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arXiv · 2202.00186

The DIVING$^{3D}$ Survey -- Deep IFS View of Nuclei of Galaxies -- I. Definition and Sample Presentation

J. E. Steiner·R. B. Menezes·T. V. Ricci·Patrícia da Silva·R. Cid Fernandes·N. Vale Asari·M. S. Carvalho·D. May·Paula R. T. Coelho·A. L. de Amorim
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Abstract

We present the Deep Integral Field Spectrograph View of Nuclei of Galaxies (DIVING$^{3D}$) survey, a seeing-limited optical 3D spectroscopy study of the central regions of all 170 galaxies in the Southern hemisphere with B < 12.0 and |b| > 15 degrees. Most of the observations were taken with the Integral Field Unit of the Gemini Multi-Object Spectrograph, at the Gemini South telescope, but some are also being taken with the Southern Astrophysical Research Telescope (SOAR) Integral Field Spectrograph. The DIVING$^{3D}$ survey was designed for the study of nuclear emission-line properties, circumnuclear (within scales of hundreds of pc) emission-line properties, stellar and gas kinematics and stellar archaeology. The data have a combination of high spatial and spectral resolution not matched by previous surveys and will result in significant contributions for studies related to, for example, the statistics of low-luminosity active galactic nuclei, the ionization mechanisms in Low-Ionization Nuclear Emission-Line Regions, the nature of transition objects, among other topics.

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J. E. Steiner, R. B. Menezes, T. V. Ricci, Patrícia da Silva, R. Cid Fernandes, N. Vale Asari, M. S. Carvalho, D. May, Paula R. T. Coelho, A. L. de Amorim. 2022-02-01. The DIVING$^{3D}$ Survey -- Deep IFS View of Nuclei of Galaxies -- I. Definition and Sample Presentation. https://doi.org/10.1093/mnras/stac034

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