most citedHigh resolution spectroscopy of the extended narrow-line region of IC 5063 and NGC 7212

26 citations · 26 across the 3 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2017

Models of emission line profiles and spectral energy distributions to characterize the multi-frequency properties of active galactic nuclei

Giovanni La Mura, Marco Berton, Sina Chen +7

The spectra of Active Galactic Nuclei (AGNs) are often characterized by a wealth of emission lines with different profiles and intensity ratios that led to a complicated classifica…

astro-ph.GA2017

Multi-frequency databases for AGN investigation - Results and perspectives

Giovanni La Mura, Marco Berton, Sina Chen +5

Active Galactic Nuclei (AGNs) are characterized by emission of radiation over more than 10 orders of magnitude in frequency. Therefore, the execution of extensive surveys of the sk…

astro-ph.GA2017

Extended narrow-line region in Seyfert galaxies

Enrico Congiu, Marcella Contini, Stefano Ciroi +7

We present our recent results about the extended narrow-line region (ENLR) of two nearby Seyfert 2 galaxies (IC 5063 and NGC 7212) obtained by modelling the observed line profiles…

astro-ph.GA201726 cited

High resolution spectroscopy of the extended narrow-line region of IC 5063 and NGC 7212

E. Congiu, M. Contini, S. Ciroi +6

We studied the properties of the gas of the extended narrow line region (ENLR) of two Seyfert 2 galaxies: IC 5063 and NGC 7212. We analysed high resolution spectra to investigate h…

astro-ph.GA2017

Kiloparsec-scale emission in the narrow-line Seyfert 1 galaxy Mrk 783

E. Congiu, M. Berton, M. Giroletti +12

We present the first results of a radio survey of 79 narrow-line Seyfert 1 (NLS1) carried out with the Karl G. Jansky Very Large Array (JVLA) at 5 GHz in A configuration aimed at s…

astro-ph.GA2016

Unveiling the parent population of beamed narrow-line Seyfert 1s

M. Berton, L. Foschini, S. Ciroi +11

Narrow-line Seyfert 1 galaxies (NLS1s) are active galactic nuclei (AGN) recently identified as a new class of -ray sources. The high energy emission is explained by the presence…