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Table 2.

Observation parameters of the targets presented in this paper for each band.

Target Observing mode (a) PSF (b) (″, kpc) τexp(c) (h)
H K H K
X_N_160_22 AO 0.31, 2.5 0.34, 2.8 3.0 1.0
X_N_81_44 AO 0.27, 2.2 0.24, 2.0 7.0 1.0
X_N_53_3 AO 0.47, 3.8 0.44, 3.6 1.0 1.0
X_N_66_23 AO 0.24, 1.9 0.45, 3.7 1.0 0.7
X_N_35_20 AO 0.27, 2.2 0.26, 2.1 1.0 1.0
X_N_12_26 AO 0.30, 2.4 0.30, 2.4 6.0 2.0
X_N_44_64 ( * ) AO 0.66, 5.4 > 0.20, > 1.6 1.0 1.0
X_N_4_48 ( * ) AO 0.36, 2.9 > 0.20, > 1.6 3.0 1.0
X_N_102_35 noAO 0.92, 7.6 0.85, 7.0 1.0 1.0
X_N_115_23 AO 0.30, 2.4 0.27, 2.2 2.0 2.0
cid_166 AO 0.29, 2.4 0.28, 2.3 3.5 1.5
cid_1605 noAO 0.7, 5.8 0.65, 5.4 2.0 2.0
cid_346 AO 0.30, 2.5 0.30, 2.5 3.7 2.0
cid_1205 AO 0.3, 2.5 0.3, 2.5 1.0 1.0
cid_467 noAO 1.1, 9.0 0.98, 8.0 2.0 2.0
J1333+1649 AO 0.50, 4.2 0.40, 3.3 1.0 1.0
J1441+0454 AO 0.34, 2.8 0.21, 1.8 1.0 1.0
J1549+1245 AO 0.22, 1.8 0.30, 2.4 1.0 1.0
S82X1905 AO 0.34, 2.5 0.35, 2.9 5.0 2.0
S82X1940 AO 0.30, 2.4 0.30, 2.4 4.3 3.0
S82X2058 AO 0.27, 2.2 0.32, 2.6 6.0 2.0

Notes.

(a)

Mode of observation: AO means that H- and K-band observations were taken separately with AO corrections, and noAO means that observations were taken with HK grating under bad weather conditions during the visitor mode runs with no corrections;

(b)

FWHM of the dedicated PSF star before the science observation in arcsec;

(c)

exposure time (hours) in each band.

( * )An accurate estimation of the PSF could not be obtained for X_N_44_64 and X_N_4_48 as the PSF star was at the edge of the SINFONI FoV.

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