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OzDES reverberation mapping program: Lag recovery reliability for 6-yr C IV analysis

OzDES reverberation mapping program: Lag recovery reliability for 6-yr C IV analysis
OzDES reverberation mapping program: Lag recovery reliability for 6-yr C IV analysis
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.
1365-2966
4008-4023
Penton, A
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Davis, T M
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Tucker, B E
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Wester, W
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Wilkinson, R D
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Lewis, G
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Penton, A
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Malik, U
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Davis, T M
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Sharp, R
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Lidman, C
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Tucker, B E
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Hoormann, J K
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Aguena, M
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Allam, S
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Annis, J
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Asorey, J
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Bacon, D
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Bertin, E
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Bhargava, S
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Brooks, D
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Calcino, J
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Carollo, D
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Carretero, J
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Costanzi, M
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Fosalba, P
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Frieman, J
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Gaztanaga, E
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Gruen, D
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Gschwend, J
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Kuehn, K
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Suchyta, E
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Tarle, G
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Uddin, S A
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Wilkinson, R D
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Lewis, G
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Penton, A, Malik, U, Davis, T M, Martini, P, Yu, Z, Sharp, R, Lidman, C, Tucker, B E, Hoormann, J K, Aguena, M, Allam, S, Annis, J, Asorey, J, Bacon, D, Bertin, E, Bhargava, S, Brooks, D, Calcino, J, Carnero rosell, A, Carollo, D, Carrasco kind, M, Carretero, J, Costanzi, M, Da costa, L N, Pereira, M E S, De vicente, J, Diehl, H T, Eifler, T F, Everett, S, Ferrero, I, Fosalba, P, Frieman, J, García-bellido, J, Gaztanaga, E, Gerdes, D W, Gruen, D, Gruendl, R A, Gschwend, J, Gutierrez, G, Hinton, S R, Hollowood, D L, Honscheid, K, James, D J, Kim, A G, Kuehn, K, Kuropatkin, N, Maia, M A G, Marshall, J L, Menanteau, F, Miquel, R, Morgan, R, Möller, A, Palmese, A, Paz-chinchón, F, Plazas, A A, Romer, A K, Sanchez, E, Scarpine, V, Scolnic, D, Serrano, S, Smith, M, Suchyta, E, Swanson, M E C, Tarle, G, To, C, Uddin, S A, Varga, T N, Wester, W, Wilkinson, R D and Lewis, G (2021) OzDES reverberation mapping program: Lag recovery reliability for 6-yr C IV analysis. Monthly Notices of the Royal Astronomical Society, 509 (3), 4008-4023. (doi:10.1093/mnras/stab3027).

Record type: Article

Abstract

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.

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Accepted/In Press date: 14 October 2021
Published date: 3 December 2021

Identifiers

Local EPrints ID: 455129
URI: http://eprints.soton.ac.uk/id/eprint/455129
ISSN: 1365-2966
PURE UUID: f8d95194-2511-4c79-ba01-af2701f79a8f
ORCID for J L Marshall: ORCID iD orcid.org/0000-0002-9242-3646

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Date deposited: 10 Mar 2022 17:43
Last modified: 17 Mar 2024 02:34

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Contributors

Author: A Penton
Author: U Malik
Author: T M Davis
Author: P Martini
Author: Z Yu
Author: R Sharp
Author: C Lidman
Author: B E Tucker
Author: J K Hoormann
Author: M Aguena
Author: S Allam
Author: J Annis
Author: J Asorey
Author: D Bacon
Author: E Bertin
Author: S Bhargava
Author: D Brooks
Author: J Calcino
Author: A Carnero rosell
Author: D Carollo
Author: M Carrasco kind
Author: J Carretero
Author: M Costanzi
Author: L N Da costa
Author: M E S Pereira
Author: J De vicente
Author: H T Diehl
Author: T F Eifler
Author: S Everett
Author: I Ferrero
Author: P Fosalba
Author: J Frieman
Author: J García-bellido
Author: E Gaztanaga
Author: D W Gerdes
Author: D Gruen
Author: R A Gruendl
Author: J Gschwend
Author: G Gutierrez
Author: S R Hinton
Author: D L Hollowood
Author: K Honscheid
Author: D J James
Author: A G Kim
Author: K Kuehn
Author: N Kuropatkin
Author: M A G Maia
Author: J L Marshall ORCID iD
Author: F Menanteau
Author: R Miquel
Author: R Morgan
Author: A Möller
Author: A Palmese
Author: F Paz-chinchón
Author: A A Plazas
Author: A K Romer
Author: E Sanchez
Author: V Scarpine
Author: D Scolnic
Author: S Serrano
Author: M Smith
Author: E Suchyta
Author: M E C Swanson
Author: G Tarle
Author: C To
Author: S A Uddin
Author: T N Varga
Author: W Wester
Author: R D Wilkinson
Author: G Lewis

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