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      The Sloan Digital Sky Survey Reverberation Mapping Project: Improving Lag Detection with an Extended Multi-Year Baseline

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          Abstract

          We investigate the effects of extended multi-year light curves (9-year photometry and 5-year spectroscopy) on the detection of time lags between the continuum variability and broad-line response of quasars at z>~1.5, and compare with the results using 4-year photometry+spectroscopy presented in a companion paper. We demonstrate the benefits of the extended light curves in three cases: (1) lags that are too long to be detected by the shorter-duration data but can be detected with the extended data; (2) lags that are recovered by the extended light curves but missed in the shorter-duration data due to insufficient light curve quality; and (3) lags for different broad line species in the same object. These examples demonstrate the importance of long-term monitoring for reverberation mapping to detect lags for luminous quasars at high-redshift, and the expected performance of the final dataset from the Sloan Digital Sky Survey Reverberation Mapping project that will have 11-year photometric and 7-year spectroscopic baselines.

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          Author and article information

          Journal
          31 July 2019
          Article
          1908.00027
          a875a7e7-08ef-489f-9d20-a8775459c8f4

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

          History
          Custom metadata
          submitted to AAS journals; 9 pages
          astro-ph.GA

          Galaxy astrophysics
          Galaxy astrophysics

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