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The Initial Mass Function and Other Stellar Properties Across the Core of the Hydra I Cluster

  • Authors: Ilaria Lonoce, W. L. Freedman, A. Feldmeier-Krause

Ilaria Lonoce et al 2023 The Astrophysical Journal 948 .

  • Provider: AAS Journals

Caption: Figure 1.

Upper panel: S/N per Å trends along the slit direction as measured for each CCD chip on the final reduced spectra. The pixel scale is 0.111 per pixel. In detail: chip7-GA = 9.°71 covers ∼3500–4300 Å (orange), chip8-GA = 9.°71 ∼4300–5100 Å (green), chip5-GA = 9.°71 5100–5900 Å (red), chip6-GA = 9.°71 5900–6700 Å (blue), and chip8-GA = 17.°11 ∼8000–8800 Å(brown). Lower panel: light profile along the slit that connects the two target galaxies NGC3309 (green) and NGC3311 (pink). Shades highlight the region within 1R e for each galaxy, i.e., ﹩{{\rm{R}}}_{e}^{3309}=21.9﹩ and ﹩{{\rm{R}}}_{e}^{3311}=36.2﹩ (Arnaboldi et al. 2012). Crosses indicate the central position of each region where a spectrum has been extracted.

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