Table 7
Summary with the source of the optical and infrared photometry or the 205 counterparts of the 164 XMM-Newton sources, and some properties of the possible and probable members.
Survey | All counterparts | Probable/Possible members |
Number | Number | |
(205 total) | (69 total)1 | |
|
||
B or V OM | 372 | 264 |
RI Dolan and Mathieu | 53 | 42 |
RI CFHT or ByN | 84 | 13 |
JHK 2MASS | 63 | 35 |
JHK Omega2000 | 76 | 2 |
JHK ByN2007 | 31 | 33 |
IRAC | 163 | 64 |
MIPS | 16 (2)3 | 10 (2)3 |
|
||
Probable members | – | 61 |
Possible members | – | 5 |
Possible companions | – | 3 |
Listed in DM1999 | – | 355 |
Listed in ByN2004 | – | 316 |
Class II9 | – | 47 |
Class III9 | – | 628 |
Notes.
55 Class III and no disk. Other two with transition disks (24 micron excess), other two with thin disks (based on IRAC slope), and another two with possible Class III based on SED (incomplete IRAC data). Finally, one has no IRAC data, but its 24 micron flux indicates it is a Class III with a transition disk.
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