ESO 435-02/ESO 435-016 ATCA HI images (Kim+, 2017)

The HI observations were conducted on March 27 and 28 2002 with the ATCA in EW367 array configuration (project ID of C1024). The ATCA primary beam is 33.1-arcmin at 1416MHz, which is comparable to the angular distance between the pair of galaxies of ~30.3-arcmin. With a single pointing, the sensitivity at the locations of the galaxies hence drops by a factor of ~1.8, and therefore we had two extra pointings centered on each galaxy in order to keep the desired sensitivity toward the pair. The observing frequency was centered on 1416MHz with a total bandwidth of 8MHz, which is configured into 512 channels, yielding a channel width of 3.3km/s.

Identifier
Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/605/A54
Related Identifier https://ui.adsabs.harvard.edu/abs/2017A&A...605A..54K
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/A+A/605/A54
Provenance
Creator Kim J., Chung A., Wong O.I., Lee B., Sung E.-C., Staveley-Smith L.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2017
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Format text/xml+votable
Version 14-Sep-2017
Discipline Astrophysics and Astronomy