activity
20172024
most citedLight Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

839 citations · 964 across the 5 of their papers we have counts for

collaborators

8 papers

astro-ph.GA2024

The SRG/eROSITA All-Sky Survey: X-ray beacons at late cosmic dawn

J. Wolf, M. Salvato, S. Belladitta +12

The SRG/eROSITA All-Sky Survey (eRASS) is expected to contain ~100 quasars that emitted their light when the universe was less than a billion years old, i.e. at z>5.6. By selection…

astro-ph.SR2024

Observational Parameters of Blue Large-amplitude Pulsators

P. Pietrukowicz, M. Latour, I. Soszynski +15

Blue large-amplitude pulsators (BLAPs) are a recently discovered class of short-period pulsating variable stars. In this work, we present new information on these stars based on ph…

astro-ph.GA20238 cited

A host galaxy study of southern narrow-line Seyfert 1 galaxies

I. Varglund, E. Järvelä, S. Ciroi +4

We studied seven nearby narrow-line Seyfert 1 (NLS1) galaxies in - and -bands with redshifts varying from 0.019 to 0.092. This is the first multi-source study targeting the…

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.HE2017839 cited

Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

M. R. Drout, A. L. Piro, B. J. Shappee +41

On 2017 August 17, gravitational waves were detected from a binary neutron star merger, GW170817, along with a coincident short gamma-ray burst, GRB170817A. An optical transient so…

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…