%0 Generic %1 to2020energy %A To, C. %A Krause, E. %A Rozo, E. %A Wu, H. %A Gruen, D. %A Wechsler, R. H. %A Eifler, T. F. %A Rykoff, E. S. %A Costanzi, M. %A Becker, M. R. %A Bernstein, G. M. %A Blazek, J. %A Bocquet, S. %A Bridle, S. L. %A Cawthon, R. %A Choi, A. %A Crocce, M. %A Davis, C. %A DeRose, J. %A Drlica-Wagner, A. %A Elvin-Poole, J. %A Fang, X. %A Farahi, A. %A Friedrich, O. %A Gatti, M. %A Gaztanaga, E. %A Giannantonio, T. %A Hartley, W. G. %A Hoyle, B. %A Jarvis, M. %A MacCrann, N. %A McClintock, T. %A Miranda, V. %A Pereira, M. E. S. %A Park, Y. %A Porredon, A. %A Prat, J. %A Rau, M. M. %A Ross, A. J. %A Samuroff, S. %A Sánchez, C. %A Sevilla-Noarbe, I. %A Sheldon, E. %A Troxel, M. A. %A Varga, T. N. %A Vielzeuf, P. %A Zhang, Y. %A Zuntz, J. %A Abbott, T. M. C. %A Aguena, M. %A Annis, J. %A Avila, S. %A Bertin, E. %A Bhargava, S. %A Brooks, D. %A Burke, D. L. %A Rosell, A. Carnero %A Kind, M. Carrasco %A Carretero, J. %A Chang, C. %A Conselice, C. %A da Costa, L. N. %A Davis, T. M. %A Desai, S. %A Diehl, H. T. %A Dietrich, J. P. %A Everett, S. %A Evrard, A. E. %A Ferrero, I. %A Flaugher, B. %A Fosalba, P. %A Frieman, J. %A García-Bellido, J. %A Gruendl, R. A. %A Gutierrez, G. %A Hinton, S. R. %A Hollowood, D. L. %A Huterer, D. %A James, D. J. %A Jeltema, T. %A Kron, R. %A Kuehn, K. %A Kuropatkin, N. %A Lima, M. %A Maia, M. A. G. %A Marshall, J. L. %A Menanteau, F. %A Miquel, R. %A Morgan, R. %A Muir, J. %A Myles, J. %A Palmese, A. %A Paz-Chinchón, F. %A Plazas, A. A. %A Romer, A. K. %A Roodman, A. %A Sanchez, E. %A Santiago, B. %A Scarpine, V. %A Serrano, S. %A Smith, M. %A Suchyta, E. %A Swanson, M. E. C. %A Tarle, G. %A Thomas, D. %A Tucker, D. L. %A Weller, J. %A Wester, W. %D 2020 %K library %T Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations %U http://arxiv.org/abs/2010.01138 %X Combining multiple observational probes is a powerful technique to provide robust and precise constraints on cosmological parameters. In this letter, we present the first joint analysis of cluster abundances and auto/cross correlations of three cosmic tracer fields measured from the first year data of the Dark Energy Survey: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis of cluster abundances, three cluster cross-correlations, and auto correlations of galaxy density, we obtain $Ømega_m=0.305^+0.055_-0.038$ and $\sigma_8=0.783^+0.064_-0.054$. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat $\nuŁambda$CDM model. We thus combine cluster abundances and all two-point correlations from three cosmic tracer fields and find improved constraints on cosmological parameters as well as on the cluster observable--mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multi-probe analyses of upcoming wide imaging surveys.

