NGC 5427 WiFeS data cubes

DOI

We have observed the nearby, nearly face-on, Seyfert 2 galaxy, NGC 5427, using optical integral field spectroscopy of both the nuclear regions and the HII regions in the spiral arms. The observed spectra have been modelled using the MAPPINGS IV photoionisation code, both to derive the chemical abundances in the HII regions and the Seyfert nucleus, and to constrain the EUV spectral energy distribution of the AGN illuminating the extended narrow-line region.

Cone search capability for table J/A+A/566/A41/list (List of data cubes)

Identifier
DOI http://doi.org/10.26093/cds/vizier.35660041
Source https://dc.g-vo.org/rr/q/lp/custom/CDS.VizieR/J/A+A/566/A41
Related Identifier https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/566/A41
Related Identifier http://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/566/A41
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_b2find&identifier=ivo://CDS.VizieR/J/A+A/566/A41
Provenance
Creator Dopita M.A.; Scharwachter J.; Shastri P.; Kewley L.J.; Davies R.,Sutherland R.; Kharb P.; Jose J.; Hampton E.; Jin C.; Banfield J.,Basurah H.; Fische S.
Publisher CDS
Publication Year 2014
Rights https://cds.unistra.fr/vizier-org/licences_vizier.html
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Resource Type Dataset; AstroObjects
Discipline Astrophysics and Astronomy; Galactic and extragalactic Astronomy; High Energy Astrophysics; Interdisciplinary Astronomy; Natural Sciences; Observational Astronomy; Physics