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Table 1

Cluster samples in the XMM-Newton archival data.

Cluster z    ⟨ T ⟩a NHb Typec Obsid (exposures of PN, MOS1 and MOS2)d
(keV) (1020   cm-2) (ks, ks, ks)

A262 0.016 2.5 5.4 cD 0109980101 (19.0 23.6 23.9) 0504780201 (24.9 31.6 33.1)
Virgo 0.004 2.8 2.6 cD 0114120101 (30.0 37.7 38.5) 0200920101 (69.6 76.9 78.5)
0106060101 (5.0 9.2 9.2) 0106060201 (1.6 5.5 5.0) 0106060301 (5.4 7.1 7.9)
0141570101 (17.4 23.2 24.7) 0112550701 (1.0 0.2) 0112552101 (7.6 13.4 13.5)
0106060401 (7.3 10.7 11.1) 0145800101 (5.9 37.8 0.2 0.2) 0106060501 (10.9 15.3 15.4)
0200650101 (42.7 53.2 53.5) 0112840101 (14.6 18.1 17.6) 0106060601 (8.6 10.5 10.7)
0112550801 (2.9 13.2 12.1) 0106060701 (1.2 12.4 5.9) 0108860101 (16.7 20.6 19.2)
0106061401 (4.9 8.0 8.3)
A4038 0.029 3.0 1.5 cD 0204460101 (27.8 29.3 28.9)
A1060 0.012 3.0 4.9 non-cD 0206230101 (28.5 37.9 38.9)
A2052 0.035 3.1 3.0 cD 0109920101 (26.4 28.9 29.0)
A1367 0.021 3.3 2.4 non-cD 0061740101 (23.7 31.8 31.4) 0005210101 (20.8 27.8 28.8)
A780 0.057 3.5 4.7 cD 0109980301 (14.0 19.1 22.2)
A2589 0.042 3.6 3.9 cD 0204180101 (21.8 26.3 27.5)
AWM7 0.017 3.6 9.8 cD 0135950301 (27.5 30.7 30.9)
MKW3s 0.045 3.7 3.0 cD 0109930101 (0.0 37.7 38.0)
A2063 0.036 3.9 3.0 cD 0200120401 (5.0 8.2 5.0)
A3526 0.010 4.0 8.2 cD 0046340101 (35.2 44.9 43.5) 0406200101 (90.5 111.7 111.7) 0504360101 (26.4 28.2 30.9)
0504360201 (32.9 34.0 34.6)
A2199 0.030 4.2 0.9 cD 0008030601 (0.5 6.9 4.7) 0008030301 (2.9 4.7 4.7) 0008030201 (13.3 14.5 14.6)
A496 0.033 4.4 4.6 cD 0135120201 (11.8 16.2 15.9) 0506260301 (44.5 57.0 59.5) 0506260401 (44.8 55.8 58.6)
A1644 0.048 4.6 4.8 non-cD 0010420201 (12.7 14.1 14.1)
A3562 0.050 4.8 4.0 non-cD 0105261301 (37.7 39.0 39.5) 0105261501 (4.8 22.4 22.4) 0105261801 (4.7 10.9 10.4)
0105261701 (0.0 20.6 20.4) 0105261601 (16.3 18.3 19.5) 0105261401 (9.0 12.8 12.4)
A3558 0.048 5.4 4.2 non-cD 0107260101 (38.2 43.1 42.5)
A3627 0.016 5.5 20.8 non-cD 0204250101 (2.4 6.2 5.8) 0208010101 (9.1 12.6 13.0) 0208010201 (10.9 13.6 14.3)
A1795 0.062 5.8 1.2 cD 0097820101 (25.1 38.3 37.9) 0109070201 (53.0 54.5 54.6) 0205190101 (26.9 29.5 28.8)
0205190201 (20.8 22.6 23.2)
A85 0.052 5.8 3.1 cD 0065140101 (9.8 12.4 12.2) 0065140201 (9.2 12.1 12.4)
A3667 0.053 6.0 4.6 non-cD 0105260101 (0.8 7.3 6.8) 0206850101 (52.3 59.2 60.0) 0105260601 (17.7 23.1 23.3)
