PSZ2 G091.83+26.11 is a galaxy cluster with M500 = 7.43 x 10^14 Msun at z = 0.822 1. This object exhibits a complex morphology with a clear bimodality observed in X-rays. However, it was detected and analysed in the Planck sample as a single, spherical cluster following a universal profile 2. This model can lead to miscalculations of thermodynamical quantities, like the pressure profile. As future multiwavelength cluster experiments will detect more and more objects at high redshifts, it is crucial to quantify this systematic effect. In this work, we use high-resolution observations of the NIKA2 camera3,4,5,6 to integrate the morphological characteristics of the cluster in our modelling. This is achieved by fitting a two-halo model to the SZ image and then by reconstruction of the resulting projected pressure profile. We then compare these results with the spherical assumption.
@article{arxiv.2204.14052,
title = {Massive merging cluster PSZ2G091 as seen by the NIKA2 camera},
author = {E. Artis and R. Adam and P. Ade and H. Ajeddig and P. André and M. Arnaud and H. Aussel and I. Bartalucci and A. Beelen and A. Benoît and S. Berta and L. Bing and O. Bourrion and M. Calvo and A. Catalano and M. De Petris and F. -X. Désert and S. Doyle and E. F. C. Driessen and A. Ferragamo and A. Gomez and J. Goupy and C. Hanser and F. Kéruzoré and C. Kramer and B. Ladjelate and G. Lagache and S. Leclercq and J. -F. Lestrade and J. -F. Macías-Pérez and A. Maury and P. Mauskopf and F. Mayet and A. Monfardini and M. Muñoz-Echeverría and A. Paliwal and L. Perotto and G. Pisano and E. Pointecouteau and N. Ponthieu and G. W. Pratt and V. Revéret and A. J. Rigby and A. Ritacco and C. Romero and H. Roussel and F. Ruppin and K. Schuster and S. Shu and A. Sievers and C. Tucker and G. Yepes},
journal= {arXiv preprint arXiv:2204.14052},
year = {2022}
}
Comments
4 pages, 3 figures Contribution to the 2022 Cosmology session of the 56th Rencontres de Moriond. arXiv admin note: substantial text overlap with arXiv:2111.05082