Characterizing the contribution of dust-obscured star formation at $z \gtrsim$ 5 using 18 serendipitously identified [CII] emitters

Documenti analoghi

• The ALMA REBELS survey: [OIII]$_{88μ\text{m}}$ line scans of UV-bright $z \gtrsim 7.6$ galaxies
  di: van Leeuwen, I. F., et al.
  Pubblicazione: (2025)
• REBELS-IFU: Steeply rising star formation histories and the importance of dust obscuration in massive $z \simeq7$ galaxies revealed by multi-wavelength observations
  di: Fisher, R., et al.
  Pubblicazione: (2025)
• NOEMA reveals the true nature of luminous red JWST z>10 galaxy candidates
  di: Meyer, R. A., et al.
  Pubblicazione: (2023)
• Beneath the Surface: >85% of z>5.9 QSOs in Massive Host Galaxies are UV-Faint
  di: Bouwens, R. J., et al.
  Pubblicazione: (2025)
• Deep Constraints on [CII]158$μ$m in JADES-GS-z14-0: Further Evidence for a Galaxy with Low Gas Content at z=14.2
  di: Schouws, Sander, et al.
  Pubblicazione: (2025)