0105260301 (12.8 17.0 16.2) 0105260401 (11.5 16.3 16.5) 0105260501 (11.2 12.6 12.6)
0105260201 (15.1 19.0 18.4)
A426 0.018 6.1 14.6 cD 0085110101 (47.5 48.8 50.7) 0204720101 (11.9 15.1 15.2) 0085590201 (38.4 41.7 40.0)
(Perseus) 0305720101 (10.0 13.0 12.6) 0305720301 (15.9 19.9 21.2) 0151560101 (18.0 24.9 25.1)
0204720201 (20.7 24.5 24.5) 0405410201 (9.4 17.3 25.5) 0405410101 (12.2 18.2 16.1)
A2256 0.058 6.3 4.1 non-cD 0141380101 (6.4 9.2 8.7) 0141380201 (10.6 13.2 12.4 )
0112951501 (5.9 10.6 10.9) 0112951601 (7.2 12.7 12.7) 0112950601 (8.4 12.3 11.8)
0112500101 (21.8 25.0 25.2)
A3571 0.040 6.5 4.4 cD 0086950201 (14.3 25.4 25.2)
A2029 0.077 7.4 3.2 cD 0111270201 (9.3 12.1 12.4)
A1656 0.023 7.8 0.9 non-cD 0300530201 (0.4 3.6 3.4 ) 0153750101 (19.2 21.3 21.8) 0124711401 (14.7 17.4 16.5)
(Coma) 0300530101 (18.6 20.9 21.0) 0300530301 (26.5 30.5 30.2) 0300530701 (16.4 24.4 24.6)
0300530401 (13.3 18.8 19.6) 0300530601 (16.7 22.6 22.1) 0300530501 (19.2 24.7 24.6)
0124710901 (16.7 21.6 22.1) 0124712001 (9.2 15.4 14.6) 0124710501 (10.7 24.4 24.8)
0124710601 (4.7 9.5 9.0) 0204040101 (69.7 73.0 74.0) 0204040301 (43.7 52.9 53.2)
0204040201 (54.8 61.8 64.8) 0124710801 (18.4 24.5 24.5) 0124710401 (8.2 5.9 5.6)
0124712501 (23.8 27.7 27.7) 0124712401 (11.0 17.4 18.1) 0124711101 (13.2 19.3 21.1)
0124712201 (18.2 26.7 26.2) 0124712101 (20.3 26.0 26.1) 0124710301 (10.6 13.4 14.0)
0124710101 (23.7 30.6 30.8)
A3266 0.055 8.4 1.5 non-cD 0105262201 (3.4 0.0 3.6) 0105260901 (18.6 24.4 24.3) 0105260801 (16.2 19.6 20.4)
0105262501 (3.5 7.6 7.7) 0105262001 (2.9 7.6 7.6) 0105260701 (16.1 20.6 20.5)
0105261101 (8.0 12.7 11.1) 0105262101 (4.4 5.6 7.2)
A754 0.054 8.6 4.7 non-cD 0112950301 (8.0 13.3 13.7) 0112950401 (7.6 14.3 14.3) 0136740201 (2.3 6.0 6.7)
0136740101 (12.5 14.2 14.2)

Notes. 

(a)

Adopted average temperature of ICM used to calculate r180.

(b)

The Galactic value of the hydrogen column density (Dickey & Lockman 1990).

(c)

“cD” corresponds to cD clusters, which are relaxed clusters with a cD galaxy at their center. Other clusters are classified as “non-cD.”

(d)

Obsid (a unique XMM-Newton observation identifier) and exposure times of PN, MOS1, and MOS2, respectively, after screening out the background flares.

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