Milky Way fieldsa for which SDSS photometry was used to select the targets to be observe with GIRAFFE (see Appendix B1).
Milky Way fields . | ΔSDSS . |
---|---|
GES_MW_082312-052959 | – |
GES_MW_083959-003000 | 0.41 |
GES_MW_095600-003000 | – |
Milky Way fields . | ΔSDSS . |
---|---|
GES_MW_082312-052959 | – |
GES_MW_083959-003000 | 0.41 |
GES_MW_095600-003000 | – |
Note.aFor UVES targets the selection is based on 2MASS photometry.
Milky Way fieldsa for which SDSS photometry was used to select the targets to be observe with GIRAFFE (see Appendix B1).
Milky Way fields . | ΔSDSS . |
---|---|
GES_MW_082312-052959 | – |
GES_MW_083959-003000 | 0.41 |
GES_MW_095600-003000 | – |
Milky Way fields . | ΔSDSS . |
---|---|
GES_MW_082312-052959 | – |
GES_MW_083959-003000 | 0.41 |
GES_MW_095600-003000 | – |
Note.aFor UVES targets the selection is based on 2MASS photometry.
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