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Table 1

Sample of the galaxy clusters analysed in this work.

Cluster z Detector Exposure [ks] RA [J2000] Dec [J2000] tot cts [kpc] n bin S b [kpc] n bin T

MACS J0159.8-0849 0.405 ACIS-I 29.1 01 59 49.50 −08 49 59.3 20 250 1130 56 786 13
MACS J2228.5+2037 0.412 ACIS-I 16.5 22 28 32.41 + 20 37 30.5 9234 1511 27 680 5
MS1621.5+2640 0.426 ACIS-I 27.5 16 23 35.40 + 26 34 11.2 9277 1109 20 856 5
MACS J1206.2-0848 0.440 ACIS-I 21.1 12 06 12.38 −08 48 07.4 10 559 1131 29 516 5
MACS J2243.3-0935 0.447 ACIS-I 18.5 22 43 21.57 −09 35 42.4 9432 1305 31 537 5
MACS J0329.7-0211 0.450 ACIS-I 28.4 03 29 41.40 −02 11 44.4 12 870 950 34 660 8
RXJ 1347.5-1145 0.451 ACIS-I 29.2 13 47 30.87 −11 45 09.9 29 013 1266 66 829 10
V1701+6414 0.453 ACIS-I 31.1 17 01 23.41 + 64 14 11.5 9841 892 15 633 6
MACS J1621.6+3810 0.465 ACIS-I 29.9 16 21 24.69 + 38 10 08.6 11 048 794 22 471 6
CL0522-3624 0.472 ACIS-I 26.4 05 22 15.29 −36 25 02.7 6871 587 16 440 3
MACS J1311.0-0310 0.494 ACIS-I 44.5 13 11 01.87 −03 10 39.8 11 297 634 25 381 6
MACS J2214.9-1400 0.503 ACIS-I 15.4 22 14 57.48 −14 00 09.6 7837 1318 19 872 5
MACS J0911.2+1746 0.505 ACIS-I 23.0 09 11 10.61 + 17 46 30.9 4220 1283 16 904 8
MACS J0257.1-2326 0.505 ACIS-I 17.0 02 57 09.13 −23 26 04.3 3832 1389 17 478 8
V1525+0958 0.516 ACIS-I 28.2 15 24 40.04 + 09 57 48.9 3613 575 8 435 4
MS0015.9+1609 0.541 ACIS-I 31.0 00 18 33.36 + 16 26 12.6 9652 1375 41 913 9
CL0848.6+4453 0.543 ACIS-I 125.2 08 48 47.73 + 44 56 13.9 13 613 300 5 282 3
MACS J1423.8+2404 0.543 ACIS-S 105.4 14 23 47.90 + 24 04 42.2 35 182 899 33 603 10
MACS J1149.5+2223 0.544 ACIS-I 51.4 11 49 35.52 + 22 23 52.7 23 253 1470 26 875 8
MACS J0717.5+3745 0.546 ACIS-I 74.6 07 17 31.22 + 37 45 22.6 34 326 1389 62 1090 21
CL1117+1744 0.548 ACIS-I 37.5 11 17 29.89 + 17 44 52.1 7098 520 8 500 3
MS0451.6-0305 0.550 ACIS-S 37.0 04 54 11.04 −03 00 57.8 18 100 955 33 486 6
MS2053.7-0449 0.583 ACIS-I 35.0 20 56 21.12 −04 37 48.4 5428 463 11 293 3
MACS J2129.4-0741 0.589 ACIS-I 18.0 21 29 25.64 −07 41 32.0 6226 1055 13 611 5
MACS J0647.7+7014 0.591 ACIS-I 17.9 06 47 49.95 + 70 14 56.2 5362 1028 20 274 4
CL1120+4318 0.600 ACIS-I 18.6 11 20 07.23 + 43 18 03.6 3452 722 13 599 4
CLJ0542.8-4100 0.640 ACIS-I 49.9 05 42 49.63 −40 59 56.3 5026 744 12 771 4
LCDCS954 0.670 ACIS-S 26.9 14 20 29.25 −11 34 19.4 1005 586 8 384 3
MACS J0744.9+3927 0.698 ACIS-I 48.7 07 44 52.82 + 39 27 26.1 9257 1106 23 508 5
V1221+4918 0.700 ACIS-I 74.3 12 21 25.71 + 49 18 30.4 2411 592 14 595 5
SPT-CL0001-5748 0.700 ACIS-I 29.4 00 00 59.91 −57 48 34.7 7544 525 14 244 3
RCS2327.4-0204 0.704 ACIS-I 73.4 23 27 27.68 −02 04 38.5 13 778 944 28 705 8
SPT-CLJ2043-5035 0.720 ACIS-I 76.6 20 43 17.48 −50 35 32.0 5006 594 11 380 3
ClJ1113.1-2615 0.730 ACIS-I 92.5 11 13 05.42 −26 15 39.2 660 330 10 288 3
CLJ2302.8+0844 0.734 ACIS-I 100.6 23 02 48.05 + 08 43 49.3 3649 627 10 350 3
SPT-CL2337-5942 0.775 ACIS-I 19.7 23 37 24.65 −59 42 22.7 2013 557 10 254 3
RCS2318+0034 0.780 ACIS-I 112.5 23 18 30.88 + 00 34 01.6 22 445 446 13 380 4
MS1137.5+6625 0.782 ACIS-I 101.3 11 40 22.53 + 66 08 14.3 3454 440 14 402 7
RXJ 1350.0+6007 0.810 ACIS-I 55.2 13 50 48.18 + 60 07 13.4 4564 698 8 450 3
RXJ 1716.9+6708 0.813 ACIS-I 50.7 17 16 48.94 + 67 08 25.2 1180 418 9 481 3
EMSS1054.5-0321 0.831 ACIS-S 63.5 10 57 00.07 −03 37 33.1 3872 566 11 574 5
CLJ1226.9+3332 0.888 ACIS-I 29.9 12 26 58.07 + 33 32 46.0 3450 779 15 277 4
XMMUJ1230+1339 0.975 ACIS-S 38.4 12 30 17.06 + 13 39 08.5 6538 344 9 287 4
J1415.1+3612 1.030 ACIS-S 97.5 14 15 11.01 + 36 12 04.1 8727 419 20 260 4
SPT-CL0547-5345 1.067 ACIS-I 28.0 05 46 37.25 −53 45 30.6 3492 657 8 597 3
SPT-CLJ2106-5844 1.132 ACIS-I 47.1 21 06 03.38 −58 44 29.6 7552 680 11 432 3
RDCS1252-2927 1.235 ACIS-I 148.7 12 52 54.58 −29 27 16.9 13 103 378 7 286 3

Notes. Columns from left to right list the target name, adopted redshift, detector used in the observation, net exposure time (in kilo-seconds) after all cleaning processes, position of the adopted X-ray centre in equatorial J2000 coordinates, and number of counts measured for each target in the [0.72] keV band, up to the radial limit . The last four columns list the upper limit of the radial range investigated in the spatial analysis () and in the spectral analysis () with the number of bins with which we can sample the surface brightness and temperature profiles (the temperature bins are obtained by integrating the spectra between 0.6 and 7 keV).

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