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Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback

Fuente: arXiv

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Detalles Bibliográficos
Autores principales:	Bigwood, L., Amon, A., Schneider, A., Salcido, J., McCarthy, I. G., Preston, C., Sanchez, D., Sijacki, D., Schaan, E., Ferraro, S., Battaglia, N., Chen, A., Dodelson, S., Roodman, A., Pieres, A., Ferte, A., Alarcon, A., Drlica-Wagner, A., Choi, A., Navarro-Alsina, A., Campos, A., Ross, A. J., Rosell, A. Carnero, Yin, B., Yanny, B., Sanchez, C., Chang, C., Davis, C., Doux, C., Gruen, D., Rykoff, E. S., Huff, E. M., Sheldon, E., Tarsitano, F., Andrade-Oliveira, F., Bernstein, G. M., Giannini, G., Diehl, H. T., Huang, H., Harrison, I., Sevilla-Noarbe, I., Tutusaus, I., Elvin-Poole, J., McCullough, J., Zuntz, J., Blazek, J., DeRose, J., Cordero, J., Prat, J., Myles, J., Eckert, K., Bechtol, K., Herner, K., Secco, L. F., Gatti, M., Raveri, M., Kind, M. Carrasco, Becker, M. R., Troxel, M. A., Jarvis, M., MacCrann, N., Friedrich, O., Alves, O., Leget, P. -F., Chen, R., Rollins, R. P., Wechsler, R. H., Gruendl, R. A., Cawthon, R., Allam, S., Bridle, S. L., Pandey, S., Everett, S., Shin, T., Hartley, W. G., Fang, X., Zhang, Y., Aguena, M., Annis, J., Bacon, D., Bertin, E., Bocquet, S., Brooks, D., Carretero, J., Castander, F. J., da Costa, L. N., Pereira, M. E. S., De Vicente, J., Desai, S., Doel, P., Ferrero, I., Flaugher, B., Frieman, J., Garcia-Bellido, J., Gaztanaga, E., Gutierrez, G., Hinton, S. R., Hollowood, D. L., Honscheid, K., Huterer, D., James, D. J., Kuehn, K., Lahav, O., Lee, S., Marshall, J. L., Mena-Fernandez, J., Miquel, R., Muir, J., Paterno, M., Malagon, A. A. Plazas, Porredon, A., Romer, A. K., Samuroff, S., Sanchez, E., Cid, D. Sanchez, Smith, M., Soares-Santos, M., Suchyta, E., Swanson, M. E. C., Tarle, G., To, C., Weaverdyck, N., Weller, J., Wiseman, P., Yamamoto, M.
Formato:	Preprint
Publicado:	2024
Materias:	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
Acceso en línea:	Acceder al recurso
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_version_	1866929307351252992
author	Bigwood, L. Amon, A. Schneider, A. Salcido, J. McCarthy, I. G. Preston, C. Sanchez, D. Sijacki, D. Schaan, E. Ferraro, S. Battaglia, N. Chen, A. Dodelson, S. Roodman, A. Pieres, A. Ferte, A. Alarcon, A. Drlica-Wagner, A. Choi, A. Navarro-Alsina, A. Campos, A. Ross, A. J. Rosell, A. Carnero Yin, B. Yanny, B. Sanchez, C. Chang, C. Davis, C. Doux, C. Gruen, D. Rykoff, E. S. Huff, E. M. Sheldon, E. Tarsitano, F. Andrade-Oliveira, F. Bernstein, G. M. Giannini, G. Diehl, H. T. Huang, H. Harrison, I. Sevilla-Noarbe, I. Tutusaus, I. Elvin-Poole, J. McCullough, J. Zuntz, J. Blazek, J. DeRose, J. Cordero, J. Prat, J. Myles, J. Eckert, K. Bechtol, K. Herner, K. Secco, L. F. Gatti, M. Raveri, M. Kind, M. Carrasco Becker, M. R. Troxel, M. A. Jarvis, M. MacCrann, N. Friedrich, O. Alves, O. Leget, P. -F. Chen, R. Rollins, R. P. Wechsler, R. H. Gruendl, R. A. Cawthon, R. Allam, S. Bridle, S. L. Pandey, S. Everett, S. Shin, T. Hartley, W. G. Fang, X. Zhang, Y. Aguena, M. Annis, J. Bacon, D. Bertin, E. Bocquet, S. Brooks, D. Carretero, J. Castander, F. J. da Costa, L. N. Pereira, M. E. S. De Vicente, J. Desai, S. Doel, P. Ferrero, I. Flaugher, B. Frieman, J. Garcia-Bellido, J. Gaztanaga, E. Gutierrez, G. Hinton, S. R. Hollowood, D. L. Honscheid, K. Huterer, D. James, D. J. Kuehn, K. Lahav, O. Lee, S. Marshall, J. L. Mena-Fernandez, J. Miquel, R. Muir, J. Paterno, M. Malagon, A. A. Plazas Porredon, A. Romer, A. K. Samuroff, S. Sanchez, E. Cid, D. Sanchez Smith, M. Soares-Santos, M. Suchyta, E. Swanson, M. E. C. Tarle, G. To, C. Weaverdyck, N. Weller, J. Wiseman, P. Yamamoto, M.
