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20082024
most citedLight Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis

839 citations · 2k across the 32 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2024★ 14 cited

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★ 6 cited

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.GA2023★ 8 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.HE2023★ 25 cited

Discovery of the luminous X-ray ignition eRASSt J234402.9352640; I. Tidal disruption event or a rapid increase in accretion in an active galactic nucleus?

D. Homan, M. Krumpe, A. Markowitz +17

In November 2020, a new, bright object, eRASSt J234402.9352640, was discovered in the second all-sky survey of SRG/eROSITA. The object brightened by a factor of at least 150 in…

astro-ph.HE2023★ 17 cited

eRASSt J074426.3+291606: prompt accretion disc formation in a 'faint and slow' tidal disruption event

A. Malyali, Z. Liu, A. Merloni +10

We report on multi-wavelength observations of the tidal disruption event (TDE) candidate eRASSt J074426.3+291606 (J0744), located in the nucleus of a previously quiescent galaxy at…

astro-ph.HE2022★ 17 cited

X-ray emission from a rapidly accreting narrow-line Seyfert 1 galaxy at z=6.56

Julien Wolf, Kirpal Nandra, Mara Salvato +14

This study aims at identifying luminous quasars at among X-ray-selected sources in the eROSITA Final Equatorial-Depth Survey (eFEDS) in order to place a lower limit on blac…

astro-ph.HE2022★ 73 cited

Deciphering the extreme X-ray variability of the nuclear transient eRASSt J045650.3-203750: A likely repeating partial tidal disruption event

Zhu Liu, A. Malyali, M. Krumpe +17

(Abridged) In this paper, we present the results of an exceptional repeating X-ray nuclear transient, eRASSt J045650.3-203750 (hereafter J0456-20), uncovered by SRG/eROSITA in a qu…

astro-ph.HE2022★ 19 cited

Spectacular 240 kpc double-sided relativistic jets in a spiral-hosted narrow-line Seyfert 1 galaxy

A. Vietri, E. Järvelä, M. Berton +4

Narrow-line Seyfert 1 (NLS1) galaxies are a peculiar subclass of active galactic nuclei (AGN). They have demonstrated that the presence of relativistic jets in an AGN is not strict…

astro-ph.GA2020★ 14 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.HE2017★ 839 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.HE2017★ 342 cited

Early Spectra of the Gravitational Wave Source GW170817: Evolution of a Neutron Star Merger

B. J. Shappee, J. D. Simon, M. R. Drout +33

On 2017 August 17, Swope Supernova Survey 2017a (SSS17a) was discovered as the optical counterpart of the binary neutron star gravitational wave event GW170817. We report time-seri…

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.GA2017★ 26 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.SR2017★ 77 cited

Blue large-amplitude pulsators as a new class of variable stars

P. Pietrukowicz, W. A. Dziembowski, M. Latour +13

Regular intrinsic brightness variations observed in many stars are caused by pulsations. These pulsations provide information on the global and structural parameters of the star. T…

astro-ph.SR2016★ 8 cited

A Profile Analysis of Raman-scattered O VI Bands at 6825 Å and 7082 Å in Sanduleak's Star

Jeong-Eun Heo, Rodolfo Angeloni, Francesco Di Mille +2

We present a detailed modeling of the two broad bands observed at 6825 Å and 7082 Å in Sanduleak's star, a controversial object in the Large Magellanic Cloud. These bands are known…

astro-ph.GA2016★ 110 cited

A spectroscopic analysis of a sample of narrow-line Seyfert 1 galaxies selected from the Sloan Digital Sky Survey

V. Cracco, S. Ciroi, M. Berton +4

We revisited the spectroscopic characteristics of narrow-line Seyfert 1 galaxies (NLS1s) by analysing a homogeneous sample of 296 NLS1s at redshift between 0.028 and 0.345, extract…

astro-ph.GA2015★ 1 cited

Exploring the parent population of beamed NLS1s: from the black hole to the jet

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

The aim of this work is to understand the nature of the parent population of beamed narrow-line Seyfert 1 galaxies (NLS1s), by studying the physical properties of three parent cand…

astro-ph.GA2015

Formation of Raman Scattering Wings around H alpha, H beta and Pa alpha in Active Galactic Nuclei

Seok-Jun Chang, Jeong-Eun Heo, Francesco Di Mille +3

Powered by a supermassive black hole with an accretion disk, the spectra of active galactic nuclei (AGNs) are characterized by prominent emission lines including Balmer lines. The…

astro-ph.GA2015★ 50 cited

[O III] line properties in two samples of radio-emitting narrow-line Seyfert 1 galaxies

M. Berton, L. Foschini, S. Ciroi +4

The [O III] 4959,5007 lines are a useful proxy to test the kinematic of the narrow-line region (NLR) in active galactic nuclei (AGN). In AGN, and particularly in narrow-line S…

astro-ph.CO2013

Are Boltzmann Plots of Hydrogen Balmer lines a tool for identifying a subclass of S1 AGN?

P. Rafanelli, S. Ciroi, V. Cracco +4

It is becoming clear that we can define two different types of nearby AGN belonging to the Seyfert 1 class (S1), on the basis of the match of the intensities of their Broad Balmer…

astro-ph.GA2013★ 2 cited

The optical emission lines of type 1 X-ray bright Active Galactic Nuclei

G. La Mura, M. Berton, S. Ciroi +3

A strong X-ray emission is one of the defining signatures of nuclear activity in galaxies. According to the Unified Model for Active Galactic Nuclei (AGN), both the X-ray radiation…

astro-ph.SR2013★ 35 cited

X-Ray Grating Observations of Recurrent Nova T Pyxidis During The 2011 Outburst

Benjamin M. Tofflemire, Marina Orio, Kim L. Page +5

The recurrent nova T Pyx was observed with the X-ray gratings of Chandra and XMM-Newton, 210 and 235 days, respectively, after the discovery of the 2011 April 14 outburst. The X-ra…

astro-ph.SR2013★ 16 cited

Symbiotic Stars in OGLE Data I. Large Magellanic Cloud Systems

R. Angeloni, C. E. Ferreira Lopes, N. Masetti +10

Symbiotic stars are long-orbital-period interacting-binaries characterized by extended emission over the whole electromagnetic range and by complex photometric and spectroscopic va…

astro-ph.SR2013★ 12 cited

On the nature of CP Pup

Elena Mason, Marina Orio, Koji Mukai +6

We present new X-ray and optical spectra of the old nova CP Pup (nova Pup 1942) obtained with Chandra and the CTIO 4m telescope. The X-ray spectrum reveals a multi-temperature opti…