Old Q0957+561 data & software: ► Simple FORTRAN programs to apply the d2 test (accurate and robust time delay measurements)
► Photos
Advertising: | LQLM III
The third phase of the monitoring programme with the 2 m Liverpool Robotic Telescope (LRT) began in 2010 October. This LQLM III project is being carried out with most of the available optical instruments: the RATCam and IO:O cameras, the FRODOspec spectrometer and the RINGO polarimeter, so it represents a final qualitative leap in our observational programme with the LRT. In addition, new observations with the world's largest ground-based telescopes and space-based facilities are used to complement the LQLM database. Here below we include a "News section" on some double quasars that are key monitoring targets. The figures show data for the two quasar images, A (red) and B (blue), and reference stars (black/green)
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