The effect of cosmic web filaments on galaxy properties in the RESOLVE and ECO surveys

Documenti analoghi

• The RESOLVE and ECO G3 Initiative: Drivers of HI Content and X-ray Emission in Galaxy Groups
  di: Hutchens, Zackary L., et al.
  Pubblicazione: (2025)
• Identification and Quenching of Nugget Galaxies in the RESOLVE Survey at z = 0
  di: Carr, Derrick S., et al.
  Pubblicazione: (2024)
• Using Machine Learning to Estimate Near-ultraviolet Magnitudes and Probe Quenching Mechanisms of $z$=0 Nuggets in the RESOLVE and ECO Surveys
  di: Carr, D. S., et al.
  Pubblicazione: (2025)
• How galaxy properties vary with filament proximity in the SIMBA simulations
  di: Bulichi, Teodora-Elena, et al.
  Pubblicazione: (2023)
• Recovering the properties of the interstellar medium through integrated spectroscopy: application to the z~0 ECO volume-limited star-forming galaxy sample
  di: Lebouteiller, V., et al.
  Pubblicazione: (2024)