Far-infrared observations of dust in Ly alpha emitters at z=2-6

arXiv:2607.00165 · astro-ph.GA · Submitted 2026-06-30 · Read on arXiv

Rahul Rana, Julie L. Wardlow, Thomas M. Cornish, Pascale H. Desmet, David Sobral, João Calhau

astro-ph.GA

Submitted: 2026-06-30

Journal ref: Mon Not R Astron Soc (2026)

DOI: 10.1093/mnras/stag1396

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• AGN — 113× in this paper · explained in 1 episode
• Dust Attenuation — 10× in this paper · explained in 2 episodes
• alpha — 9× in this paper · explained in 1 episode
• Aperture — 5× in this paper · explained in 1 episode
• Metallicity — 4× in this paper · explained in 3 episodes
• Alignment — 2× in this paper · explained in 1 episode
• Calibration — 2× in this paper · explained in 7 episodes
• Aperture Correction — 1× in this paper · explained in 1 episode
• Aperture Photometry — 1× in this paper · explained in 1 episode
• Robustness — 1× in this paper · explained in 5 episodes
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Dust in the Average Galaxy: Attenuation, Emission, and Opacity from 0<z<7
• The effect of the high-pass filter data reduction technique on the Herschel PACS Photometer PSF and noise

Related papers

• Apparent Stability in Self-Gravitating Turbulence and the Evolution of Molecular Clouds
• Two sets of potential-density basis pairs for the study of radial perturbations in collisionless spherical stellar systems
• Constraining reionization-era Ly alpha escape with JELS-MUSE: a highly complete H alpha-selected sample at z about6.1
• Deriving volume density profiles of filaments from observed surface densities
• Little Red Dots and Supermassive Black Hole Seed Formation in Ultralight Dark Matter Halos
• MEGATRON: how the first stars can create an iron metallicity plateau in the smallest dwarf galaxies