activity
20152022
most citedA treatment procedure for VLT/SINFONI data cubes: application to NGC 5643

43 citations · 185 across the 9 of their papers we have counts for

collaborators

9 papers

astro-ph.GA2022★ 8 cited

The DIVING Survey -- Deep IFS View of Nuclei of Galaxies -- I. Definition and Sample Presentation

J. E. Steiner, R. B. Menezes, T. V. Ricci +7

We present the Deep Integral Field Spectrograph View of Nuclei of Galaxies (DIVING) survey, a seeing-limited optical 3D spectroscopy study of the central regions of all 170…

astro-ph.GA2020★ 8 cited

Digging process in NGC 6951: the molecular disc bumped by the jet

D. May, J. E. Steiner, T. V. Ricci +2

We present a study of the central 200 pc of the galaxy NGC 6951, SAB(rs)bc, an active twin of the Milky Way, at a distance of 24 Mpc. Its nucleus has been observed in the optical w…

astro-ph.GA2020★ 39 cited

A two-stage outflow in NGC 1068

D. May, J. E. Steiner

We present an analysis of the Seyfert 2 galaxy NGC 1068 with archive data from SINFONI-VLT, in the HK bands with pixel scales of 0.1 (data set 1 - DS1) and 0.025 (DS2) arcsec. The…

astro-ph.GA2020★ 20 cited

The nuclear architecture of NGC 4151: on the path toward a universal outflow mechanism in light of NGC 1068

D. May, J. E. Steiner, R. B. Menezes +2

We report near-infrared integral field spectroscopic observations of the active galactic nucleus NGC 4151 with archive data from the NIFS-Gemini North Telescope. We have selected b…

astro-ph.HE2020★ 11 cited

Constraining X-ray reflection in the low-luminosity AGN NGC 3718 using NuSTAR and XMM--Newton

Y. Diaz, P. Arévalo, L. Hernández-García +9

One distinctive feature of low-luminosity active galactic nuclei (LLAGN) is the relatively weak reflection features they may display in the X-ray spectrum, which can result from th…

astro-ph.GA2020★ 14 cited

The curious activity in the nucleus of NGC 4151: jet interaction causing variability?

D. R. A. Williams, R. D. Baldi, I. M. McHardy +14

A key characteristic of many active galactic nuclei (AGN) is their variability, but its origin is poorly understood, especially in the radio domain. Williams et al. (2017) reported…