出版社:SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要:We present the results of the first long-term (2.2 years) spectroscopic monitoring of a gravitationally
lensed quasar, namely the Einstein Cross QSO 2237+0305.
We spatially deconvolve deep VLT/FORS1 spectra to accurately separate the spectrum of the lensing
galaxy from the spectra of the quasar images. Accurate cross-calibration of the observations
at 31 epochs from October 2004 to December 2006 is carried out using foreground stars observed
simultaneously with the quasar. The quasar spectra are further decomposed into a continuum
component and several broad emission lines.
We find prominent microlensing events in the quasar images A and B, while images C and D are
almost quiescent on a timescale of a few months. The strongest variations are observed in the
continuum, and their amplitude is larger in the blue than in the red, consistent with microlensing
of an accretion disk. Variations in the intensity and profile of the broad emission lines are also
reported, most prominently in the wings of the C III] and in the center of the C IV emission lines.
During a strong microlensing episode observed in quasar image A, the broad component of the
C III] is more magnified than the narrow component. In addition, the emission lines with higher
ionization potentials are more magnified than the lines with lower ionization potentials, consistent
with the stratification of the broad line region (BLR) infered from reverberation mapping
observations.