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Table 2

32 observations analyzed in this work.

Field name Obs ID RA (deg) Dec (deg) Time (ks) Date TM ∆RA (arcsec) ∆DEC (arcsec) ∆Θ (arcsec)
A3391 300014 96.6568 −54.0524 8.3 2019-10-07 5,6,7

A3391 300005s 96.6989 −53.8210 1.0 2019-10-08 5,6,7

A3391 300006s 96.7149 −53.8080 1.0 2019-10-09 5,6,7

A3391 300016s 97.1387 −54.3858 2.2 2019-10-17 1–7 reference

1H0707 300003 107.3127 −19.3800 11.9 2019-10-11 5,6,7

A3266 700154 67.8202 −61.4269 31.6 2019-11-11 1–7

A3158 700177 55.7146 −53.6270 34.8 2019-11-21 1–7 i

N7793 300011 359.4624 −32.6090 27.4 2019-11-18 1–6

J1856 700008 284.1596 −37.9058 38.6 2019-10-24 1–7
J1856 710001 284.1332 −37.9139 16.2 2020-04-01 1–7
J1856 720002 284.1600 −37.9047 30.1 2020-10-07 1–7 reference

3C390 900060 280.5922 79.7712 1.6 2019-09-24 6
3C390 900068 280.5920 79.7719 1.5 2019-09-28 6
3C390 900069 280.5920 79.7721 1.7 2019-09-29 6
3C390 900070 280.5912 79.7724 1.7 2019-09-30 6 reference

H2213 300017 285.6054 −37.1228 25.5 2019-10-26 1–7

J2334 700180 353.5144 −47.2260 18.9 2019-11-19 1–7
J2334 700181 353.7685 −47.5110 18.5 2019-11-20 1–7 reference

47Tuc 700012 6.5318 −72.1758 1.5 2019-09-28 6
47Tuc 700163 6.5264 −72.1604 11.1 2019-11-01 1,2,4–7 reference
47Tuc 700011 5.5181 −71.9681 11.3 2019-11-01 1,2,4–7
47Tuc 700013 6.3215 −71.9086 10.9 2019-11-02 1,2,4–7
47Tuc 700014 5.7088 −72.2212 11.9 2019-11-02 1–7
47Tuc 700173 5.5198 −71.9692 3.0 2019-11-19 1–7
47Tuc 700174 6.5349 −72.1609 3.8 2019-11-19 1–7
47Tuc 700175 6.3350 −71.9095 3.8 2019-11-19 1–7

ES0102 700001 16.0279 −72.0127 27.6 2019-11-07 1–7 reference
ES0102 700002 15.0568 −71.8692 29.6 2019-11-08 1–7
ES0102 700003 17.0144 −72.1514 30.2 2019-11-09 1–7
ES0102 700004 16.3022 −71.8317 27.6 2019-11-09 1–7
ES0102 700005 16.4384 −71.7413 28.0 2019-11-10 1–7
ES0102 710000 16.2691 −72.0570 16.0 2020-06-18 1–4,6,7

Notes. The columns are: (1) field name; (2) observation ID; (3-4) pointing coordinates (J2000); (5) 0.2-2.3 keV vignetted exposure time, averaged in the field and among the 7 TMs; (6) date of the observation starting time; (7) active telescope modules; (8-10) relative astrometric correction on the pointing RA, Dec and the roll angle Θ with 1-σ uncertainties. The mark “s on the observation ID indicates scanning mode. The ∆RA is already multiplied by cos(Dec), where Dec is the Declination of the field center (Table 1). The ∆RA, ∆Dec in bold font and with a suffix | mark are absolute corrections of each field with respect to WISE counterparts (Sect. 4.3); and the others are relative corrections of each observation (Sect. 2) with respect to the reference observation (flagged as “reference” in the ∆Θ column).

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