Table 1.
INSPIRE DR1 sample.
| ID | RA | Dec | magr | ⟨μe⟩r | 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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