Table 2

Surveys included in the first release of the CeSAM XXL database and contributing to our galaxy sample.

SpecOrigin in the Parent survey and references Field Type
spectroscopic database
AAT_AAOmega Lidman et al. (2016) – XXL Paper XIV S PI XXL
AAT_AAOmega_GAMA GAMA, Baldry et al. (2018) N E
AAOmega2012 XXL Paper XX N PI XXL
Akiyama Akiyama et al. (2015) N E
Alpha_compilation Adami et al. (2011) N PI XMMLSS + E
ESO_Large_Programme XXL Paper XX N+S PI XXL
LDSS03 Adami et al. (2011) N PI XMMLSS
Magellan XXL Paper XX N E (XXL agreement)
Milano Adami et al. (2011) N PI XMMLSS + E
NED N+S E
NTT Adami et al. (2011) N+S PI XMMLSS
SDSS_DR10 SDSS, Ahn et al. (2014) N E
Simpson Simpson et al. (2012) N E
SNLS Balland et al. (2018) N E
Stalin Stalin et al. (2010) N E
Subaru Akiyama et al. (2015) N E
VIPERS/XXL and VIPERS_2DR VIPERS, (Scodeggio et al. 2018) N E
VVDS_Deep VVDS, Le Fèvre et al. (2005) N E
VVDS_UD VUDS, Le Fèvre et al. (2015) N E
XMMLSS Adami et al. (2011) N PI XMMLSS
WHT Koulouridis et al. (2016) – XXL Paper XII N PI XXL

Notes. Entries in the first column are reported as they appear in the SpecOrigin column in the original database, and in the second column theyhave been grouped into main surveys and observing programmes relative to a given instrument or telescope. The Field column indicates which XXL area is covered by the survey (North (N), South (S), or both), and the Type column indicates the source of the data: E (External), PI (XXL or XMMLSS PI).

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