We make use of the statistical power of the MaNGA survey, which has observed ~10000 galaxies, to build a large sample of counter-rotators. The Integral-Field Spectroscopy (IFS) data used in this study are taken from the Data Release 16 (DR16; Ahumada et al. 2020ApJS..249....3A, Cat. V/154) of the MaNGA survey. DR16 includes IFS data for 4597 unique galaxies observed in the redshift range 0.01 < z < 0.15. The physical properties of these 4597 galaxies (e.g. morphological classification, mass, ellipticity etc.) used in this paper were kindly provided by Mark Graham, the tableg18.dat and refer to Graham et al. (2019arXiv191005139G) for a detailed description of how the properties have been measured (i.e see also Graham et al. 2018MNRAS.477.4711G, Cat. J/MNRAS/477/4711).
Bevacqua, D., Cappellari, M., Pellegrini, S. (2025). VizieR Online Data Catalog: CRDs galaxies candidates in SDSS-IV MaNGA (Bevacqua+, 2022) [10.26093/cds/vizier.75110139].
VizieR Online Data Catalog: CRDs galaxies candidates in SDSS-IV MaNGA (Bevacqua+, 2022)
Bevacqua, D.;Pellegrini, S.
2025
Abstract
We make use of the statistical power of the MaNGA survey, which has observed ~10000 galaxies, to build a large sample of counter-rotators. The Integral-Field Spectroscopy (IFS) data used in this study are taken from the Data Release 16 (DR16; Ahumada et al. 2020ApJS..249....3A, Cat. V/154) of the MaNGA survey. DR16 includes IFS data for 4597 unique galaxies observed in the redshift range 0.01 < z < 0.15. The physical properties of these 4597 galaxies (e.g. morphological classification, mass, ellipticity etc.) used in this paper were kindly provided by Mark Graham, the tableg18.dat and refer to Graham et al. (2019arXiv191005139G) for a detailed description of how the properties have been measured (i.e see also Graham et al. 2018MNRAS.477.4711G, Cat. J/MNRAS/477/4711).I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
