Atacama Cosmology Telescope measurements of a large sample of candidates from the Massive and Distant Clusters of WISE Survey - Sunyaev-Zeldovich effect confirmation of MaDCoWS candidates using ACT

Free Access

Table 1.

Stacks of values for the MaDCoWS cluster candidates.

λ_15, low	λ_15, high	# in bin	[10⁻⁴]
10	20	191	(0 ± 1) × 10⁻²
20	30	401	(30 ± 8) × 10⁻³
30	40	251	(54 ± 9) × 10⁻³
40	50	94	(20 ± 3) × 10⁻²
50	60	34	(40 ± 8) × 10⁻²
60	100	13	(53 ± 9) × 10⁻²

Notes. The above stacked values of exclude the co-detections, as discussed in Sect. 4 and shown in Fig. 4. The value λ_15, low denotes the lower edge (exclusive) used for binning, and λ_15, high denotes the upper edge (inclusive) used for binning. The uncertainty on is calculated via bootstrapping.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.