Main.AGN History
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I actively develop the use of microlensing produced by stars in lensing galaxy to study the inner regions of distant AGNs. I am working on both observational and modeling aspects. I performed detailed studies of the micro-lensed induced spectral deformation of several lensed quasars based on single epoch spectra and based on spectro-photometric monitoring data (Sluse et al. 2007, 2011, 2012b). These works allowed me to derive interesting constraints on the ''structure of the BLR''
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I actively develop the use of microlensing produced by stars in lensing galaxies to study the inner regions of distant AGNs. I work on both observational and modeling aspects. I performed detailed studies of the micro-lensed induced spectral deformation of several lensed quasars based on single epoch spectra and based on spectrophotometric monitoring data (Sluse et al. 2007, 2011, 2012b). These works allowed me to derive interesting constraints on the ''structure of the Broad Line Region''
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%lframe thumb% Attach:BLRmicro.jpg | Example of microlensing event allowing to reproduce the microlensing of the accretion disc continuum emission (red) and of the CIV emission line (black) in the Einstein Cross Q2237-0305
%rframe thumb% Attach:BLRsize.jpg | Size of the CIV emission line in Q2237+0305, as derived with microlensing, compared with sizes derived in local objects using the reverberation mapping technique (blue).
%rframe thumb% Attach:BLRsize.jpg | Size of the CIV emission line in Q2237+0305, as derived with microlensing, compared with sizes
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%lframe width=300px% Attach:BLRmicro.jpg | Example of microlensing event allowing to repro- [[<<]] duce the microlensing of the accretion disc conti- [[<<]] nuum emission (red) and of the CIV emission line [[<<]] (black) in the Einstein Cross Q2237-0305
%lframe width=300px% Attach:BLRsize.jpg | Size of the CIV emission line in Q2237+0305,[[<<]] as derived with microlensing, compared with sizes [[<<]]derived in local objects using the reverberation [[<<]] mapping technique (blue).
%lframe width=300px% Attach:BLRsize.jpg | Size of the CIV emission line in Q2237+0305,[[<<]] as derived with microlensing, compared with sizes [[<<]]derived in local objects using the reverberation [[<<]] mapping technique (blue).
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for different emission lines (Balmer lines, MgII, FeII) as well as on the ''structure of the absorbing outflow'' in a broad absorption line quasar (Hutsemékers et al. 2010).
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for different emission lines (Balmer lines, MgII, FeII) as well as on the ''structure of the absorbing outflow'' in a broad absorption line quasar (Hutsemékers et al. 2010).
%lframe thumb% Attach:BLRmicro.jpg | Example of microlensing event allowing to reproduce the microlensing of the accretion disc continuum emission (red) and of the CIV emission line (black) in the Einstein Cross Q2237-0305
%rframe thumb% Attach:BLRsize.jpg | Size of the CIV emission line in Q2237+0305, as derived with microlensing, compared with sizes derived in local objects using the reverberation mapping technique (blue).
%lframe thumb% Attach:BLRmicro.jpg | Example of microlensing event allowing to reproduce the microlensing of the accretion disc continuum emission (red) and of the CIV emission line (black) in the Einstein Cross Q2237-0305
%rframe thumb% Attach:BLRsize.jpg | Size of the CIV emission line in Q2237+0305, as derived with microlensing, compared with sizes derived in local objects using the reverberation mapping technique (blue).
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(:title Study of Active Galactic Nucleii with Microlensing:)
I actively develop the use of microlensing produced by stars in lensing galaxy to study the inner regions of distant AGNs. I am working on both observational and modeling aspects. I performed detailed studies of the micro-lensed induced spectral deformation of several lensed quasars based on single epoch spectra and based on spectro-photometric monitoring data (Sluse et al. 2007, 2011, 2012b). These works allowed me to derive interesting constraints on the ''structure of the BLR''
for different emission lines (Balmer lines, MgII, FeII) as well as on the ''structure of the absorbing outflow'' in a broad absorption line quasar (Hutsemékers et al. 2010).
I actively develop the use of microlensing produced by stars in lensing galaxy to study the inner regions of distant AGNs. I am working on both observational and modeling aspects. I performed detailed studies of the micro-lensed induced spectral deformation of several lensed quasars based on single epoch spectra and based on spectro-photometric monitoring data (Sluse et al. 2007, 2011, 2012b). These works allowed me to derive interesting constraints on the ''structure of the BLR''
for different emission lines (Balmer lines, MgII, FeII) as well as on the ''structure of the absorbing outflow'' in a broad absorption line quasar (Hutsemékers et al. 2010).