We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr 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 yr 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 are 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 ...
We present reverberation-mapping (RM) lags and black hole mass measurements using the C IV lambda 15...
Reverberation mapping (RM) measurements of broad-line region (BLR) lags in z > 0.3 quasars are im...
As photons from different bands emerge from different radial ranges in the accretion disk, the lags ...
We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr spectroscopy...
We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr spectroscopy...
We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr spectroscopy...
We present reverberation mapping results from the first year of combined spectroscopic and photometr...
We present composite broad-line region (BLR) reverberation mapping lag measurements for H alpha, H b...
We investigate the performance of different methodologies that measure the time lag between broad-li...
Funding: STFC grant ST/M001296/1 (KH).We present composite broad-line region (BLR) reverberation map...
We investigate the performance of different methodologies that measure the time lag between broad-li...
We present reverberation mapping results for the Mg ii λ2800 Å broad emission line in a sample of 19...
K.H. acknowledges support from STFC grant ST/M001296/1.We present reverberation-mapping (RM) lags an...
We present composite broad-line region (BLR) reverberation mapping lag measurements for Hα, Hβ, He I...
We present reverberation-mapping (RM) lags and black hole mass measurements using the C iv λ1549 bro...
We present reverberation-mapping (RM) lags and black hole mass measurements using the C IV lambda 15...
Reverberation mapping (RM) measurements of broad-line region (BLR) lags in z > 0.3 quasars are im...
As photons from different bands emerge from different radial ranges in the accretion disk, the lags ...
We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr spectroscopy...
We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr spectroscopy...
We investigate the effects of extended multiyear light curves (9 yr photometry and 5 yr spectroscopy...
We present reverberation mapping results from the first year of combined spectroscopic and photometr...
We present composite broad-line region (BLR) reverberation mapping lag measurements for H alpha, H b...
We investigate the performance of different methodologies that measure the time lag between broad-li...
Funding: STFC grant ST/M001296/1 (KH).We present composite broad-line region (BLR) reverberation map...
We investigate the performance of different methodologies that measure the time lag between broad-li...
We present reverberation mapping results for the Mg ii λ2800 Å broad emission line in a sample of 19...
K.H. acknowledges support from STFC grant ST/M001296/1.We present reverberation-mapping (RM) lags an...
We present composite broad-line region (BLR) reverberation mapping lag measurements for Hα, Hβ, He I...
We present reverberation-mapping (RM) lags and black hole mass measurements using the C iv λ1549 bro...
We present reverberation-mapping (RM) lags and black hole mass measurements using the C IV lambda 15...
Reverberation mapping (RM) measurements of broad-line region (BLR) lags in z > 0.3 quasars are im...
As photons from different bands emerge from different radial ranges in the accretion disk, the lags ...