Emission-line sources MUSE spectral catalogue (Goettgens+, 2019)

The spectra were extracted from datacubes taken with MUSE at the VLT. We used matched filtering to search for emission-line objects (ELOs) in globular clusters. The tables contain the properties of the detected ELOs, including references to the literature. Please see the paper for details about which filter was used for the reported V magnitude, and which conventions are used for the cluster membership indicator and the indicator for radial velocity variations.

Identifier
Source http://cdsarc.u-strasbg.fr/cgi-bin/Cat?J/A+A/631/A118
Related Identifier https://ui.adsabs.harvard.edu/abs/2019A&A...631A.118G
Metadata Access http://dc.g-vo.org/rr/q/pmh/pubreg.xml?verb=GetRecord&metadataPrefix=oai_datacite&identifier=ivo://CDS.VizieR/J/A+A/631/A118
Provenance
Creator Goettgens F., Husser T.-O., Kamann S., Dreizler S., Giesers B., Kollatschny W., Weilbacher P.M., Roth M.M., Wendt M.
Publisher CDS
Contributor International Virtual Observatory Alliance (IVOA)
Publication Year 2019
Rights public
OpenAccess true
Contact CDS support team <cds-question(at)unistra.fr>
Representation
Format text/xml+votable
Version 25-Sep-2019
Discipline Astrophysics and Astronomy