Free Access
| LAE candidates | |||||||||
| LAE_ |
 |
 |
 |
HR1 | HR2 |
 |
Offset |
 |
Offset |
| COSMOS_# | (X-ray) | (Radio) | |||||||
| 25 |
 |
 |
 |
 |
 |
 |
11.06 | -- | -- |
| 36 | -- | -- | -- | -- | -- | -- | -- |  |
0.10 |
| 57 | -- | -- | -- | -- | -- | -- | -- |  |
6.17 |
| 82 |
 |
-- | -- | <0.52 | -- |
 |
1.07 | -- | -- |
| 101 | -- | -- | -- | -- | -- | -- | -- |  |
0.06 |
| 113 |
 |
 |
-- |
 |
<0.01 |
 |
10.55 | -- | -- |
| 115 |
 |
 |
-- |
 |
<-0.25 |
 |
0.17 | -- | -- |
| 119 |
 |
-- | -- | <0.63 | -- |
 |
2.67 | -- | -- |
| 121 |
 |
 |
 |
 |
 |
 |
6.36 | -- | -- |
| 129 |
 |
-- | -- | <0.57 | -- |
 |
1.95 | -- | -- |
| 132 | -- | -- | -- | -- | -- | -- | -- | |
9.83 |
| 140 |
 |
 |
 |
 |
 |
 |
0.74 | -- | -- |
| 150 |
 |
 |
-- |
 |
<0.08 |
 |
0.62 |  |
0.21 |
| 161 |
 |
-- | -- | <0.25 | -- |
 |
0.21 | -- | -- |
| GALEX-detected candidates | |||||||||
| 42 |
 |
-- | -- | <-0.10 | -- |
 |
0.55 | -- | -- |
| 108 |
 |
 |
-- |
 |
<-0.27 |
 |
1.01 | -- | -- |
| 126 |
 |
 |
-- |
|
<-0.11 |
 |
0.45 | -- | -- |
| 155 |
 |
 |
-- |
 |
<0.27 |
 |
1.57 | -- | -- |
| 173 | -- | -- | -- | -- | -- | -- | -- |  |
9.44 |
Data from the catalogues of Cappelluti et al. (2007) and Schinnerer et al. (2007). X-ray fluxes are given in units of 10-15 erg s-1 cm-2 and radio fluxes in units of  Jy. HR1 and HR2 correspond to the hardness ratios defined in Eqs. (4) and (5). The X-ray luminosity is in erg s-1, assuming the objects are located at redshifts z = 2.25 and 0.06 for LAE and GALEX-detected candidates respectively. Offsets are distance from centroid of narrow-band detection to X-ray/radio detection in units of arcseconds. It is expected that the objects with offsets larger than a few arcseconds (25, 57, 113, 121, 132 and 173) are unrelated to the candidates due to the large offset and the relatively large probability of random association.
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