54 citations · 128 across the 4 of their papers we have counts for
6 papers
The first 62 AGN observed with SDSS-IV MaNGA - IV: gas excitation and star-formation rate distributions
Janaína C. do Nascimento, Thaisa Storchi-Bergmann, Nícolas D. Mallmann +8
We present maps of the ionized gas flux distributions, excitation, star-formation rate SFR, surface mass density , and obtain total values of SFR and ionized gas masses {\i…
The first 62 AGN observed with SDSS-IV MaNGA -- III: stellar and gas kinematics
Gabriele S. Ilha, Rogemar A. Riffel, Jaderson S. Schimoia +13
We investigate the effects of Active Galactic Nuclei (AGN) on the gas kinematics of their host galaxies, using MaNGA data for a sample of 62 AGN hosts and 109 control galaxies (ina…
Precessing winds from the nucleus of the prototype Red Geyser?
Rogemar A. Riffel, Rodrigo Nemmen, Gabriele S. Ilha +10
Super-massive black holes (SMBH) are present at the center of most galaxies, with the related mass accretion processes giving origin to outflows in Active Galactic Nuclei (AGN). It…
The Fifteenth Data Release of the Sloan Digital Sky Surveys: First Release of MaNGA Derived Quantities, Data Visualization Tools and Stellar Library
D. S. Aguado, Romina Ahumada, Andres Almeida +230
Twenty years have passed since first light for the Sloan Digital Sky Survey (SDSS). Here, we release data taken by the fourth phase of SDSS (SDSS-IV) across its first three years o…
The first 62 AGN observed with SDSS-IV MaNGA - I: their characterization and definition of a control sample
Sandro B. Rembold, Jáderson S. Shimoia, Thaisa Storchi-Bergmann +16
We report the characterization of the first MaNGA Active Galactic Nuclei (AGN) hosts in the Fifth Product Launch (MPL-5) and the definition of a control sample of non-active g…
The origin of the near-IR line emission from molecular, low and high ionization gas in the inner kiloparsec of NGC6240
Gabriele S. Ilha, Marina Bianchin, R. A. Riffel
The understating of the origin of the H2 line emission from the central regions of galaxies represent an important key to improve our knowledge about the excitation and ionization…