Jack Sayers, Nicole G. Czakon, Carrie Bridge, Sunil R. Golwala, Patrick M. Koch, Kai-Yang Lin, Sandor M. Molnar, Keiichi Umetsu
We present Bolocam observations of two clusters of galaxies reported as
unconfirmed in the Planck early Sunyaev-Zel'dovich (eSZ) sample, PLCKESZ
G115.71 and PLCKESZ G189.84. These are the only remaining unconfirmed
candidates from the original list of eight unconfirmed candidates in the eSZ.
We observed each of these candidates with Bolocam at 140 GHz from the Caltech
Submm Observatory in October 2011. The resulting images have white noise levels
of \simeq 30 {\mu}KCMB-arcmin in their central regions. We find a significant
SZ decrement towards PLCKESZ G115.71. This decrement has a false detection
probability of 5.3\times10-5, and we therefore confirm PLCKESZ G115.71 as a
cluster. The maximum SZ decrement towards PLCKESZ G189.84 corresponds to a
false detection probability of 0.027, and it therefore remains as an
unconfirmed cluster candidate. In order to make our SZ-derived results more
robust, we have also analyzed data from the Wide-field Infrared Survey Explorer
(WISE) at the location of each cluster candidate. We find an overdensity of
WISE sources consistent with other clusters in the eSZ at the location of
PLCKESZ G115.71, providing further evidence that it is a cluster. We do not
find a significant overdensity of WISE sources at the location of PLCKESZ
G189.84, although the number of WISE sources is above average.
View original:
http://arxiv.org/abs/1112.5151
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