The XXL Survey. V. Detection of the Sunyaev-Zel'dovich Effect of the Redshift 1.9 Galaxy Cluster XLSSU J021744.1–034536 with CARMA

• Published in: The Astrophysical Journal
• Main Authors: Mantz, A. B., Abdulla, Z., Carlstrom, J. E., Greer, C. H., Leitch, E. M., Marrone, D. P., Muchovej, S., Adami, C., Birkinshaw, M., Bremer, M., Clerc, N., Giles, P.
• Format: Article in Journal/Newspaper
• Language: English
• Published: American Astronomical Society 2014
• Subjects: South Pole; South pole
• Online Access: https://authors.library.caltech.edu/51727/; https://authors.library.caltech.edu/51727/1/0004-637X_794_2_157.pdf; https://authors.library.caltech.edu/51727/7/1401.2087v2.pdf; https://resolver.caltech.edu/CaltechAUTHORS:20141113-155029950

We report the detection of the Sunyaev-Zel'dovich (SZ) effect of galaxy cluster XLSSU J021744.1–034536, using 30 GHz Combined Array for Research in Millimeter-wave Astronomy (CARMA) data. This cluster was discovered via its extended X-ray emission in the XMM- Newton Large Scale Structure survey, the precursor to the XXL survey. It has a photometrically determined redshift z = 1.91^(+0.19)_(-0.21), making it among the most distant clusters known, and nominally the most distant for which the SZ effect has been measured. The spherically integrated Comptonization is Y _500 = (3.0 ± 0.4) × 10^(–12), a measurement that is relatively insensitive to assumptions regarding the size and redshift of the cluster, as well as the background cosmology. Using a variety of locally calibrated cluster scaling relations extrapolated to z ~ 2, we estimate a mass M _500 ~ (1-2) × 10^(14) M ☉ from the X-ray flux and SZ signal. The measured properties of this cluster are in good agreement with the extrapolation of an X-ray luminosity-SZ effect scaling relation calibrated from clusters discovered by the South Pole Telescope at higher masses and lower redshifts. The full XXL-CARMA sample will provide a more complete, multi-wavelength census of distant clusters in order to robustly extend the calibration of cluster scaling relations to these high redshifts.