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20152026
most citedA kilonova as the electromagnetic counterpart to a gravitational-wave source

888 citations · 1.4k across the 41 of their papers we have counts for

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Showing 2018Show all

9 papers · 1 filter

astro-ph.GA2018★ 2 cited

Fe II velocity shifts in optical spectra of type 1 AGN

E. Bon, P. Marziani, M. Berton +4

Here we present a critical view of practical problems in the analysis of optical Fe II emission lines of Type 1 AGN spectra. Besides the very complex and unclear physical interpret…

astro-ph.GA2018

The link between X-ray complexity and optical lines in NLS1s

A. Vietri, M. Berton, S. Ciroi +8

Narrow-line Seyfert 1 galaxies (NLS1s) are a subclass of active galactic nuclei (AGN). It is often believed that these AGN have small black hole mass, which is responsible for the…

astro-ph.GA2018

A catalog of narrow-line Seyfert 1 galaxies in the southern hemisphere

S. Chen, M. Berton, G. La Mura +7

We present a new accurate sample of narrow-line Seyfert 1 galaxies (NLS1s) in the southern hemisphere from the Six-degree Field Galaxy Survey (6dFGS). Based on the optical spectral…

astro-ph.GA2018

Models of Optical Emission Lines To Investigate Narrow-Line Seyfert 1 Galaxies in Spectroscopic Databases

G. La Mura, D. Bastieri, M. Berton +6

Thanks to the execution of extensive spectroscopic surveys that have covered large fractions of the sky down to magnitudes as faint as , it has been possible to ident…

astro-ph.SR2018

SN 2017ens: The Metamorphosis of a Luminous Broad-lined Type Ic Supernova into an SN IIn

T. -W. Chen, C. Inserra, M. Fraser +46

We present observations of supernova (SN) 2017ens, discovered by the ATLAS survey and identified as a hot blue object through the GREAT program. The redshift z=0.1086 implies a pea…

astro-ph.GA2018

Near-infrared morphologies of the host galaxies of narrow-line Seyfert 1 galaxies

Emilia Järvelä, Anne Lähteenmäki, Marco Berton

We present -band near-infrared (NIR) imaging of the host galaxies of nine narrow-line Seyfert 1 galaxies (NLS1). Based on high-frequency radio observations at 37~GHz, seven of t…