scispace - formally typeset
A

Ascensión del Olmo

Researcher at Spanish National Research Council

Publications -  46
Citations -  697

Ascensión del Olmo is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Quasar & Redshift. The author has an hindex of 14, co-authored 46 publications receiving 577 citations.

Papers
More filters
Journal ArticleDOI

Is Mg II 2800 a Reliable Virial Broadening Estimator for Quasars

TL;DR: In this article, a comparison of MgII 2800 and Hbeta profile measures in the same sources and especially FWHM measures that provide the virial broadening estimator was made.
Journal ArticleDOI

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.
Journal ArticleDOI

Low-ionization outflows in high eddington ratio quasars

TL;DR: In this paper, Sulentic et al. interpreted the Mg II {lambda}2800 blueshift as the signature of a radiation-driven wind or outflow in the highest accreting quasars.
Journal ArticleDOI

The Mice at play in the CALIFA survey - A case study of a gas-rich major merger between first passage and coalescence

Vivienne Wild, +56 more
TL;DR: In this article, optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (≳10^11 M_⊙) gas-rich spirals NGC 4676A and B, observed between first passage and final coalescence.
Journal ArticleDOI

GTC spectra of z ≈ 2.3 quasars: comparison with local luminosity analogs

TL;DR: In this article, the authors conducted a search for z-dependent gradients in line-emission diagnostics and derived physical properties by comparing, in a narrow bolometric luminosity range (log L ∼ 46.1± 0.4 [erg s −1 ]), some of the most luminous local z < 0.6 quasars with the lowest luminosity sources yet found at redshift z = 2.1−2.5.