author_facet	Bigwood, L. Amon, A. Schneider, A. Salcido, J. McCarthy, I. G. Preston, C. Sanchez, D. Sijacki, D. Schaan, E. Ferraro, S. Battaglia, N. Chen, A. Dodelson, S. Roodman, A. Pieres, A. Ferte, A. Alarcon, A. Drlica-Wagner, A. Choi, A. Navarro-Alsina, A. Campos, A. Ross, A. J. Rosell, A. Carnero Yin, B. Yanny, B. Sanchez, C. Chang, C. Davis, C. Doux, C. Gruen, D. Rykoff, E. S. Huff, E. M. Sheldon, E. Tarsitano, F. Andrade-Oliveira, F. Bernstein, G. M. Giannini, G. Diehl, H. T. Huang, H. Harrison, I. Sevilla-Noarbe, I. Tutusaus, I. Elvin-Poole, J. McCullough, J. Zuntz, J. Blazek, J. DeRose, J. Cordero, J. Prat, J. Myles, J. Eckert, K. Bechtol, K. Herner, K. Secco, L. F. Gatti, M. Raveri, M. Kind, M. Carrasco Becker, M. R. Troxel, M. A. Jarvis, M. MacCrann, N. Friedrich, O. Alves, O. Leget, P. -F. Chen, R. Rollins, R. P. Wechsler, R. H. Gruendl, R. A. Cawthon, R. Allam, S. Bridle, S. L. Pandey, S. Everett, S. Shin, T. Hartley, W. G. Fang, X. Zhang, Y. Aguena, M. Annis, J. Bacon, D. Bertin, E. Bocquet, S. Brooks, D. Carretero, J. Castander, F. J. da Costa, L. N. Pereira, M. E. S. De Vicente, J. Desai, S. Doel, P. Ferrero, I. Flaugher, B. Frieman, J. Garcia-Bellido, J. Gaztanaga, E. Gutierrez, G. Hinton, S. R. Hollowood, D. L. Honscheid, K. Huterer, D. James, D. J. Kuehn, K. Lahav, O. Lee, S. Marshall, J. L. Mena-Fernandez, J. Miquel, R. Muir, J. Paterno, M. Malagon, A. A. Plazas Porredon, A. Romer, A. K. Samuroff, S. Sanchez, E. Cid, D. Sanchez Smith, M. Soares-Santos, M. Suchyta, E. Swanson, M. E. C. Tarle, G. To, C. Weaverdyck, N. Weller, J. Wiseman, P. Yamamoto, M.
contents	Extracting precise cosmology from weak lensing surveys requires modelling the non-linear matter power spectrum, which is suppressed at small scales due to baryonic feedback processes. However, hydrodynamical galaxy formation simulations make widely varying predictions for the amplitude and extent of this effect. We use measurements of Dark Energy Survey Year 3 weak lensing (WL) and Atacama Cosmology Telescope DR5 kinematic Sunyaev-Zel'dovich (kSZ) to jointly constrain cosmological and astrophysical baryonic feedback parameters using a flexible analytical model, `baryonification'. First, using WL only, we compare the $S_8$ constraints using baryonification to a simulation-calibrated halo model, a simulation-based emulator model and the approach of discarding WL measurements on small angular scales. We find that model flexibility can shift the value of $S_8$ and degrade the uncertainty. The kSZ provides additional constraints on the astrophysical parameters and shifts $S_8$ to $S_8=0.823^{+0.019}_{-0.020}$, a higher value than attained using the WL-only analysis. We measure the suppression of the non-linear matter power spectrum using WL + kSZ and constrain a mean feedback scenario that is more extreme than the predictions from most hydrodynamical simulations. We constrain the baryon fractions and the gas mass fractions and find them to be generally lower than inferred from X-ray observations and simulation predictions. We conclude that the WL + kSZ measurements provide a new and complementary benchmark for building a coherent picture of the impact of gas around galaxies across observations.
