Results from the full sky map of Sunyaev-Zeldovich effect
(y-distortion) constructed from full mission Planck HFI public data
The CO mask is the minimal mask derived by comparing the fits to CO vs SZ
effect in arXiv:1505.00778. It masks strong sources of CO emission, in
particular the Galactic molecular clouds at high latitudes which can contaminate the SZ maps
and catalogs. The mask covers 14.2% of the sky. See the reference for details.
See arXiv:1505.00778 for details.
This is a ASCII annotated second Planck cluster
catalog which retains partial entries from the original catalog and
adds new entries identifying the cluster candidate as a molecular cloud or
a cluster. The significance of the identification as a cloud or cluster is
quantified in chi-square difference with negative values implying the
source to be a
molecular cloud (CO emission) and positive values for the cluster (SZ
effect). The table is sorted according to S/N quoted in the original
table. The columns are explained in the README file.
References:
arXiv:1410.7396
This paper describes the LIL algorithm used to separate the SZ component
arXiv:1505.00778
This paper describes the construction of the SZ maps, chi-square maps, masks and classification of the cluster catalog
candidates.
arXiv:1505.00781
This accompanying paper
uses these results from Planck data together with
the SPT cluster catalog to place upper and lower limits on the average
y-distortion monopole.
arXiv:1502.01598
Planck clusters paper
arXiv:1409.0850
SPT clusters paper
Last modified: Sun Aug 16 13:22:38 IST 2015