Bibcode
Vogt, S. M. L.; Bocquet, S.; Davies, C. T.; Mohr, J. J.; Schmidt, F.; Ruan, C. -Z.; Li, B.; Hernández-Aguayo, C.; Grandis, S.; Bleem, L. E.; Klein, M.; Schrabback, T.; Aguena, M.; Brooks, D.; Burke, D. L.; Campos, A.; Carnero Rosell, A.; Carretero, J.; Costanzi, M.; da Costa, L. N.; Pereira, M. E. S.; De Vicente, J.; Doel, P.; Everett, S.; Ferrero, I.; Frieman, J.; García-Bellido, J.; Gatti, M.; Giannini, G.; Gruen, D.; Gruendl, R. A.; Hinton, S. R.; Hollowood, D. L.; Lee, S.; Lima, M.; Marshall, J. L.; Mena-Fernández, J.; Miquel, R.; Myles, J.; Paterno, M.; Pieres, A.; Plazas Malagón, A. A.; Reichardt, C. L.; Romer, A. K.; Samuroff, S.; Sarkar, A.; Sanchez, E.; Sevilla-Noarbe, I.; Smith, M.; Suchyta, E.; Swanson, M. E. C.; Tarle, G.; Vikram, V.; Weaverdyck, N.; Weller, J.; SPT Collaboration; DES Collaboration
Bibliographical reference
Physical Review D
Advertised on:
2
2025
Journal
Citations
5
Refereed citations
0
Description
We present constraints on the f(R) gravity model using a sample of 1005 galaxy clusters in the redshift range 0.25–1.78 that have been selected through the thermal Sunyaev-Zel'dovich effect from South Pole Telescope data and subjected to optical and near-infrared confirmation with the multicomponent matched filter algorithm. We employ weak gravitational lensing mass calibration from the Dark Energy Survey Year 3 data for 688 clusters at z<0.95 and from the Hubble Space Telescope for 39 clusters with 0.63×1014M⊙.