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The Dipole Anisotropy of the 2MASS
Redshift Survey
Pirin Erdoğdu
(University of Nottingham)
and the 2MRS Team
MNRAS, in press
OUTLINE
What is the 2MASS Redshift Survey?
What is the acceleration on our Local Group
of galaxies?
Why do I think I am right?
Main Assumptions
CMB dipole is due to the motion of the Sun.
Linear theory of density perturbations is
acceptable.
The 2MASS has constant mass-to-light ratio
and linear bias.
The 2MASS Redshift Survey
z ≤ 0.01 0.01 < z ≤ 0.025 0.025 < z < 0.05 0.05 ≤ z
Number Weighting Technique
If we have a perfect 3-dimensional
galaxy catalogue with same mass, with no selection
effects, no z-distortions and with linear biasing then
Linear theory:
Linear theory:
r
G
g 0 G d r m r 3
r
b
0
3
rˆi
i r 2
i
H0
v0
g 0
4G
m
b
0.6
From CMB: vLG = 627
km/sec towards l=273o and
b=29o
From galaxy cat.
The 2MRS Redshift Distribution
The Rocket Effect
(Kaiser, 1987)
cz=H0r + (vpec- v(0)).(r/r)
LG
Gal 2 with d = 100 km/sec v pec= -20 km/sec
Thus calculated distance=80 km/sec
Thus calculated dipole = 64 % more than the
Real dipole
Gal 1 with d=100 km/sec v pec = 20 km/sec
Thus calculated distance=120 km/sec
Thus calculated dipole= 44% less than
the real dipole
Net effect: A spurious contribution to the LG dipole from
All the galaxies.
Flux Weighting Technique
If we have a perfect 2-dimensional
galaxy catalogue with no selection effects, constant mass-tolight ratio and with linear biasing then
ˆ
ri
M
g (0) G M i 2 G
ri
L
i
M
4G
L
since
ˆ
Si ri
i
L
S
2
4r
ˆ
ri
Li 2
ri
i
Luminosity Weighting Function
Notice the Zone of Avodiance
Star: CMB
Triangle: 2MRS – Lum
Weighted
Triangle: 2MRS-Num
Weighted
Circle: 2MASS by Maller
etal 2003
Upside down Triangle:
IRAS PSCz Dipole
Upside down Triangle:
2MASS dipole of PSCz
galaxies
Triangle: 2MRS – Lum
Weighted without Maffei 1,
2, Dwingeloo 1, IC342, M87
Blue square: Dipole from XRay Clusters (Kocevski &
Ebeling 2005)
Shapley
Centaurus
Hydra
To summarise…
The flux weighted galaxy dipoles are better.
Most of the LG dipole is caused by the tug-of-war
between the GA and Per-Pis. The dipole
converges by ~ 60 Mpc/h.
If dipole converged β2mrs = 0.4±0.1
Small discrepancy between LG and CMB dipoles
are due to ZoA, 2nd and 3rd assumptions
mentioned in the earlier slide and structure
beyond. But no big deal!