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Table 1
Spectroscopic cluster members of XMMU J1007.4+1237.
| ID | RA | Dec | H | z − H | dcen | rproj | SFR | zspec | Comment |
| J2000 | J2000 | mag | mag | ″ | kpc | M⊙ yr-1 | |||
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|
|||||||||
| 1 | 10:07:21.8 | +12:37:51.5 | 19.2 | 3.2 | 4.3 | 37 | 11 | 1.556 | BCG |
| 2 | 10:07:21.4 | +12:38:05.1 | 19.6 | 3.8 | 10.9 | 92 | 5 | 1.530 | Δv = −2900 km s-1 |
| 3 | 10:07:20.8 | +12:37:59.6 | 19.7 | 2.1 | 12.3 | 104 | 75 | 1.554 | strong [O ii] |
| 4 | 10:07:22.9 | +12:37:56.7 | 20.4 | 2.6 | 20.8 | 176 | 31 | 1.558 | strong [O ii] |
Notes. Listed are total Vega H-band magnitudes, z − H colors, projected cluster-centric distances in arcseconds and kpc relative to the X-ray center (see Table 2), and first estimates of the ongoing SF activity following Kennicutt (1992).
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