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Title: | VizieR Online Data Catalog: Radio haloes in nearby galaxies (Heesen+, 2018) | Authors: | Heesen, V. Krause, M. Beck, R. Adebahr, B. Bomans, D. J. CARRETTI, ETTORE Dumke, M. Heald, G. Irwin, J. Koribalski, B. S. Mulcahy, D. D. Westmeier, T. Dettmar, R. -J. |
Issue Date: | 2018 | Journal: | VizieR Online Data Catalog | First Page: | J/MNRAS/476/158 | Abstract: | We present radio continuum observations of 12 nearby (D=2-27Mpc) edge-on galaxies at two different frequencies, namely at 1.4 and 5GHz (one galaxy at 8.5GHz instead of 5GHz). Our sample includes 11 late-type spiral (Sb or Sc) galaxies and one Magellanic-type barred galaxy (SBm), which are all highly inclined (i>=76°). <P />As part of our study we have obtained several additional radio continuum maps. We make these maps publicly available (as well as all the other radio continuum maps in the paper). <P />For 4 galaxies (NGC 55, 253, 891 and 4631) we have used single-dish maps, to correct for the missing zero-spacing flux where necessary. The Effelsberg maps of NGC 253 and 4631 were already presented in Heesen et al. (2009A&A...494..563H) and Mora & Krause (2013A&A...560A..42M), respectively, and the Effelsberg map of NGC 891 was already presented in Dumke (1997, PhD thesis, University of Bonn). We present these maps for completeness. <P />The 4.80-GHz map of NGC 55 obtained with the 64-m Parkes telescope is so far unpublished. Furthermore, we show two maps of NGC 4631 at 1.35 and 1.65GHz observed with the VLA in D- configuration (R. Beck 2016, priv. comm.). The data were observed in August 1996, with 12 h on-source (ID: AG486) and reduced in standard fashion with AIPS. The maps have an angular resolution of 52 arcsec, so that we did not use them in the analysis, but they also show the halo of this galaxy very well. Lastly, we obtained maps of three further edge-on galaxies observed with the VLA (NGC 4157, 4217 and 4634). We reduced the data as described in Section 2, but since we had only one frequency available and no spectral index map, we did not use them in the analysis. The maps of NGC 4157 and 4217 were created by re-reducing archive data (IDs AI23, AF85, AH457 and AS392 for NGC 4157 and ID AM573 for NGC 4217). The map of NGC 4634 was created by using so far unpublished data from the VLA (ID: AD538). <P />(3 data files). | URI: | http://hdl.handle.net/20.500.12386/32506 | URL: | https://cdsarc.unistra.fr/viz-bin/cat/J/MNRAS/476/158 | Bibcode ADS: | 2018yCat..74760158H | Fulltext: | open |
Appears in Collections: | 4.06 Banche Dati |
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