Selection . | No. of sources . | . |
---|---|---|
Full ALESS sample | 131 | |
ALESS MAIN sample | 99 | |
Photometric MAIN samplea | 78 | |
Photometric MAIN sample within VLA footprint | 76 | |
VLA-detected sub-sample | 52 | |
GMRT-detected sub-sampleb | 35 |
Selection . | No. of sources . | . |
---|---|---|
Full ALESS sample | 131 | |
ALESS MAIN sample | 99 | |
Photometric MAIN samplea | 78 | |
Photometric MAIN sample within VLA footprint | 76 | |
VLA-detected sub-sample | 52 | |
GMRT-detected sub-sampleb | 35 |
aFrom Simpson et al. (2013); ball GMRT 610 MHz-detected SMGs are also detected in the VLA 1.4 GHz map.
Selection . | No. of sources . | . |
---|---|---|
Full ALESS sample | 131 | |
ALESS MAIN sample | 99 | |
Photometric MAIN samplea | 78 | |
Photometric MAIN sample within VLA footprint | 76 | |
VLA-detected sub-sample | 52 | |
GMRT-detected sub-sampleb | 35 |
Selection . | No. of sources . | . |
---|---|---|
Full ALESS sample | 131 | |
ALESS MAIN sample | 99 | |
Photometric MAIN samplea | 78 | |
Photometric MAIN sample within VLA footprint | 76 | |
VLA-detected sub-sample | 52 | |
GMRT-detected sub-sampleb | 35 |
aFrom Simpson et al. (2013); ball GMRT 610 MHz-detected SMGs are also detected in the VLA 1.4 GHz map.
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