Revealing the non-linear behaviour of the lensed quasar Q0957+561
Knowledge about how the non-linear behaviour of the intrinsic signal from lensed background sources changes on its path to the observer provides much information, particularly about the matter distribution in lensing galaxies and the physical properties of the current universe, in general. Here,...
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| Principais autores: | , , , |
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| Formato: | article |
| Idioma: | English |
| Publicado em: |
Oxford University Press (OUP)
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| Assuntos: | |
| Endereço do item: | https://repositorio.ufrn.br/jspui/handle/123456789/29454 http://dx.doi.org/10.1093/mnras/stz203 |
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| Resumo: | Knowledge about how the non-linear behaviour of the intrinsic signal from lensed background
sources changes on its path to the observer provides much information, particularly about
the matter distribution in lensing galaxies and the physical properties of the current universe,
in general. Here, we analyse the multifractal behaviour of the optical observations of A and
B images of Q0957+561 in the r and g bands. Aims: To verify the presence, or absence,
of extrinsic variations in the observed signals of the quasar images and whether extrinsic
variations affect the multifractal behaviour of their intrinsic signals. Method: We apply a
wavelet transform modulus maxima-based multifractality analysis approach. Results: We
detect strong multifractal signatures in the light curves of the quasar images. The degree of
multifractality for both images in the r band changes over time in a non-monotonic way,
indicating the presence of extrinsic variabilities in the light curves of the images. Additionally,
in the r band, in periods of quiescent microlensing activity, we find that the degree of
multifractality of image A is stronger than that of B, while B has a larger multifractal strength
in recent epochs when it appears to be affected by microlensing. Finally, comparing the optical
bands in a period of quiescent microlensing activity, we find that the degree of multifractality
is stronger in the r band for both quasar images. In the absence of microlensing, the observed
excesses of non-linearity are most likely generated when the broad-line region reprocesses the
radiation from the compact sources. |
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