format	Preprint
id	arxiv_https___arxiv_org_abs_2404_06098
institution	arXiv
publishDate	2024
record_format	arxiv
spellingShingle	Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback Bigwood, L. Amon, A. Schneider, A. Salcido, J. McCarthy, I. G. Preston, C. Sanchez, D. Sijacki, D. Schaan, E. Ferraro, S. Battaglia, N. Chen, A. Dodelson, S. Roodman, A. Pieres, A. Ferte, A. Alarcon, A. Drlica-Wagner, A. Choi, A. Navarro-Alsina, A. Campos, A. Ross, A. J. Rosell, A. Carnero Yin, B. Yanny, B. Sanchez, C. Chang, C. Davis, C. Doux, C. Gruen, D. Rykoff, E. S. Huff, E. M. Sheldon, E. Tarsitano, F. Andrade-Oliveira, F. Bernstein, G. M. Giannini, G. Diehl, H. T. Huang, H. Harrison, I. Sevilla-Noarbe, I. Tutusaus, I. Elvin-Poole, J. McCullough, J. Zuntz, J. Blazek, J. DeRose, J. Cordero, J. Prat, J. Myles, J. Eckert, K. Bechtol, K. Herner, K. Secco, L. F. Gatti, M. Raveri, M. Kind, M. Carrasco Becker, M. R. Troxel, M. A. Jarvis, M. MacCrann, N. Friedrich, O. Alves, O. Leget, P. -F. Chen, R. Rollins, R. P. Wechsler, R. H. Gruendl, R. A. Cawthon, R. Allam, S. Bridle, S. L. Pandey, S. Everett, S. Shin, T. Hartley, W. G. Fang, X. Zhang, Y. Aguena, M. Annis, J. Bacon, D. Bertin, E. Bocquet, S. Brooks, D. Carretero, J. Castander, F. J. da Costa, L. N. Pereira, M. E. S. De Vicente, J. Desai, S. Doel, P. Ferrero, I. Flaugher, B. Frieman, J. Garcia-Bellido, J. Gaztanaga, E. Gutierrez, G. Hinton, S. R. Hollowood, D. L. Honscheid, K. Huterer, D. James, D. J. Kuehn, K. Lahav, O. Lee, S. Marshall, J. L. Mena-Fernandez, J. Miquel, R. Muir, J. Paterno, M. Malagon, A. A. Plazas Porredon, A. Romer, A. K. Samuroff, S. Sanchez, E. Cid, D. Sanchez Smith, M. Soares-Santos, M. Suchyta, E. Swanson, M. E. C. Tarle, G. To, C. Weaverdyck, N. Weller, J. Wiseman, P. Yamamoto, M. Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies Extracting precise cosmology from weak lensing surveys requires modelling the non-linear matter power spectrum, which is suppressed at small scales due to baryonic feedback processes. However, hydrodynamical galaxy formation simulations make widely varying predictions for the amplitude and extent of this effect. We use measurements of Dark Energy Survey Year 3 weak lensing (WL) and Atacama Cosmology Telescope DR5 kinematic Sunyaev-Zel'dovich (kSZ) to jointly constrain cosmological and astrophysical baryonic feedback parameters using a flexible analytical model, `baryonification'. First, using WL only, we compare the $S_8$ constraints using baryonification to a simulation-calibrated halo model, a simulation-based emulator model and the approach of discarding WL measurements on small angular scales. We find that model flexibility can shift the value of $S_8$ and degrade the uncertainty. The kSZ provides additional constraints on the astrophysical parameters and shifts $S_8$ to $S_8=0.823^{+0.019}_{-0.020}$, a higher value than attained using the WL-only analysis. We measure the suppression of the non-linear matter power spectrum using WL + kSZ and constrain a mean feedback scenario that is more extreme than the predictions from most hydrodynamical simulations. We constrain the baryon fractions and the gas mass fractions and find them to be generally lower than inferred from X-ray observations and simulation predictions. We conclude that the WL + kSZ measurements provide a new and complementary benchmark for building a coherent picture of the impact of gas around galaxies across observations.
title	Weak lensing combined with the kinetic Sunyaev Zel'dovich effect: A study of baryonic feedback
topic	Cosmology and Nongalactic Astrophysics Astrophysics of Galaxies
url	https://arxiv.org/abs/2404.06098