activity
20092026
most citedPCA Tomography: how to extract information from datacubes

91 citations · 629 across the 44 of their papers we have counts for

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Showing astro-ph.COShow all

7 papers · 1 filter

astro-ph.CO2013★ 14 cited

Collimation and scattering of the active galactic nucleus emission in the Sombrero galaxy

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

We present an analysis of a data cube of the central region of M104, the Sombrero galaxy, obtained with the GMOS-IFU of the Gemini-South telescope, and report the discovery of coll…

astro-ph.CO2012★ 16 cited

Discovery of an Halpha emitting disk around the supermassive black hole of M31

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

Due to its proximity, the mass of the supermassive black hole in the nucleus of Andromeda galaxy (M31), the most massive black hole in the Local Group of galaxies, has been measure…

astro-ph.CO2011★ 19 cited

NGC 7097: the AGN and its mirror, revealed by PCA Tomography

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

Three-dimensional (3D) spectroscopy techniques are becoming more and more popular, producing an increasing number of large data cubes. The challenge of extracting information from…

astro-ph.CO2010

The nature of the LINER in the galaxy NGC 404

Roberto B. Menezes, João E. Steiner, Tiago V. Ricci +1

NGC 404, at a distance of 3.4 Mpc, is the nearest S0 galaxy. This galaxy harbors a LINER; however, since the spectrum does not show a broad Hα emission, it is not certain that this…

astro-ph.CO2010

Stellar archeology of the nearby LINER galaxies NGC 4579 and NGC 4736

J. E. Steiner, R. B. Menezes, T. V. Ricci +1

Stellar archeology of nearby LINER galaxies may reveal if there is a stellar young population that may be responsible for the LINER phenomenon. We show results for the classical LI…

astro-ph.CO2010

The stellar populations of the AGN/Starburst galaxy NGC7582

T. V. Ricci, J. E. Steiner, R. B. Menezes +2

NGC 7582 is defined as a Starburst/AGN galaxy, since its optical and X-Ray spectra reveal both characteristics. In this work, we show the results of a stellar population modeling i…