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Intensive disc-reverberation mapping of Fairall 9: 1st year of Swift & LCO monitoring
Monthly Notices of the Royal Astronomical Society ( IF 4.8 ) Pub Date : 2020-09-21 , DOI: 10.1093/mnras/staa2365
J V Hernández Santisteban 1 , R Edelson 2 , K Horne 1 , J M Gelbord 3, 4 , A J Barth 5 , E M Cackett 6 , M R Goad 7 , H Netzer 8 , D Starkey 1 , P Uttley 9 , W N Brandt 10, 11, 12 , K Korista 13 , A M Lohfink 14 , C A Onken 15, 16 , K L Page 7 , M Siegel 10 , M Vestergaard 17 , S Bisogni 18 , A A Breeveld 19 , S B Cenko 20, 21 , E Dalla Bontã 22, 23 , P A Evans 7 , G Ferland 24 , D H Gonzalez-Buitrago 25 , D Grupe 26 , M D Joner 27 , G Kriss 28 , S J LaPorte 29 , S Mathur 30, 31 , F Marshall 32 , M Mehdipour 33 , D Mudd 5 , B M Peterson 28, 30, 31 , T Schmidt 5 , S Vaughan 7 , S Valenti 34
Affiliation  

We present results of time-series analysis of the first year of the Fairall 9 intensive disc-reverberation campaign. We used Swift and the Las Cumbres Observatory global telescope network to continuously monitor Fairall 9 from X-rays to near-infrared at a daily to sub-daily cadence. The cross-correlation function between bands provides evidence for a lag spectrum consistent with the τ ∝ λ4/3 scaling expected for an optically thick, geometrically thin blackbody accretion disc. Decomposing the flux into constant and variable components, the variable component's spectral energy distribution is slightly steeper than the standard accretion disc prediction. We find evidence at the Balmer edge in both the lag and flux spectra for an additional bound-free continuum contribution that may arise from reprocessing in the broad-line region. The inferred driving light curve suggests two distinct components, a rapidly variable ( 100 days) component with an opposite lag to the reverberation signal.

中文翻译:

Fairall 9 的密集光盘混响映射:Swift 和 LCO 监测的第一年

我们展示了 Fairall 9 密集唱片混响活动第一年的时间序列分析结果。我们使用 Swift 和 Las Cumbres 天文台全球望远镜网络,以每日到次日的节奏持续监测从 X 射线到近红外的 Fairall 9。波段之间的互相关函数为滞后谱提供了证据,该滞后谱与光学厚、几何薄黑体吸积盘预期的 τ ∝ λ4/3 标度一致。将通量分解为常数和可变分量,可变分量的光谱能量分布比标准吸积盘预测略陡。我们在滞后和通量谱中的 Balmer 边缘找到了证据,证明可能由宽线区域中的再处理产生的额外的无界连续谱贡献。
更新日期:2020-09-21
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