@misc{to2020energy, abstract = {Combining multiple observational probes is a powerful technique to provide robust and precise constraints on cosmological parameters. In this letter, we present the first joint analysis of cluster abundances and auto/cross correlations of three cosmic tracer fields measured from the first year data of the Dark Energy Survey: galaxy density, weak gravitational lensing shear, and cluster density split by optical richness. From a joint analysis of cluster abundances, three cluster cross-correlations, and auto correlations of galaxy density, we obtain $\Omega_{\rm{m}}=0.305^{+0.055}_{-0.038}$ and $\sigma_8=0.783^{+0.064}_{-0.054}$. This result is consistent with constraints from the DES-Y1 galaxy clustering and weak lensing two-point correlation functions for the flat $\nu\Lambda$CDM model. We thus combine cluster abundances and all two-point correlations from three cosmic tracer fields and find improved constraints on cosmological parameters as well as on the cluster observable--mass scaling relation. This analysis is an important advance in both optical cluster cosmology and multi-probe analyses of upcoming wide imaging surveys.}, added-at = {2020-10-06T07:37:56.000+0200}, author = {To, C. and Krause, E. and Rozo, E. and Wu, H. and Gruen, D. and Wechsler, R. H. and Eifler, T. F. and Rykoff, E. S. and Costanzi, M. and Becker, M. R. and Bernstein, G. M. and Blazek, J. and Bocquet, S. and Bridle, S. L. and Cawthon, R. and Choi, A. and Crocce, M. and Davis, C. and DeRose, J. and Drlica-Wagner, A. and Elvin-Poole, J. and Fang, X. and Farahi, A. and Friedrich, O. and Gatti, M. and Gaztanaga, E. and Giannantonio, T. and Hartley, W. G. and Hoyle, B. and Jarvis, M. and MacCrann, N. and McClintock, T. and Miranda, V. and Pereira, M. E. S. and Park, Y. and Porredon, A. and Prat, J. and Rau, M. M. and Ross, A. J. and Samuroff, S. and Sánchez, C. and Sevilla-Noarbe, I. and Sheldon, E. and Troxel, M. A. and Varga, T. N. and Vielzeuf, P. and Zhang, Y. and Zuntz, J. and Abbott, T. M. C. and Aguena, M. and Annis, J. and Avila, S. and Bertin, E. and Bhargava, S. and Brooks, D. and Burke, D. L. and Rosell, A. Carnero and Kind, M. Carrasco and Carretero, J. and Chang, C. and Conselice, C. and da Costa, L. N. and Davis, T. M. and Desai, S. and Diehl, H. T. and Dietrich, J. P. and Everett, S. and Evrard, A. E. and Ferrero, I. and Flaugher, B. and Fosalba, P. and Frieman, J. and García-Bellido, J. and Gruendl, R. A. and Gutierrez, G. and Hinton, S. R. and Hollowood, D. L. and Huterer, D. and James, D. J. and Jeltema, T. and Kron, R. and Kuehn, K. and Kuropatkin, N. and Lima, M. and Maia, M. A. G. and Marshall, J. L. and Menanteau, F. and Miquel, R. and Morgan, R. and Muir, J. and Myles, J. and Palmese, A. and Paz-Chinchón, F. and Plazas, A. A. and Romer, A. K. and Roodman, A. and Sanchez, E. and Santiago, B. and Scarpine, V. and Serrano, S. and Smith, M. and Suchyta, E. and Swanson, M. E. C. and Tarle, G. and Thomas, D. and Tucker, D. L. and Weller, J. and Wester, W.}, biburl = {https://www.bibsonomy.org/bibtex/24e081e9ea54bf072cba4126dab5ce3ab/gpkulkarni}, description = {Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations}, interhash = {8dcbb68332764df3c136d92a4e5fd7b9}, intrahash = {4e081e9ea54bf072cba4126dab5ce3ab}, keywords = {library}, note = {cite arxiv:2010.01138Comment: 14 pages, 7 figures, 2 tables; submitted to PRL; comments are welcome}, timestamp = {2020-10-06T07:37:56.000+0200}, title = {Dark Energy Survey Year 1 Results: Cosmological Constraints from Cluster Abundances, Weak Lensing, and Galaxy Correlations}, url = {http://arxiv.org/abs/2010.01138}, year = 2020 }