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Table B.1.

Comparison of the masses inferred using ACT data to those from SZ observations with CARMA (Gonzalez et al. 2019a), ACA (Di Mascolo et al. 2020), MUSTANG2 (Dicker et al. 2020), and NIKA2 (Ruppin et al. 2020).

Cluster ID M500,ACT M500,ACA(a) M500,CARMA(b) M500, MUSTANG 2(c) M500, NIKA 2(d)
[1014M] [1014M] [1014M] [1014M] [1014M]
MOO J0105+1324
MOO J0129−1640
MOO J0319−0025
MOO J1014+0038
MOO J1142+1527 6.06 ± 3.47
MOO J1322−0228
MOO J1354+1329
MOO J1414+0227
MOO J1514+1346
MOO J1521+0452
MOO J2146−0320
MOO J2206+0906
MOO J2231+1130

Notes.

(c)

Dicker et al. 2020. A full treatment of the uncertainty is available in the publication.

(d)

The NIKA2 measurement, as reported in Ruppin et al. 2020, relied on a strong, informative prior on the integrated SZ signal from CARMA (Gonzalez et al. 2019a) and hence should likely not be regarded as an independent constraint. We include it for completeness, and note they include a large, 56% systematic uncertainty. All three surveys assumed the Arnaud et al. (2010) scaling relation.

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