Abstract
Abstract
We present a joint analysis of the power spectra of the Planck Compton y parameter map and the projected galaxy density field using the Wide Field Infrared Survey Explorer (WISE) all-sky survey. We detect the statistical correlation between WISE and Planck data (gy) with a significance of 21.8σ. We also measure the autocorrelation spectrum for the thermal Sunyaev–Zel’dovich (tSZ) (yy) and the galaxy density field maps (gg) with a significance of 150σ and 88σ, respectively. We then construct a halo model and use the measured correlations
C
ℓ
gg
,
C
ℓ
yy
, and
C
ℓ
g
y
to constrain the tSZ mass bias
B
≡
M
500
/
M
500
tSZ
. We also fit for the galaxy bias, which is included with explicit redshift and multipole dependencies as
b
g
(
z
,
ℓ
)
=
b
g
0
(
1
+
z
)
α
(
ℓ
/
ℓ
0
)
β
, with ℓ
0 = 117. We obtain the constraints to be B = 1.50 ± 0.07(stat) ± 0.34(sys), i.e., 1 − b
H = 0.67 ± 0.03(stat) ± 0.16(sys) (68% confidence level) for the hydrostatic mass bias, and
b
g
0
=
1.28
−
0.04
+
0.03
(
stat
)
±
0.11
(
sys
)
, with
α
=
0.20
−
0.07
+
0.11
(
stat
)
±
0.10
(
sys
)
and β = 0.45 ±0.01(stat) ± 0.02(sys) for the galaxy bias. Incoming data sets from future CMB and galaxy surveys (e.g., Rubin Observatory) will allow probing the large-scale gas distribution in more detail.
Funder
National Research Foundation
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Cited by
7 articles.
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