Free Access
Table 4.
Measured time delays, in days, for the two PyCS estimators and their combination (see text).
| PyCS free-knot splines | PyCS regression differences | PyCS combined | |
|---|---|---|---|
| HE 0047−1756 |
 |
 |
 |
| WG 0214−2105 |
 |
 |
 |
 |
 |
 |
|
 |
 |
 |
|
 |
 |
 |
|
 |
 |
 |
|
 |
 |
 |
|
| DES 0407−5006 |
 |
 |
 |
| 2M 1134−2103 |
 |
 |
 |
 |
 |
 |
|
 |
 |
 |
|
 |
 |
 |
|
 |
 |
 |
|
 |
 |
 |
|
| PSJ 1606−2333 |
 |
 |
 |
 |
 |
 |
|
 |
 |
 |
|
| DES 2325−5229 |
 |
 |
 |
Notes. In the case of HE 0047−1756, the final PyCS-mult estimate is 
d and is obtained by combining our WFI data set with monitoring data from the Leonhard Euler 1.2 m Swiss telescope (Millon et al. 2020).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.