Old Q0957+561 data & software: ► Simple FORTRAN programs to apply the d2 test (accurate and robust time delay measurements)
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Old Q0957+561 data & software: ► Simple FORTRAN programs to apply the d2 test (accurate and robust time delay measurements)
► Photos
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● g-SDSS: QSO 0957+561A & QSO 0957+561B QSO 0957+561A (including fluxes from some frames with 80 < SNR < 100) ● r-SDSS: QSO 0957+561A & QSO 0957+561B New two-colour light curves of Q0957+561: time delays and origin of intrinsic variations (A&A) Structure function of the UV variability of Q0957+561 (A&A) ● Press Release: Mystery Of Twin Quasar Brightness Revealed ● 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 in 2010 (Swift/UVOT + LRT) Accretion onto the Supermassive Black Hole in the High-redshift Radio-loud AGN 0957+561 (ApJ) Continuum reverberation mapping in a z = 1.41 radio-loud QSO (J. Phys. Conf. Ser.) ● Relevant datasets for Q0957+561B in 2010 [Time (MJD-50000), Flux (10-12 erg s-1 cm-2 in X-rays and mJy in UV/optical bands), Error in flux]: - X-ray (absorbed power-law & unabsorved power-law) - UV (U band) ● Q0957+561A and Q0957+561B from NUV to NIR (2010) [Time (MJD-50000), SA (mJy), s(SA), SB (mJy), s(SB)]:- UV (U band) A 5.5-year robotic optical monitoring of Q0957+561: substructure in a non-local cD galaxy (A&A) ● Global dataset: - ReadMe - Table 1: Fluxes in the g band (4686 Å) - Table 2: Fluxes in the r band (6165 Å) - On the time delays from the Liverpool main fluctuations: resampled g-band light curves (45 data points): Q0957+561A and Q0957+561B A(+ 417 days) & B [left panel], as well as AB cross-correlation (filled circles) & average autocorrelation (+ 417 days; open circles) for α = 6 days [middle panel] and a = 9 days [right panel]: resampled r-band light curves (45 data points): Q0957+561A and Q0957+561B A(+ 417 days) & B [left panel], as well as AB cross-correlation (filled circles) & average autocorrelation (+ 417 days; open circles) for α = 6 days [middle panel] and a = 9 days [right panel]:
Spectra of faint sources in crowded fields with FRODOSpec on the Liverpool Robotic Telescope (Astron. Nachr.) Polarimetric monitoring with RINGO since 2011 LT + IAC80 light curves in 1996–2016 (21 years) A = red circles B = blue squares
LT light curves in 2005–2014 (10 years): suitable scale factors and time shifts are used to show the agreement/disagreement between A and B
New database for a sample of optically bright lensed quasars in the northern hemisphere (A&A) ● Datasets: – Table 6: IAC80-LT light curves in the r band [1067 epochs in 1996-2016] -------------------------------------------------------------------------------- – Table 8: LT/FRODOSpec (red grating) spectra [16 epochs in 2010-2014] Subtables: 8a, 8b, 8c, 8d, 8e, 8f, 8g, 8h, 8i, 8j, 8k, 8l, 8m, 8n, 8o, 8p Observing dates (yyyymmdd): a = 20101105, b = 20101109, c = 20101223, d = 20110109, e = 20110109, f = 20110224, g = 20110301, h = 20110410, i = 20110530, j = 20111024, k = 20111101, l = 20111205, m = 20111218, n = 20111221, o = 20130220, p = 20140104
-------------------------------------------------------------------------------- – Table 9: LT/SPRAT spectra [5 epochs in 2015-2017] Observing dates (yyyymmdd): a = 20150315, b = 20151119, c = 20151121, d = 20170117, e = 20170118
-------------------------------------------------------------------------------- – Tables 10-11: NOT/ALFOSC spectra [3 epochs in 2010-2013] Subtables 10 (grism 7): 10a, 10b, 10c Subtables 11 (grism 14): 11a, 11b, 11c
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