Table 3
Spectroscopic data available in the XXL fields at the end of 2015.
| Instrument/Programme | Field | Resolution | Coverage | Type | Status |
|
|
|||||
| VIMOS/VIPERS | N | R = 200 | 16 deg2 | E-S | C |
| BOSS ancillary programme | N | R = 1400−2600 | ~25 deg2AGNs | E-S | C |
| AAOmega/GAMA field G02 | N | R = 1400 | 23.5 deg2 overlap with XXL | E-S | C |
| SDSS DR10 | N | R = 1300−3000 | larger than XXL | E-S | C |
| WHT | N | R = 800 | detailed studies of groups and clusters | PI-T | OG |
| NTT | N+S | R = 300 | individual clusters | PI*-T | OG |
| FORS2 | N+S | R = 600 | individual clusters | PI*-T | OG |
| AAOmega | S | R = 1400 | 25 deg2clusters + AGNs | PI-S | C |
Notes. The ⟨Type⟩ column indicates the source of the data: E (external), PI (XXL PI), and whether the observations are conducted in survey mode (S) or using target XXL sources (T). The ⟨Status⟩ column indicates whether the observations are completed (C) or on-going (OG). The * stands for ESO Large Programme. More detailed information, maps, and references are available at http://xxlmultiwave.pbworks.com.
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