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dc.date.accessioned2022-02-16T18:54:45Z
dc.date.available2022-02-16T18:54:45Z
dc.date.created2022-01-26T17:18:48Z
dc.date.issued2021
dc.identifier.citationPenton, Andrew Malik, U. Davis, Tamara M. Martini, P. Yu, Z. Sharp, R. Lidman, Christer Tucker, B. E. Hoormann, J. K. Aguena, Michel Allam, Sahar Annis, James Asorey, Jacobo Bacon, David Bertin, Emmanuel Bhargava, S. Brooks, D. Calcino, J. Carnero Rosell, Aurelio Carollo, D. Carrasco Kind, Matias Carretero, Jorge Costanzi, Matteo da Costa, L. N. Pereira, Maria Elidaiana da Silva De Vicente, J. Diehl, Herman T. Eifler, Tim F. Everett, S. Ferrero, Ismael Fosalba, Pablo Frieman, J. García-Bellido, Juan Gaztañaga, Enrique Gerdes, David W. Gruen, Daniel Gruendl, Robert A. Gschwend, J. Gutierrez, G. Hinton, Samuel R. Hollowood, Devon L. Honscheid, Klaus James, D. J. Kim, A. G. Kuehn, Kyler Kuropatkin, Nikolay Maia, Marcio A. G. Marshall, J. L. Menanteau, Felipe Miquel, Ramon Morgan, R. Möller, A. Palmese, Antonella Paz-Chinchón, Francisco Plazas, Andrés A. Romer, A. K. Sanchez, E. Scarpine, V. Scolnic, Daniel Serrano, S. Smith, Mathew Suchyta, Eric Swanson, Molly E. C. Tarlé, Gregory To, Chun-Hao Uddin, S. A. Varga, Tamas Norbert Wester, W. Wilkinson, R. D. Lewis, G. . OzDES reverberation mapping program: Lag recovery reliability for 6-yr C IV analysis. Monthly notices of the Royal Astronomical Society. 2021, 509(3), 4008-4023
dc.identifier.urihttp://hdl.handle.net/10852/91015
dc.description.abstractABSTRACT We present the statistical methods that have been developed to analyse the OzDES reverberation mapping sample. To perform this statistical analysis we have created a suite of customizable simulations that mimic the characteristics of each source in the OzDES sample. These characteristics include: the variability in the photometric and spectroscopic light curves, the measurement uncertainties, and the observational cadence. By simulating the sources in the OzDES sample that contain the C iv emission line, we developed a set of criteria that rank the reliability of a recovered time-lag depending on the agreement between different recovery methods, the magnitude of the uncertainties, and the rate at which false positives were found in the simulations. These criteria were applied to simulated light curves and these results used to estimate the quality of the resulting Radius–Luminosity relation. We grade the results using three quality levels (gold, silver, and bronze). The input slope of the R–L relation was recovered within 1σ for each of the three quality samples, with the gold standard having the lowest dispersion with a recovered a R–L relation slope of 0.454 ± 0.016 with an input slope of 0.47. Future work will apply these methods to the entire OzDES sample of 771 AGN.
dc.languageEN
dc.titleOzDES reverberation mapping program: Lag recovery reliability for 6-yr C IV analysis
dc.typeJournal article
dc.creator.authorPenton, Andrew
dc.creator.authorMalik, U.
dc.creator.authorDavis, Tamara M.
dc.creator.authorMartini, P.
dc.creator.authorYu, Z.
dc.creator.authorSharp, R.
dc.creator.authorLidman, Christer
dc.creator.authorTucker, B. E.
dc.creator.authorHoormann, J. K.
dc.creator.authorAguena, Michel
dc.creator.authorAllam, Sahar
dc.creator.authorAnnis, James
dc.creator.authorAsorey, Jacobo
dc.creator.authorBacon, David
dc.creator.authorBertin, Emmanuel
dc.creator.authorBhargava, S.
dc.creator.authorBrooks, D.
dc.creator.authorCalcino, J.
dc.creator.authorCarnero Rosell, Aurelio
dc.creator.authorCarollo, D.
dc.creator.authorCarrasco Kind, Matias
dc.creator.authorCarretero, Jorge
dc.creator.authorCostanzi, Matteo
dc.creator.authorda Costa, L. N.
dc.creator.authorPereira, Maria Elidaiana da Silva
dc.creator.authorDe Vicente, J.
dc.creator.authorDiehl, Herman T.
dc.creator.authorEifler, Tim F.
dc.creator.authorEverett, S.
dc.creator.authorFerrero, Ismael
dc.creator.authorFosalba, Pablo
dc.creator.authorFrieman, J.
dc.creator.authorGarcía-Bellido, Juan
dc.creator.authorGaztañaga, Enrique
dc.creator.authorGerdes, David W.
dc.creator.authorGruen, Daniel
dc.creator.authorGruendl, Robert A.
dc.creator.authorGschwend, J.
dc.creator.authorGutierrez, G.
dc.creator.authorHinton, Samuel R.
dc.creator.authorHollowood, Devon L.
dc.creator.authorHonscheid, Klaus
dc.creator.authorJames, D. J.
dc.creator.authorKim, A. G.
dc.creator.authorKuehn, Kyler
dc.creator.authorKuropatkin, Nikolay
dc.creator.authorMaia, Marcio A. G.
dc.creator.authorMarshall, J. L.
dc.creator.authorMenanteau, Felipe
dc.creator.authorMiquel, Ramon
dc.creator.authorMorgan, R.
dc.creator.authorMöller, A.
dc.creator.authorPalmese, Antonella
dc.creator.authorPaz-Chinchón, Francisco
dc.creator.authorPlazas, Andrés A.
dc.creator.authorRomer, A. K.
dc.creator.authorSanchez, E.
dc.creator.authorScarpine, V.
dc.creator.authorScolnic, Daniel
dc.creator.authorSerrano, S.
dc.creator.authorSmith, Mathew
dc.creator.authorSuchyta, Eric
dc.creator.authorSwanson, Molly E. C.
dc.creator.authorTarlé, Gregory
dc.creator.authorTo, Chun-Hao
dc.creator.authorUddin, S. A.
dc.creator.authorVarga, Tamas Norbert
dc.creator.authorWester, W.
dc.creator.authorWilkinson, R. D.
dc.creator.authorLewis, G.
cristin.unitcode185,15,3,0
cristin.unitnameInstitutt for teoretisk astrofysikk
cristin.ispublishedtrue
cristin.fulltextoriginal
cristin.qualitycode1
dc.identifier.cristin1990726
dc.identifier.bibliographiccitationinfo:ofi/fmt:kev:mtx:ctx&ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.jtitle=Monthly notices of the Royal Astronomical Society&rft.volume=509&rft.spage=4008&rft.date=2021
dc.identifier.jtitleMonthly notices of the Royal Astronomical Society
dc.identifier.volume509
dc.identifier.issue3
dc.identifier.startpage4008
dc.identifier.endpage4023
dc.identifier.doihttps://doi.org/10.1093/mnras/stab3027
dc.identifier.urnURN:NBN:no-93599
dc.subject.nviVDP::Astrofysikk, astronomi: 438
dc.type.documentTidsskriftartikkel
dc.type.peerreviewedPeer reviewed
dc.source.issn0035-8711
dc.identifier.fulltextFulltext https://www.duo.uio.no/bitstream/handle/10852/91015/1/stab3027.pdf
dc.type.versionPublishedVersion
dc.relation.projectNFR/287772


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