The second phase of the monitoring programme with the 2 m Liverpool Robotic Telescope (LRT) began in 2008 February and finished in 2010 July. This Liverpool Quasar Lens Monitoring (LQLM) II project was carried out with the RATCam optical CCD camera on the LRT, using griz Sloan  filters. The field of view and the pixel scale (binning 2 ´ 2) were ~ 4.6' ´ 4.6' and 0.278², respectively. In this almost final data-tools release, we include the frames of H1413+117 and Q0957+561 (LQLM ARCHIVE at GAVO, LRT DATA ARCHIVE or SEND A REQUEST TO US) as well as several outputs. In particular, a key subproject was the spectral follow-up of the predicted outburst in the B image of QSO 0957+561 in 2010 (ATel#2228). Apart from LRT frames of QSO 0957+561 (griz filters), we have also analyzed Swift/UVOT and Chandra exposures to properly understand the variability mechanism of the distant radio-loud quasar. This LQLM II data release also includes our two-band long-term monitoring of QSO 0957+561 (2005-2010; see below).

► H1413+117ABCD 

LIGHT CURVES     

● Time delays in the gravitationally lensed quasar H1413+117 (Cloverleaf)  (ApJ paper)

► Key subproject: X-ray, NUV, optical and NIR monitoring of QSO 0957+561B in 2010

● The Astronomer's Telegram: An opportunity for a multi-wavelength follow-up of a prominent event in the brightness of Q0957+561B in the first semester of 2010

● Time evolution of Q0957+561B in the ugriz filters (Swift/UVOT + LRT)                                                      

● Accretion onto the Supermassive Black Hole in the High-redshift Radio-loud AGN 0957+561 (ApJ paper)

● AHAR2011: The Central Kiloparsec in Galactic Nuclei: Astronomy at High Angular Resolution 2011 (Bad Honnef, Germany, August 29 - September 2, 2011)

[Time (MJD-50000), S_A (mJy), s(S_A), S_B (mJy), s(S_B)]:

- UV (U band)

- optical (g band & r band)

- IR (i band & z band)

► Global photometric follow-up of QSO 0957+561

● A 5.5-year robotic optical monitoring of Q0957+561: substructure in a non-local cD galaxy (A&A paper)

- ReadMe

- Table 1: Fluxes in the g band (4686 Å)

- Table 2: Fluxes in the r band (6165 Å)

- Time delays from the Liverpool main fluctuations (see A&A paper):

resampled g-band light curves (45 data points): Q0957+561A and Q0957+561B

Figure of A(+ 417 days) & B in the g band (EPS file)

AB cross-correlation (filled circles) & average autocorrelation (+ 417 days; open circles) in the g band for α = 6 days (EPS file)

AB cross-correlation (filled circles) & average autocorrelation (+ 417 days; open circles) in the g band for α = 9 days (EPS file)

resampled r-band light curves (45 data points): Q0957+561A and Q0957+561B

Figure of A(+ 417 days) & B in the r band (EPS file)

AB cross-correlation (filled circles) & average autocorrelation (+ 417 days; open circles) in the r band for α = 6 days (EPS file)

AB cross-correlation (filled circles) & average autocorrelation (+ 417 days; open circles) in the r band for α = 9 days (EPS file)

► SDSS1001+5027AB 

● Light curves in the g band (February-May 2010)

► SDSS1339+1310AB 

● Light curves in the r band (February-July 2009)

► Global perspectives (reviews)

● Robotic Monitoring of Gravitationally Lensed Quasars (Advances in Astronomy paper)

● The Mechanism of Intrinsic Variability in Bright Gravitationally Lensed Quasars at 1 < z < 2 (The Open Astronomy Journal paper)

● IAUS285: IAU Symposium 285: New Horizons in Time Domain Astronomy (Oxford, UK, September 19-23, 2011)