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Table B.2.

Physical properties of the sources.

RA (a) Dec. (b) Redshift (c) Magnification (d) Star Formation Rate (e)
(deg) (deg) (M yr−1)
Abell_2744
3.5938 −30.4154 6.588
3.5801 −30.4079 6.556 2.70 R
3.5831 −30.4119 6.519 3.00 R
3.5769 −30.3863 6.457
3.5983 −30.4178 6.4
3.5728 −30.4145 6.477

MACS_J0416.1−2403
64.0508 −24.0664 6.148 0.4 R
64.0482 −24.0624 6.147
64.0429 −24.0572 6.145
64.0435 −24.0590 6.147 4.81 R 0.6 R
64.0478 −24.0621 6.147
64.0260 −24.0891 6.15 9.63 R
64.0318 −24.0889 6.405
64.0325 −24.0557 5.996
64.0459 −24.0742 6.457
64.0537 −24.0711 6.385 1.81 AD 0.7 AD
64.0330 −24.0662 6.455
64.0439 −24.0563 6.161
64.0493 −24.0710 6.147 2.23 R
64.0398 −24.0669 5.998 2.21 R
64.0364 −24.0622 6.066 3.37 R
64.0484 −24.0736 6.066 2.08 R
64.0458 −24.0741 5.998 3.20 R
64.0517 −24.0695 6.561 2.01 R
64.0556 −24.0638 6.074 2.12 R
64.0520 −24.0705 6.067 1.85 R
64.0460 −24.0582 6.498 8.34 R
64.0410 −24.0641 6.066 2.82 R
64.0433 −24.0629 6.147 3.69 R 1.3 R
64.0389 −24.0606 6.147 4.05 R

Abell_S1063
342.1841 −44.5353 6.107 16.73
342.1924 −44.5157 6.5
342.1909 −44.5375 6.107
342.1811 −44.5346 6.107
342.1841 −44.5317 6.107 1.77 HFFDS 125.9 HFFDS
342.1890 −44.5300 6.107 5.35 HFFDS 23.4 HFFDS

MACS_J1149.5+2223
177.3793 22.4033 6.478

MACS1206.2−0847
181.5511 −8.8037 6.014 72.90 R
181.5533 −8.7988 6.063
181.5517 −8.7992 6.06 6.88 R

RXJ_1347−1145
206.8921 −11.7483 5.98
206.8762 −11.7386 6.457
206.8832 −11.7563 6.566 12.29 R

MACS0329.7−0211
52.4258 −2.1898 6.011 11.52 R
52.4312 −2.1914 6.026 3.51 R
52.4202 −2.1945 6.026 4.93 R
52.4169 −2.1977 6.1
52.4281 −2.1964 6.011 10.71 R
52.4310 −2.2044 6.075 3.72 R

MACS1115.9+0129
168.9553 1.4993 6.057

Abell 383
42.0136 −3.5263 6.027
42.0192 −3.5329 6.027

Notes. IDs are placed next to values when they are extracted from the literature, R stands for Richard et al. (2021), AD for ASTRODEEP and HFFDS for Huble Frontier Field DeepSpace. Values with no mention have been computed through our own analysis presented in Sect. 2.2.2.

(a)

Right Ascension coordinate of the source (degrees);

(b)

Declination coordinate of the source (degrees);

(c)

Redshift of the source;

(d)

Source lensing magnification;

(e)

Source SFR. When not derived from the literature, SFR were derived using the UV luminosity and corrected for dust attenuation (see Sect. 2.2.2).

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