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The DIVING3D Survey - Deep IFS View of Nuclei of Galaxies

Published online by Cambridge University Press:  29 March 2021

J. E. Steiner ,
R. B. Menezes ,
T. V. Ricci Open the ORCID record for T. V. Ricci [Opens in a new window]  and
DIVING3D team
J. E. Steiner
Affiliation:
Instituto de Astronomia, Geofísica e Ciências Atmosféricas, Universidade de São Paulo, 05508-090, São Paulo, SP, Brasil email: joao.steiner@iag.usp.br
R. B. Menezes
Affiliation:
Instituto Mauá de Tecnologia, Praça Mauá 1, 09580-900, São Caetano do Sul, SP, Brasil
T. V. Ricci
Affiliation:
Universidade Federal da Fronteira Sul, Campus Cerro Largo, RS, 97900-000, Brasil
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Abstract

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The DIVING3D Survey (Deep Integral Field Spectrograph View of Nuclei of Galaxies) aims to observe, with high signal/noise and high spatial resolution, a statistically complete sample of southern galaxies brighter than B = 12.0 The main objectives of this survey are to study: 1) the nuclear emission line properties; 2) the circumnuclear emission line properties; 3) the central stellar kinematics and 4) the central stellar archaeology. Preliminary results of individual or small groups of galaxies have been published in 18 papers.

Keywords

galaxies: activegalaxies: nucleigalaxies: statisticsgalaxies: kinematics and dynamicsgalaxies: stellar contentgalaxies: Seyfertsurveys
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S359: Galaxy Evolution and Feedback across Different Environments , March 2019 , pp. 402 - 406
Copyright
© The Author(s), 2021. Published by Cambridge University Press on behalf of International Astronomical Union

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