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Table 1.

INSPIRE DR1 sample.

ID RA Dec magr μer OBs Exp. time PA ⟨Seeing UVB⟩ ⟨Seeing VIS⟩
(deg) (deg) (AB) (AB) # (s) (deg) (arcsec) (arcsec)
KiDS J0211–3155 32.8962202 −31.9279437 19.78 18.38 4/4 11 240 289.3 0.88 0.85
KiDS J0224–3143 36.0902655 −31.7244923 19.25 17.98 4/4 11 240 311.9 1.08 1.00
KiDS J0226–3158 36.5109217 −31.9810149 19.25 18.83 3/3 8430 33.4 0.99 0.96
KiDS J0240–3141 40.0080971 −31.6950406 19.05 17.00 2/2 5620 267.7 0.90 0.89
KiDS J0314–3215 48.5942558 −32.2632679 19.57 16.98 3/3 8430 263.4 0.74 0.71
KiDS J0316–2953 49.1896388 −29.8835868 19.66 18.09 3/3 8430 342.1 0.98 0.99
KiDS J0317–2957 49.4141028 −29.9561748 19.1 18.02 2/2 5620 339.9 0.86 0.87
KiDS J0321–3213 50.2954390 −32.2221290 19.23 18.28 4/4 11 240 311.5 0.80 0.80
KiDS J0326–3303 51.5140585 −33.0540443 19.48 18.89 4/4 11 240 354.4 0.90 0.90
KiDS J0838+0052 129.530452 0.88238415 19.29 19.03 3/3 8430 334.7 0.85 0.85
KiDS J0842+0059 130.666536 0.98993690 19.6 18.36 3/3 8430 346.8 0.86 0.85
KiDS J0847+0112 131.911239 1.20571289 18.41 18.69 2/2 5620 314.4 0.94 0.96
KiDS J0857–0108 134.251219 −1.14570771 19.21 19.02 2/2 2810 356.2 0.88 0.83
KiDS J0918+0122 139.644643 1.37947803 19.13 18.47 3/3 8430 301.0 0.89 0.89
KiDS J0920+0212 140.232084 2.21268315 18.87 18.54 2/2 5620 270.5 0.94 0.96
KiDS J2305–3436 346.335663 −34.6030907 19.69 18.93 4/4 11 240 316.4 0.92 0.93
KiDS J2312–3438 348.238904 −34.6485914 19.32 18.34 9/9 (*) 25 290 275.4 1.40 1.33
KiDS J2327–3312 351.991016 −33.2007599 19.35 18.28 4/4 11 240 315.6 0.92 0.92
KiDS J2359–3320 359.985168 −33.3335828 19.59 18.07 4/4 2810 265.1 0.90 0.87

Notes. Together with ID and coordinates, we give, for each relic candidate, the aperture magnitudes (MAG_AUTO from the KiDS DR3 catalogue) and the surface brightness luminosities averaged within the effective radius (⟨μe⟩), both in r-band, that have been used to decide the number of OBs scheduled for each system, which is also listed in the table. (*)For J2312−3438 a total of four OBs were requested, however five OBs were repeated because they were classified as grade C for violating the seeing constraints. This means that for this particular system we received more data than originally expected but of lower quality. Furthermore, the total exposure time on target, the PA to which the slit was oriented (on the major axis of the galaxies), and the median seeing during observations both in UVB and VIS arm are also given. These values are the median of the headers keyword HIERARCH ESO TEL IA FWHM of each OB, representing the delivered seeing corrected per airmass.

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