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dc.contributor.authorEdelson, R
dc.contributor.authorGelbord, J.
dc.contributor.authorCackett, E.
dc.contributor.authorPeterson, B. M.
dc.contributor.authorHorne, K.
dc.contributor.authorBarth, A. J.
dc.contributor.authorStarkey, D. A.
dc.contributor.authorBentz, M.
dc.contributor.authorBrandt, W. N.
dc.contributor.authorGoad, M.
dc.contributor.authorJoner, M.
dc.contributor.authorKorista, K.
dc.contributor.authorNetzer, H.
dc.contributor.authorPage, K.
dc.contributor.authorUttley, P.
dc.contributor.authorVaughan, S.
dc.contributor.authorBreeveld, A.
dc.contributor.authorCenko, S. B.
dc.contributor.authorDone, C.
dc.contributor.authorEvans, P.
dc.contributor.authorFausnaugh, M.
dc.contributor.authorFerland, G.
dc.contributor.authorGonzalez-Buitrago, D.
dc.contributor.authorGropp, J.
dc.contributor.authorGrupe, D.
dc.contributor.authorKaastra, J.
dc.contributor.authorKennea, J.
dc.contributor.authorKriss, G.
dc.contributor.authorMathur, S.
dc.contributor.authorMehdipour, M.
dc.contributor.authorNousek, J.
dc.contributor.authorSchmidt, T.
dc.contributor.authorVestergaard, M.
dc.contributor.authorVillforth, C.
dc.date.accessioned2018-12-14T13:45:12Z
dc.date.available2018-12-14T13:45:12Z
dc.date.issued2018-11-19
dc.identifierhttps://doi.org/10.13016/M2280532D
dc.identifier.citationarXiv:1811.07956en_US
dc.identifier.urihttp://hdl.handle.net/1903/21536
dc.descriptionen_US
dc.description.abstractSince 2014, the Niel Gehrels Swift observatory has conducted a series of intensive accretion disk reverberation mapping (IDRM) campaigns of bright AGN. This archive contains reduced data from the first four of these campaigns. We are making the data publicly available to facilitate uniform modeling and analysis of these data. Please feel free to download and use the data as you wish. This table will be updated as more IDRM campaigns are published and as the data reduction (mostly dropout filtering) improves. If these data result in publications, please cite the source paper: "The First Swift Intensive AGN Accretion Disk Reverberation Mapping Survey" by Edelson et al. (2019 ApJ 870 123; available at http://iopscience.iop.org/article/10.3847/1538-4357/aaf3b4/meta). Also please note: © AAS. Reproduced with permission. TABLE NOTES: Column 1: Object name. Column 2: Filter/band used to measure the data point. Column 3: Cadence number, where the most significant digit refers to the object and the next three refer to the visit number for that object. Column 4: Modified Julian Day at the midpoint of the exposure. Column 5: Duration of the integration in that filter/band, in seconds. Column 6: Mean flux of the data point. UVOT fluxes are given in units of 10^-{14} erg/cm2/s/A and X-ray fluxes in units of ct/s. Column 7: Uncertainty on the flux, in the same units as Column 6.en_US
dc.description.sponsorshipNASAen_US
dc.language.isoen_USen_US
dc.publisherarXiv.orgen_US
dc.subjectActive Galactic Nucleien_US
dc.subjectNeil Gehrels Swift Observatoryen_US
dc.titleReduced data for the Swift Intensive Accretion Disk Reverberation Mapping Surveyen_US
dc.typeDataseten_US
dc.relation.isAvailableAtAstronomyen_us
dc.relation.isAvailableAtCollege of Computer, Mathematical & Natural Sciencesen_us
dc.relation.isAvailableAtDigital Repository at the University of Marylanden_us
dc.relation.isAvailableAtUniversity of Maryland (College Park, MD)en_us


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