activity
20062020
most citedDust Extinction of Gamma-ray Burst Host Galaxies: Identification of Two Classes?

38 citations · 90 across the 5 of their papers we have counts for

collaborators

7 papers

astro-ph.GA202014 cited

The Radio Structure of the Narrow-Line Seyfert 1 Mrk 783 with VLBA and e-MERLIN

E. Congiu, P. Kharb, A. Tarchi +9

In this paper, we present the analysis of new radio and optical observations of the narrow-line Seyfert 1 galaxy Mrk 783. 1.6 GHz observations performed with the e-MERLIN interfero…

astro-ph.GA202025 cited

Radio morphology of southern narrow-line Seyfert 1 galaxies with Very Large Array observations

S. Chen, E. Jarvela, L. Crepaldi +8

We present the results of new radio observations carried out with the Karl G. Jansky Very Large Array C-configuration at 5.5 GHz for a sample of southern narrow-line Seyfert 1 gala…

astro-ph.GA201913 cited

Broadband X-ray observations of four gamma-ray narrow-line Seyfert 1 galaxies

M. Berton, V. Braito, S. Mathur +4

Narrow-line Seyfert 1 galaxies (NLS1s) is one of the few classes of active galactic nuclei (AGN) harboring powerful relativistic jets and detected in rays. NLS1s are well-known…

astro-ph.GA2019

A correlation between [O III] line property and X-ray spectral complexity in narrow-line Seyfert 1 galaxies?

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

We present a detailed study of 11 narrow-line Seyfert 1 galaxies (NLS1s) from the Six-degree Field Galaxy Survey (6dFGS) that both have optical and X-ray spectroscopic observations…

astro-ph.HE2019

Fermi and Swift Observations of GRB 190114C: Tracing the Evolution of High-Energy Emission from Prompt to Afterglow

M. Ajello, M. Arimoto, M. Axelsson +147

We report on the observations of gamma-ray burst (GRB) 190114C by the Fermi Gamma-ray Space Telescope and the Neil Gehrels Swift Observatory. The early-time observations reveal mul…

astro-ph.HE2019

SN 2017gmr: An energetic Type II-P supernova with asymmetries

Jennifer E. Andrews, D. J. Sand, S. Valenti +77

We present high-cadence ultraviolet (UV), optical, and near-infrared (NIR) data on the luminous Type II-P supernova SN 2017gmr from hours after discovery through the first 180 days…