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20242026
most citedChemical abundances along the quasar main sequence

17 citations · 31 across the 18 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA2026

Mapping the Quasar Main Sequence in the UV range: A Connection with the UV Fe III Emission

D. Martínez Collipal, M. L. Martínez-Aldama, A. Pandey +3

The quasar main sequence (MS) provides a consistent unification scheme for type I AGNs. This framework, constructed from the relative flux between the optical emissions $\mathrm{H}…

astro-ph.GA2026

Observations of a Possible Transient Magnetically Arrested Accretion State in a Nearby Quasar: OQ208

Brian Punsly, Cormac Reynolds, Paola Marziani +12

OQ208 is a nearby, partially obscured quasar (z=0.077) that is a young, bright, parsec scale radio source. We assemble archival and new high frequency VLBA and VLA observations and…

astro-ph.CO2026

Preliminary cosmological results using extreme accretors Quasar formalism

Rodrigo Sandoval-Orozco, Castalia Alenka Negrete, Paola Marziani +1

We revisited the xA Quasar formalism from the cosmological point of view, where a completely cleaned and standardized sample is compiled from different literature references. This…

astro-ph.GA2026

Spectral Evolution and Transient Broad-Line Features in the Isolated AGN UNAM-KIAS 613

Edgar Cortes-Suárez, Paola Marziani, Héctor Manuel Hernández-Toledo +2

We present multi-epoch optical spectroscopy of the isolated elliptical galaxy UNAM-KIAS 613, hosting a low-luminosity Type 1 AGN. Analysis of archival Sloan Digital Sky Survey (SDS…

astro-ph.GA2026★ 1 cited

Investigating the origin of radio emission in candidate super-Eddington accreting black holes

Marie-Lou Gendron-Marsolais, Paola Marziani, Marco Berton +8

Recent works show that the radio power of quasars accreting at very high rates can reach surprisingly high values. These studies suggest that this radio emission might originate fr…

astro-ph.GA2026

AGN Variability with Rubin Observatory in the 2030s

Swayamtrupta Panda, Francisco Pozo Nuñez, Hygor Benati Gonçalves +4

AGN variability offers a direct probe of accretion physics, disk structure, and black hole growth, but progress has been limited by sample size, cadence heterogeneity, and photomet…