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Table 1.

Comparison of instrument specifications with performance routinely observed on sky.

Parameter Specification On-sky experience Reference or comment
[Goal]
Driving specifications and goals

NIR contrast on bright targets
DBI contrast at 0.5″ for H <  8 13.25 [15.75] Typical Δmag = 13.5 Fig. 21
Best Δmag = 15.0 Vigan et al. (2015)
IFS contrast at 0.5″ for J <  8 15.00 [20.00] Typical Δmag15 Fig. 21, Appendix C
Best Δmag = 16.5 Sect. 7.3; Vigan et al. (2015)
IFS spectral information 0.95–1.35 μm Ok e.g., Zurlo et al. (2016),
or 0.95–1.65 μm Samland et al. (2017), …

VIS polarimetric contrast
Contrast at 1″ in 4 h on I = 2.5 17 at 0.2″ Sect. 6.3.7; Hunziker et al. (in prep.)
> 20 at 1″

NIR survey capability on large samples
IRDIS+IFS simultaneity Required Used routinely
AO ultimate performance Up to R = 9 Ok Fig. 7
AO robust operations Up to R = 12 Overdone: R = 14 Fig. 7
Throughput > 15% > 20% Fig. 5
Elevation 5°–60° Ok

Additional observation capabilities without impact on driving specifications

Near-infrared
Imaging in various filters Y to K, BB, NB Ok
Dual-polarimetry imaging contrast 9.25 [11.3] at 0.1″ 13.0 at 0.2″ van Holstein et al. (2017), high-efficiency
11.75 [14.25] at 0.5″ 15.0 at 0.5″ in J-band, but strong dependency on
derotator orientation
Long-slit spectroscopy LRS (R ∼ 50Y − Ks) Ok Fig. 23
MRS (R ∼ 350Y − Ks) Ok Fig. 24; Hinkley et al. (2015)

Visible
High-angular resolution imaging NB to very BB Ok Sect. 6.3.2; Schmid et al. (2018)
High-contrast imaging Best effort > 6.5 at 0.1″ Sect. 6.3.5
(non-polarimetric)

Notes. All contrast values are specified in magnitudes and at 5σ.

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