The Sloan Digital Sky Survey Reverberation Mapping Project : comparison of lag measurement methods with simulated observations
MetadataShow full item record
Altmetrics Handle Statistics
Altmetrics DOI Statistics
We investigate the performance of different methodologies that measure the time lag between broad-line and continuum variations in reverberation mapping data using simulated light curves that probe a range of cadence, time baseline, and signal-to-noise ratio in the flux measurements. We compare three widely adopted lag-measuring methods: the interpolated cross-correlation function (ICCF), the z-transformed discrete correlation function (ZDCF), and the Markov chain Monte Carlo code JAVELIN, for mock data with qualities typical of multiobject spectroscopic reverberation mapping (MOS-RM) surveys that simultaneously monitor hundreds of quasars. We quantify the overall lag-detection efficiency, the rate of false detections, and the quality of lag measurements for each of these methods and under different survey designs (e.g., observing cadence and depth) using mock quasar light curves. Overall JAVELIN and ICCF outperform ZDCF in essentially all tests performed. Compared with ICCF, JAVELIN produces higher quality lag measurements, is capable of measuring more lags with timescales shorter than the observing cadence, is less susceptible to seasonal gaps and signal-to-noise ratio degradation in the light curves, and produces more accurate lag uncertainties. We measure the Hβ broad-line region size–luminosity (R–L) relation with each method using the simulated light curves to assess the impact of selection effects of the design of MOS-RM surveys. The slope of the R–L relation measured by JAVELIN is the least biased among the three methods and is consistent across different survey designs. These results demonstrate a clear preference for JAVELIN over the other two nonparametric methods for MOS-RM programs, particularly in the regime of limited light-curve quality as expected from most MOS-RM programs.
Li , J I-H , Shen , Y , Brandt , W N , Grier , C J , Hall , P B , Ho , L C , Homayouni , Y , Horne , K , Schneider , D P , Trump , J R & Starkey , D A 2019 , ' The Sloan Digital Sky Survey Reverberation Mapping Project : comparison of lag measurement methods with simulated observations ' , Astrophysical Journal , vol. 884 , no. 2 , 119 , pp. 1-21 . https://doi.org/10.3847/1538-4357/ab41fb
Copyright © 2019 The American Astronomical Society. This work has been made available online in accordance with publisher policies or with permission. Permission for further reuse of this content should be sought from the publisher or the rights holder. This is the final published version of the work, which was originally published at https://doi.org/10.3847/1538-4357/ab41fb
Items in the St Andrews Research Repository are protected by copyright, with all rights reserved, unless otherwise indicated.