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5 papers

astro-ph.IM2026

HARMONI@ELT: instrument design, performance, and science capabilities

B. Neichel, J. Dunlop, S. Chittick +17

The paper describes the design, performance expectations, and scientific capabilities of HARMONI, the near‑infrared integral field spectrograph being built for the Extremely Large…

astro-ph.IM2026

HARMONI at ELT: line spread functions in a diffraction limited spectrometer

Stephen P. Todd, Éamonn J. Harvey, Anna MacIver +8

HARMONI is the first light, adaptive optics assisted, near-IR integral field spectrograph for the ELT. It covers a spectral range from 800~nm to 2450~nm with resolving powers from…

astro-ph.GA2026

Multi-resolution kinematic modelling of nearby galaxies: a demonstration using MHONGOOSE observations

B. R. Makinson, K. A. Oman, A. M. Swinbank

We present a novel method of combining kinematic models obtained at multiple spatial resolution levels in a self-consistent manner. The MHONGOOSE survey has mapped atomic hydrogen…

astro-ph.GA2025

ALMA Deep Field in SSA22: Reconstructed [CII] Luminosity Function at z = 6

Natsuki H. Hayatsu, Rob J. Ivison, Paola Andreani +19

The ADF22 line survey reported detections of two high- line-emitting source candidates above 6-, both of which were shown to be spurious after follow-up observations. We inv…

astro-ph.CO2025

High-definition imaging of a filamentary connection between a close quasar pair at z=3

Davide Tornotti, Michele Fumagalli, Matteo Fossati +16

Filaments connecting halos are a long-standing prediction of cold dark matter theories. We present a detection of the cosmic web emission connecting two quasar-host galaxies at red…