The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z~1

@article{Bouche2021TheME,
  title={The MUSE Extremely Deep Field: Evidence for SFR-induced cores in dark-matter dominated galaxies at z~1},
  author={Nicolas F. Bouch'e and Samuel Bera and Davor Krajnovi{\'c} and Eric Emsellem and Wilfried Mercier and Joop Schaye and Beno{\^i}t {\'E}pinat and Johan Richard and Sebastiaan L. Zoutendijk and Valentina Abril-Melgarejo and Jarle Brinchmann and Roland Bacon and Thierry Contini and Leindert A. Boogaard and Lutz Wisotzki and Michael V. Maseda and Matthias Steinmetz},
  journal={Astronomy \& Astrophysics},
  year={2021}
}
Context. Disc-halo decompositions z = 1−2 star-forming galaxies (SFGs) at z > 1 are often limited to massive galaxies (M? > 1010 M ) and rely on either deep integral field spectroscopy data or stacking analyses. Aims. We present a study of the dark-matter (DM) content of nine z ≈ 1 SFGs selected among the brightest [O ii] emitters in the deepest Multi-Unit Spectrograph Explorer (MUSE) field to date, namely the 140 h MUSE Extremely Deep Field. These SFGs have low stellar masses, ranging from 108… 
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Observational constraints on stellar feedback in dwarf galaxies

Feedback to the interstellar medium (ISM) from ionising radiation, stellar winds and supernovae is central to regulating star formation in galaxies. Due to their low mass ( M ∗ < 10 9 M (cid:12) ),

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