Figure 19.
![The metallicity distribution of all Milky Way field stars observed with GIRAFFE in the Gaia-ESO Survey iDR4. (a, c) and (b, d) show metallicity distribution of stars within blue and red boxes, respectively. The blue and red lines show the observed metallicity; the black dashed lines show weighted metallicity distributions. Only stars with [Fe/H] < 0.50 are included.](https://oup.silverchair-cdn.com/oup/backfile/Content_public/Journal/mnras/460/1/10.1093_mnras_stw1011/2/stw1011fig19.jpeg?Expires=1750066614&Signature=SfpgsVuTGX48X-A8Wrj-4z~2AZMz9Uha5WjQumcE5K2eLuDto81uI16HGdLtHMXov~6am49gShROGLttV0dNJPkk~4ftgyDd2EC6zLaRFphtzTZ~J8fvnbRjyhPVnlVPaovuIjVewkUIe8qyXK1VOOAL8TStSEknirUofVCfg896ZX6CntBBiITkUF0F6Et-ByhW9lv7dVBTWrc17BY--FGH-mMPomF4f60pAIy5Re7OJ-hyvdcpB9IfmyiAidVoqGT63DhB9icgeBuwnoxISfZLbbQkvZuNlNFQA5Uk3pIvU5aEwQldzjGwTYYYOHfY4h0d5kwGG8j8fPGLijBvjA__&Key-Pair-Id=APKAIE5G5CRDK6RD3PGA)
The metallicity distribution of all Milky Way field stars observed with GIRAFFE in the Gaia-ESO Survey iDR4. (a, c) and (b, d) show metallicity distribution of stars within blue and red boxes, respectively. The blue and red lines show the observed metallicity; the black dashed lines show weighted metallicity distributions. Only stars with [Fe/H] < 0.50 are included.
