Correction to: Structure and morphology of the MATLAS dwarf galaxies and their central nuclei
Year: 2025
Type: erratum
Abstract: In the published version of this article (2021, MNRAS 506, 5494), an error appears in table 1, where the numerical values of the two surface brightness parameters, |$\mu _{0,g}$| and |$\langle \mu _{e,g} \rangle$|, were reported incorrectly. The corrected version of table 1 is given below. This correction does not affect the scientific conclusions of the paper. Structural and photometric properties of the MATLAS dwarfs. Notes. The full table is available as supplementary material as well as at CDS. Columns meanings: (1) Dwarf ID; (2) Assumed host ETG; (3) Distance; (4) Distance flag: 1 = one single massive Atlas|$^{\rm 3D}$| galaxy in the field with distance; 2 = several massive Atlas3D galaxies in the field all located at roughly the same distance; 3 = several massive Atlas|$^{\rm 3D}$| galaxies in the field with a majority at roughly the same distance, but some discrepant one(s); 4 = several massive Atlas3D galaxies in the field with a range of distances; (5) Distance measurement from |$^{\rm (a)}$| SDSS DR13 database, |$^{\rm (b)}$| Poulain et al., in preparation, |$^{\rm (c)}$| H. B. Ann, M. Seo & D. K. Ha (2015), |$^{\rm (d)}$| I. D. Karachentsev, D. I. Makarov & E. I. Kaisina (2013), |$^{\rm (e)}$| O. Müller et al. (2021); (6) and (7) Right ascension and declination of the dwarf; (8) Apparent magnitude in the g band; (9) |$g-i$| colour corrected for Galactic extinction; (10) g|$-$|r colour corrected for Galactic extinction; (11) Sérsic index (12) Effective radius; (13) Axis-ratio; (14) Position angle; (15) Central surface brightness in the g-band; (16) Average surface brightness within R|$_{\rm e}$| in the g-band; (17) Dwarf morphology. dE* corresponds to the dwarf whose nucleus matches with a star in the Gaia DR2 catalogue. dE** corresponds to the dwarf for which one of the central bright GCs is possibly an NSC (D. A. Forbes et al. 2019). ** corresponds to a Sérsic index derived on a binned image. Structural and photometric properties of the MATLAS dwarfs. Notes. The full table is available as supplementary material as well as at CDS. Columns meanings: (1) Dwarf ID; (2) Assumed host ETG; (3) Distance; (4) Distance flag: 1 = one single massive Atlas|$^{\rm 3D}$| galaxy in the field with distance; 2 = several massive Atlas3D galaxies in the field all located at roughly the same distance; 3 = several massive Atlas|$^{\rm 3D}$| galaxies in the field with a majority at roughly the same distance, but some discrepant one(s); 4 = several massive Atlas3D galaxies in the field with a range of distances; (5) Distance measurement from |$^{\rm (a)}$| SDSS DR13 database, |$^{\rm (b)}$| Poulain et al., in preparation, |$^{\rm (c)}$| H. B. Ann, M. Seo & D. K. Ha (2015), |$^{\rm (d)}$| I. D. Karachentsev, D. I. Makarov & E. I. Kaisina (2013), |$^{\rm (e)}$| O. Müller et al. (2021); (6) and (7) Right ascension and declination of the dwarf; (8) Apparent magnitude in the g band; (9) |$g-i$| colour corrected for Galactic extinction; (10) g|$-$|r colour corrected for Galactic extinction; (11) Sérsic index (12) Effective radius; (13) Axis-ratio; (14) Position angle; (15) Central surface brightness in the g-band; (16) Average surface brightness within R|$_{\rm e}$| in the g-band; (17) Dwarf morphology. dE* corresponds to the dwarf whose nucleus matches with a star in the Gaia DR2 catalogue. dE** corresponds to the dwarf for which one of the central bright GCs is possibly an NSC (D. A. Forbes et al. 2019). ** corresponds to a Sérsic index derived on a binned image. We are grateful to J. Gannon and A. Levitskiy for bringing the error in table 1 to our attention. Table 1. Structural and photometric properties of the MATLAS dwarfs.
Institutions: Universität Innsbruck, Centre National de la Recherche Scientifique, Observatoire astronomique de Strasbourg, Université de Strasbourg, Royal Observatory, UK Astronomy Technology Centre, Youngstown State University, Yonsei University, Leiden University, Leiden Observatory, Universidade do Porto, Institute of Astrophysics and Space Sciences, Centro de Astrofísica da Universidade do Porto, Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, Lyon 1 Université, École Normale Supérieure de Lyon, Centre de Recherche Astrophysique de Lyon
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $3,046
OpenAlex ID: W4415634226