Spectroscopic data available in the XXL fields at the end of 2015.
|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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