sembroski, K Shahinyan,AW Smith,D Staszak,I Telezhinsky,JV Tucci,J Tyler, S Vincent,SP Wakely,OM Weiner,A Weinstein,DA Williams, B Zitzer

yCat（2018）

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摘要

In this paper, we present the results of the analysis of most of the non-detected blazars observed by VERITAS from 2007 (the beginning of full-scale scientific operations) to 2012 August (before the upgrade of the VERITAS array, see Kieda 2013arXiv1308. 4849D). The VERITAS (Very Energetic Radiation Imaging Telescope Array System) telescope array is composed of four IACTs of 12 m diameter each, located at the Fred Lawrence Whipple Observatory, on the slopes of Mount Hopkins, in southern Arizona (31 40'N, 110 57'W). Each telescope has a segmented mirror that focuses light onto a camera composed of 499 photomultipliers located at the focal plane. The instrument FOV is 3.5. For further details on the VERITAS instrument, see Holder et al.(2006APh.... 25.. 391H) and Holder (2011ICRC... 12.. 137H). The VERITAS observations here have an average length of 20 minutes (referred to as a run), before …

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