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20172022
most citedNGC 1566: analysis of the nuclear region from optical and near-infrared Integral Field Unit spectroscopy

35 citations · 91 across the 5 of their papers we have counts for

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6 papers · 1 filter

astro-ph.GA20228 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.GA202012 cited

The nuclear region of NGC 613. I -- Multiwavelength analysis

Patrícia da Silva, Roberto B. Menezes, João E. Steiner

In this paper, we report a detailed study with a variety of data from optical, near-infrared, X-ray, and radio telescopes of the nuclear region of the galaxy NGC 613 with the aim o…

astro-ph.GA201927 cited

A treatment procedure for GMOS/IFU data cubes: application to NGC 2835

R. B. Menezes, T. V. Ricci, J. E. Steiner +3

We present a set of treatment techniques for GMOS/IFU data cubes, including: correction of the differential atmospheric refraction; Butterworth spatial filtering, to remove high sp…

astro-ph.GA2018

NGC 6744 - A nearby Milky Way twin with a very low-luminosity AGN

Patrícia da Silva, J. E. Steiner, R. B. Menezes

NGC 6744 is the nearest and brightest south-hemisphere galaxy with a morphological type similar to that of the Milky Way. Using data obtained with the Integral Field Unit of the Ge…

astro-ph.GA20179 cited

The molecular H2 and stellar discs in the nuclear region of NGC 4258

R. B. Menezes, J. E. Steiner, Patrícia da Silva

NGC 4258 is an SABbc Seyfert galaxy, located at a distance of Mpc. This object is well known by its nearly edge-on molecular nuclear disc, located between 0.16 and 0.…

astro-ph.GA201735 cited

NGC 1566: analysis of the nuclear region from optical and near-infrared Integral Field Unit spectroscopy

Patrícia da Silva, J. E. Steiner, R. B. Menezes

We analysed the centre of NGC 1566, which hosts a well-studied active galactic nucleus (AGN), known for its variability. With the aid of techniques such as Principal Component Anal…