论文标题

Cosmograil XIX:从15年的光学监测中进行的18种强烈镜头类星体的时间延迟

COSMOGRAIL XIX: Time delays in 18 strongly lensed quasars from 15 years of optical monitoring

论文作者

Millon, M., Courbin, F., Bonvin, V., Paic, E., Meylan, G., Tewes, M., Sluse, D., Magain, P., Chan, J. H. H., Galan, A., Joseph, R., Lemon, C., Tihhonova, O., Anderson, R. I., Marmier, M., Chazelas, B., Lendl, M., Triaud, A. H. M. J., Wyttenbach, A.

论文摘要

我们介绍了15年监测镜头类星体的结果,该结果是由Cosmograil计划在Leonhard Euler 120万瑞士望远镜上进行的。首次提出了23个镜头系统的十年光曲线。我们将数据集与文献中可用的其他监视数据相辅相成,以测量18个系统中的时间延迟,其中9个相对精度至少在一个时间延迟中的相对精度高于15%。为了实现这一目标,我们开发了一个自动化版本的曲线移动工具箱pycs,以确保在存在微透析的情况下对时间延迟的稳健估计,同时由于微透镜的不完美表示而考虑了错误。我们还通过分别添加六个和两个新季节的监视,并确认了以前的时间延迟测量值,从而重新安排了RX J1131 $ - $ 1231和HE 0435 $ - $ 1223的时间延迟。当可能的时间延迟测量值时,我们从它们的时间延迟中校正了镜头图像的光曲线,并呈现差异曲线,以突出数据中包含的微透镜信号。迄今为止,这是长达十年镜头监测数据的最大样本,这对于测量$ H_0 $和具有微透明的类星体积聚盘的大小以及研究类星体可变性很有用。

We present the results of 15 years of monitoring lensed quasars, which was conducted by the COSMOGRAIL programme at the Leonhard Euler 1.2m Swiss Telescope. The decade-long light curves of 23 lensed systems are presented for the first time. We complement our data set with other monitoring data available in the literature to measure the time delays in 18 systems, among which nine reach a relative precision better than 15% for at least one time delay. To achieve this, we developed an automated version of the curve-shifting toolbox PyCS to ensure robust estimation of the time delay in the presence of microlensing, while accounting for the errors due to the imperfect representation of microlensing. We also re-analysed the previously published time delays of RX J1131$-$1231 and HE 0435$-$1223, by adding six and two new seasons of monitoring, respectively, and confirming the previous time-delay measurements. When the time delay measurement is possible, we corrected the light curves of the lensed images from their time delay and present the difference curves to highlight the microlensing signal contained in the data. To date, this is the largest sample of decade-long lens monitoring data, which is useful to measure $H_0$ and the size of quasar accretion discs with microlensing as well as to study quasar variability.

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