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P h o t o z z=0.8 z=0.6 z=0.4 z=0.2 I AB
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1
Photozz=0.8z=0.6z=0.4z=0.2
IAB<25
1.4Mio galaxies
X-raycontours
X-ray galaxy groups in zCOSMOS
Alexis FinoguenovAlexis FinoguenovMPE/UMBCMPE/UMBC
+zCOSMOS team+zCOSMOS team
Alexis FinoguenovView on baryons from
COSMOS 3
N(z)=>2
X-ray+red sequence: 278Xray+spectroscopy:195z<0.8 152/175 91%0.8<z<1 37/50 74%z>1 6/53 11%
Alexis FinoguenovView on baryons from
COSMOS 4
X-ray only groups
How X-ray groups are different from spectroscopic groups?
5
Spec. completeness is better at low zBut drops faster with redshift
Comparison of a group definition
Alexis FinoguenovView on baryons from
COSMOS 6
X-ray onlySpec-z groups with X-raysSpec-z 3 member groups, no X-rays: stacked X-ray signal @<2.e-16>@z>0.8 X-rays (`a 6.e-
16 cgs) are more sensitive group tracercompared to IAB<22.5 galaxies
Inside dense LSSFraction of X-ray groupsincreases by a factor of 2
Stacked X-ray detection of Knobel groups
Redshift Flux (cgs) Lx (0.1-2.4 keV)
M200Msun
kT (keV)
0.9-1.1 1.6e-16 2.e42 1.7e13 0.7
0.7-0.9 9.e-17 1.e42 1.1e13 0.6
0.4-0.7 4.e-17 6.e40 0.4e13 0.3
0.1-0.30.37
1.e-16 4.e-16
8.e40 1.6e41
0.3e13 0.5e13
0.30.4
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COSMOS 7
8
Stacked detectionof spectro-z groups
Lx-sigma relation
Alexis FinoguenovView on baryons from
COSMOS 9
10
LSS at 0.12, 0.22, 0.34, 0.37, 0.51, 0.73, 0.89(Optical groups:0.22,0.36,0.38)
K.Kovac
Resolving LSS with X-ray groups
Alexis FinoguenovView on baryons from
COSMOS 11
12A. Faltenbacher, AF, N. Drory 2010 ApJ
Fraction of matter resolved in groups
Simulations…
Alexis Finoguenov
Environmental dependence of galaxy mass function
Alexis FinoguenovView on baryons from
COSMOS 13
No change in HOD!
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COSMOS 14
Bump in galaxy mass function:centrals vs sattelites
Alexis FinoguenovView on baryons from
COSMOS 15
Conclusions
X-ray groups approach the status of being spectroscopically confirmed.
X-ray groups are not a subsample of spectroscopic groups
Groups are tracers of density field and can be used to overcome to sample variance.
Alexis FinoguenovView on baryons from
COSMOS 16
People involved Masayuki Tanaka – properties of galaxies in X-ray groups using
zCOSMOS Stefania Giodini – HOD of galaxies, galaxy mass function, fossil groups Alexie Leauthaud – properties of BCGs Berian James – conditional mass function – modeling Andreas Faltenbacher – conditional mass function – simulations Katarina Kovac – density fields Angela Iovino, Michol Bolzonella, Olga Cucciatti – properties of galaxies Viola Allevato (my PhD student) – clustering analysis Michael Ballogh – 10 groups at z~0.9 with Gemini Masayuki Tanaka – groups at z>1 with Subaru Mara Salvato – high-z clusters Simona Mei et al. FORS2 program – already 350 redshifts for groups
added (or 30% of total number) And likely you! (a number of on-going efforts!)
Alexis FinoguenovView on baryons from
COSMOS 17