Space telescope and optical reverberation mapping project. III. Optical continuum emission and broadband time delays in NGC 5548

摘要: The LBT is an international collaboration among institutions in the United States, Italy and Germany. Corporation partners are: Ohio State University, Research Corporation, on behalf of University Notre Dame, University of Minnesota Virginia; Arizona university system; Istituto Nazionale di Astrofisica, Italy; Beteiligungsgesellschaft, Germany, representing Max-Planck Society, the Astrophysical Institute Potsdam, Heidelberg University. This paper used data obtained with MODS spectrographs built funding from National Science Foundation (NSF) grant AST-9987045 NSF Telescope System Instrumentation Program (TSIP), additional funds Ohio Board Regents Office Research. This made use modsIDL spectral data reduction pipeline developed in part provided by NSF Grant AST - 1108693. The Liverpool operated island La Palma by John Moores Spanish Observatorio del Roque de los Muchachos Instituto de Astrofisica Canarias financial support UK Science Technology Facilities Council. KAIT its ongoing operation were possible donations from Sun Microsystems, Inc., Hewlett-Packard Company, AutoScope Corporation, Lick Observatory, the NSF, California, Sylvia Jim Katzman Foundation, TABASGO Foundation. Research at Lick Observatory partially supported a generous gift from Google. Support for HST program number GO-13330 was provided by NASA through grant Space Science Institute, which Association Universities for Astronomy, under contract NAS5-26555. M.M.F., G.D.R., B.M.P., C.J.G., R.W.P. are grateful AST- 1008882 to University. A.J.B. L.P. have been AST-1412693. A.V.F. W.- K.Z. are assistance AST- 1211916, Foundation, Christopher R. Redlich Fund. M.C. Bentz gratefully acknowledges support through CAREER AST-1253702 Georgia State University. Bottorff HHMI undergraduate science education Southwestern University. K.D.D. Fellowship awarded AST-1302093. R.E. acknowledges support awards NNX13AC26G, NNX13AC63G, NNX13AE99G. J.M.G. award NNH13CH61C. P.B.H. NSERC. M.I. support from Creative Initiative program, No. 2008-0060544, of the Korea (NRFK) funded by Korean government (MSIP). M.D.J. NSF grant AST-0618209 obtaining 0.91 m telescope at WMO. SRON financially NWO, Netherlands Organization Scientific Research. B.C.K. partially supported UC Center Galaxy Evolution. C.S.K. acknowledges the AST-1009756. D.C.L. acknowledges grants AST-1009571 and AST-1210311, this research (photometric observations collected at MLO) carried out. We thank Nhieu Duong, Harish Khandrika, Richard Mellinger, J. Chuck Horst, Steven Armen, Eddie Garcia the MLO observations. P.L. Fondecyt grant #1120328. A.P. graduate fellowship, UCSB Dean’s Fellowship, Einstein Fellowship. J.S.S. CNPq, Council for Technological Development (Brazil) for partial warm hospitality. T.T. has been AST-1412315. T.T. acknowledge Packard Foundation in form Fellowship T.T.; also, T.T. thanks American Academy Rome Observatory of Monteporzio Catone kind hospitality. The Dark Cosmology Centre funded Danish National Research M.V. Council Independent via grant no. DFF–4002-00275. J.-H.W. the National (NRF) (No. 2010-0027910). E.D.B. is supported Padua 60A02-5857/13, 60A02-5833/14, 60A02-4434/15, CPDA133894. K.H. STFC ST/M001296/1. S.A.K. thanks Dr. I. A. Rakhimov, Director Svetloe Observatory, for his hospitality. This NASA/IPAC Extragalactic Database (NED), Jet Propulsion Laboratory, California Technology, contract with NASA.