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Table 1.

Summary of targets and VLT/MUSE observations.

Field name RA Dec zem Total Exp. Instrument Effective Program ID Lens
[h:m:s] [°: $ \prime $:″] time [s] Mode PSF (a) [″] Ref. (b)
SGAS J0033+0242 00:33:41.52 +02:42:27.0 2.39 11 × 700 WFM-NOAO-N 0.84 098.A-0459(A) (1)
SGAS J1527+0652 15:27:44.74 +06:52:19.4 2.76 25 × 600 WFM-AO-E 0.78 0103.A-0485(B) (2)
PSZ1 G311.65–18.48 15:50:07.46 −78:11:23.2 2.37 2 × 1483 WFM-NOAO-N 0.82 297.A-5012(A) (3)
SGAS J2111–0114 21:11:19.01 −01:14:30.4 2.86 15 × 606 WFM-AO-E 0.74 0103.A-0485(B) (4)

Notes.

(a)

Point spread function at ≈5000 Å measured from fitting 2D Gaussian profiles to stars in the final combined MUSE cubes.

(b)

Lens model references: (1) Fischer et al. (2019), (2) Sharon et al. (2020), (3) Lopez et al. (2020), and (4) Sharon et al. (2020).

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