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Mary Loli Martínez-Aldama

Researcher at Polish Academy of Sciences

Publications -  63
Citations -  1009

Mary Loli Martínez-Aldama is an academic researcher from Polish Academy of Sciences. The author has contributed to research in topics: Quasar & Redshift. The author has an hindex of 16, co-authored 58 publications receiving 733 citations. Previous affiliations of Mary Loli Martínez-Aldama include National Autonomous University of Mexico & Spanish National Research Council.

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A Main Sequence for Quasars

TL;DR: In this article, the empirical correlates of the so-called "main sequence" associated with the quasar Eigenvector 1, its governing physical parameters and several implications on the view of quasar structure, as well as some luminosity effects associated with a virialized component of the line emitting regions.
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What does CIVλ1549 tell us about the physical driver of the Eigenvector quasar sequence

TL;DR: In this paper, the authors used broad emission lines in quasars to resolve the structure and kinematics of the broad-line emitting region (BLR) thought to involve an accretion disk feeding a supermassive black hole.
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What does Civ{\lambda}1549 tell us about the physical driver of the Eigenvector Quasar Sequence?

TL;DR: In this paper, the authors used broad emission lines in quasars to resolve the structure and kinematics of the broad line emitting region (BLR) thought to in-volve an accretion disk feeding a supermassive black hole.
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Can Reverberation-measured Quasars Be Used for Cosmology?

TL;DR: In this article, a correction for the time delay based on the dimensionless accretion rate considering the virial factor anti-correlated with the FWHM of H$\beta was proposed.
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Highly accreting quasars: The SDSS low-redshift catalog

TL;DR: The most highly accreting quasars (xA) are of special interest in studies of the physics of AGNs and host galaxy evolution, and their observational properties are largely unknown as mentioned in this paper.