Abstract
We aim to apply a methodology to build a sample of extreme-emission-line galaxies (EELGs) using integral field spectroscopy data. In this work, we followed the spectroscopic criteria corresponding to EELG selection and used the MUSE Hubble Ultra-Deep field survey, which includes the deepest spectroscopic survey ever performed. Objects in the primary (extended) sample were detected requiring a rest-frame equivalent width of EWo geqslant 300 leq EWo leq 300 ) in any of the emission lines of OII OIII or Halpha . A detailed closer inspection of the spectra of the candidates selected has been performed on a one-by-one basis in order to confirm their classification. For this sample, the line fluxes, physical properties, and chemical abundances of the EELGs have been derived, as well as their spatially resolved structure and kinematics. Four (five) of the galaxies in the primary (extended) sample, sim 57$<!PCT!>$ (sim 83$<!PCT!>$), were spatially resolved. Three (none) of them present a clear pattern compatible with rotation. We show how our entire EELG sample shares the same loci defined by high-redshift galaxies (z approx 6-8) for the mass-metallicity relation, illustrating their role as local analogs.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Disclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.