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 9 z ≈ 1 SFGs selected among the brightest [O ii] emitters in the deepest Multi-Unit Spectrograph Explorer (MUSE) field to date, namely the 140hr MUSE Extremely Deep Field. These SFGs have low stellar masses, ranging from 108… Expand

References

SHOWING 1-8 OF 8 REFERENCES
In press
29. Cited by Tsuchiya, Kenzaburo: The relation of occupation to cancer, especially cancer of the lung. Cancer, 1965, 18, 136-144. 30. Thiersch, J. B.: Review of certain classes of chemicals whichExpand
Colossus: COsmology, haLO, and large-Scale StrUcture toolS
Galactic dynamics (Princeton
  • NJ: Princeton
  • 2013
2018) used Eq. A.4 with a constant scale height ad an exponentially declining dispersion profile σr(r) ≡ σ0 exp(−r/2rd) and found with Eq
  • 2018
The Theory of Probability (Oxford U
  • J. A. 2018,
  • 2017
Assuming a constant disk thickness hz, i.e. ρ ∝ Σ, and a constant dispersion profile σr, one has v2c = v 2
  • 1996
A&A proofs: manuscript no. mxdf_dark
    Article number