Intend to look at the properties below in 2-3 SAMs; few hydro runs, HOD:
- BCG mass vs halo mass
- radius
- age
- metallicity
- star formation rate (SFR)
- close companions?
- Brightness difference between first and second brightest galaxy (M1-M2)
stellarmass_colour copy.pdf
g-r colours are similar to those observed in SDSS (von der Linden+2007)
stellarmass_SFR copy.pdf
SFR are similar to observed
stellarmass_radius copy.pdf
radii are similar to those observed (Jimmy+2012)
---
st_age_metallicity copy.pdf
- ages are similar in range to those observed in similar mass clusters (Oliva-Altamirano+2015)
- however, metallicities are significantly different.
stellarmass_Z copy.pdf
- range of metallicities and stellar masses much wider than observed
stellarmass_dominance copy.pdf
- dominance > 2 is regarded as extreme and seen in only 7% of LOCUSS clusters (Smith+10)
Comments (1)
sarah.brough@aao.gov.au said
at 2:07 am on Mar 24, 2015
Intend to look at the properties below in 2-3 SAMs; few hydro runs, HOD:
- BCG mass vs halo mass
- radius
- age
- metallicity
- star formation rate (SFR)
- close companions?
- Brightness difference between first and second brightest galaxy (M1-M2)
You don't have permission to comment on this page.