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Table 3
Projected masses of Abell 1835.
| R | M Chandra | M XMM − Newton | M Chandra(T = TXMM) | M wl | |||
| 1014 M⊙ | 1014 M⊙ | 1014 M⊙ | 1014 M⊙ | ||||
|
|
|||||||
| r 2500 | 4.42 ± 0.52 | 3.15 ± 0.62 | 3.28 ± 0.40 | 2.88 ± 0.58 | |||
| r 1000 | 7.11 ± 1.86 | 5.80 ± 1.42 | 5.28 ± 1.39 | 6.15 ± 0.95 | |||
| r 500 | 13.80 ± 3.91 | 8.99 ± 3.60 | 8.19 ± 3.21 | 9.65 ± 1.70 | |||
Notes. The weak lensing masses are reported in Zhang et al. (2010). r2500, r1000 and r500 are determined from the weak lensing analysis.
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