Suzaku Observations of Galaxy Groups (and related systems)

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Abundances in Groups with Suzaku: : Priorities More observations of a wide range of groups! Do with SCI (resolution matters) -- need good background tools to go to r virial Find groups where we can measure Ne (?) and Ca (?) Combine with higher angular resolution observations
Abundances in Groups with Suzaku: : Priorities Connect to cosmological context SDSS statistical M/L vs. Suzaku individual, star formation/halo connection -- an X-ray analog? Go to higher redshift (see Miller et al. Poster A22) Balestra et al. 2007 clusters
Page 1 and 2: Suzaku Observations of Galaxy Group
Page 3 and 4: Matter in the Universe (the modern
Page 5 and 6: Sub-types of interest X-ray: NASA/C
Page 7 and 8: Why Study Groups in X-rays? • The
Page 9 and 10: ROSAT and ASCA Highlights • Abund
Page 11 and 12: XMM-Newton and Chandra More heating
Page 13 and 14: XMM-Newton and Chandra • High res
Page 15 and 16: Cool (
Page 17 and 18: Temperature Structure XIS requires
Page 19 and 20: Abundances RGS: N(?), O, Ne, Mg, Fe
Page 21 and 22: Complementarity, , e.g. NGC 4472
Page 23 and 24: Abundance Profiles courtesy K. Mats
Page 25 and 26: Abundance Patterns Similar pattern
Page 27: Abundances in Groups with Suzaku: :

Suzaku Observations of Galaxy Groups (and related systems)

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