Key specifications

HARMONI is the first light visible and near-IR integral field spectrograph for the ELT. It covers a large spectral range from 0.46µm to 2.46µm with resolving powers from R (≡λ/Δλ) 3,300 to 17,300 and spatial sampling from 60mas to 4mas. It can operate in two Adaptive Optics modes - LTAO and SCAO - or with no AO.

Field of view and spatial resolution

HARMONI has a field of view of 152×214 spatial pixels (spaxels) and ~4000 spectral channels per spaxel. There are 4 spaxel scales available (from 4mas × 4mas to 60mas × 30mas), which permit the user to optimally configure the instrument for a wide range of science programs. From ultra-sensitive to diffraction limited. The coarsest scale (30mas × 60mas spaxels) provides a 9.1″ × 6.2″ FoV, well suited to seeing limited observations, and the finest scale, a factor of 15 finer (4mas × 4mas), Nyquist sampling the diffraction limit of the ELT at near-infrared wavelengths. With its large range of spaxel scales, HARMONI can easily adapt to any flavour of adaptive optics - LTAO and SCAO -, or even with no AO at all.

Scale (mas) FoV Comments
60×30 9.1"×6.2" For non-AO & visible observations
20×20 3.0"×4.1" For optimal sensitivity (faint targets)
10×10 1.5"×2.1" Best combination of sensitivity and spatial resolution
4×4 0.6"×0.8" Highest spatial resolution (diffraction limited)

Spectral configurations

HARMONI has 11 spectral configurations covering the visible and near-IR spectral range from 0.46µm to 2.46µm with three spectral resolutions: ~3,300 (low-R), ~7,100 (mid-R) and ~17,300 (high-R).

Spectral configurations
Band R λmin(µm) λmax(µm)
V+R 3300 0.458 0.820
I+z+J 3355 0.811 1.369
H+K 3355 1.450 2.450
I+z 7104 0.830 1.050
J 7104 1.046 1.324
H 7104 1.435 1.815
K 7104 1.951 2.469
z-high 17385 0.828 0.902
H-high 17385 1.538 1.678
K-short 17385 2.017 2.201
K-long 17385 2.199 2.400

Adaptive Optics modes

HARMONI operates in 2 AO modes or with no AO:
  • Single conjugate AO (SCAO). Natural guide star. Diffraction limited (10mas) 1% sky coverage. Suited for Galatic center or densly populated fields.
  • Laser tomography AO (LTAO). Laser guide stars. Lower performance than SCAO but a higher sky coverage (50-90%)
  • No AO (noAO)