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Bonvin et al. The LT monitoring offers a unique opportunity to obtain homogeneous and accurate light curves of GLQs, and thus time delays with an uncertainty of a few days. For three objects that have been updated in recent papers, i. Here, we present additional r-band photometric data of the two quasar images A and B, which were obtained from RATCam frames in February—April 18 epochs , as well as using the IO:O camera in the period spanning from October to June epochs; see Table 3.

After some initial processing tasks, including cosmic-ray removal and bad pixel masking, a crowded-field photometry pipeline produced magnitudes of A and B for every IO:O frame. This model only consists of two close stellar-like sources, where each source is described by an empirical point-spread function PSF.

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Kochanek et al. By visual inspection of the pre-selected brightness records, we then found that the magnitudes of A and B at a few epochs strongly deviate from adjacent data. These outliers were also discarded. In a last step, assuming the root-mean-square deviations between magnitudes on consecutive nights as errors, the uncertainties were 0. The r-band data collected by us and the USNO group during a yr period are also displayed in the top panel of Fig. The new epochs of magnitudes after day lead to new microlensing variability in the difference light curve DLC; see the middle and bottom panels of Fig.

These last records 37 epochs , based on Uzbekistan MAO observations between and , indicated the existence of a long-timescale microlensing fluctuation. The MAO monitoring programme was conducted by an international collaboration of astronomers from Russia, Ukraine, Uzbekistan, and other countries.

We also analyse these frames, which are not included in the database. The lensing galaxy is too faint to be detected with a red filter, and thus the system was described as two stellar-like objects, that is, two PSFs. The S1 field star was used to estimate the PSF, whereas we considered the S3 field star to check the reliability of the quasar brightness fluctuations see the finding chart in Fig.

Most of the LT frames 64 of 72 led to reasonable photometric results, and these usable frames were then combined on a nightly basis to produce r-band magnitudes at 28 epochs.

For each object, the typical photometric error for an individual exposure was determined from the intra-night scatter of the magnitude values measured on the individual frames.

These intra-night scatters were 0. We remark that both magnitude offsets were calculated from the records of the non-variable star S3. The top panel of Fig. The brightness changes of A and B are significantly greater than the observational noise level in the record of S3, which is appreciably fainter than both quasar images.

In addition, the almost parallel behaviour ofA and B indicates the presence of intrinsic variations.

Regarding the extrinsic signal in the r-band, the DLC and the single-epoch differences are shown in the bottom panel of Fig. It is apparent that the DLC values basically agree with single-epoch differences close to them.

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Only bins including two or moredata have been taken into account to compute differences between A and B. We also show the single-epochmagnitude differences grey data points , as well as the single-epoch flux ratio of the Mg II emission line in magnitudes horizontal dashed line.

As usual, the clean 2D profile of the H star was considered as the empirical PSF and the lens system was modelled as two stellar-like sources i. Ut in ultrices risus. Etiam aliquet magna velit, in sodales eros vulputate tempus. Phasellus eu sodales est. Nullam mollis augue at purus iaculis porta. Etiam scelerisque volutpat nisl sit amet tempus. Morbi feugiat tellus quis ipsum tempor, id tempus mauris fringilla. Donec justo ipsum, sodales in cursus vitae, molestie sed sapien.

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The engraved look of the detail makes me think that it's probably custom lettering, but with font design as intricate as it is these days, I figured even for a book that's been around since , that there might be such a font. Rogue Sans Ext Light. You agree to treat the Font Software as you would any other copyrighted material, such as a book. Myriad Pro-Semibold Semi Ext.

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