Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4
We present a measurement of the cross-correlation between the MagLim galaxies selected from the Dark Energy Survey (DES) first three years of observations (Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology Telescope (ACT) Data Release 4 (DR4), reconstructed over $\sim 436$...
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| creator | Marques, G. A Madhavacheril, M. S Darwish, O Shaikh, S Aguena, M Alves, O Avila, S Bacon, D Baxter, E. J Bechtol, K Becker, M. R Bertin, E Blazek, J Bond, J. Richard Brooks, D Cai, H Calabrese, E Rosell, A. Carnero Carretero, M. Carrasco Kind J Cawthon, R Crocce, M da Costa, L. N Pereira, M. E. S De Vicente, J Desai, S Diehl, H. T Doel, P Doux, C Drlica-Wagner, A Dunkley, J Elvin-Poole, J Everett, S Ferraro, Simone Ferrero, I Flaugher, B Fosalba, P García-Bellido, J Gatti, M Giannini, G Gluscevic, V Gruen, D Gruendl, R. A Gutierrez, G Harrison, I Hill, J. Colin Hinton, S. R Hollowood, D. L Honscheid, K Huterer, D Jeffrey, N Kim, J Kuehn, K Lahav, O Lemos, P Lima, M Huffenberger, K. M MacCrann, N Marshall, J. L Mena-Fernández, J Miquel, R Mohr, J. J Moodley, K Muir, J Naess, S Nati, F Page, L. A Palmese, A Malagón, A. A. Plazas Porredon, A Prat, J Qu, F. J Raveri, M Ross, A. J Rykoff, E. S Farren, G. S Samuroff, S Sanchez, E Schubnell, M Sevilla-Noarbe, I Sheldon, E Sherwin, B. D Sifón, C Smith, M Spergel, D. N Staggs, S. T Suchyta, E Tarle, G To, C Van Engelen, A Weaverdyck, N Weller, J Wenzl, L Wiseman, P Wollack, E. J Yanny, B |
| description | We present a measurement of the cross-correlation between the MagLim galaxies
selected from the Dark Energy Survey (DES) first three years of observations
(Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology
Telescope (ACT) Data Release 4 (DR4), reconstructed over $\sim 436$ sq.deg. of
the sky. Our galaxy sample, which covers $\sim 4143$ sq.deg., is divided into
six redshift bins spanning the redshift range of $0.20 |
| doi_str_mv | 10.48550/arxiv.2306.17268 |
| format | Article |
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selected from the Dark Energy Survey (DES) first three years of observations
(Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology
Telescope (ACT) Data Release 4 (DR4), reconstructed over $\sim 436$ sq.deg. of
the sky. Our galaxy sample, which covers $\sim 4143$ sq.deg., is divided into
six redshift bins spanning the redshift range of $0.20<z<1.05$. We adopt a
blinding procedure until passing all consistency and systematics tests. After
imposing scale cuts for the cross-power spectrum measurement, we reject the
null hypothesis of no correlation at 9.1\sigma. We constrain cosmological
parameters from a joint analysis of galaxy and CMB lensing-galaxy power spectra
considering a flat \LCDM model, marginalized over 23 astrophysical and
systematic nuisance parameters. We find the clustering amplitude $S_8\equiv
\sigma_8 (\Omega_m/0.3)^{0.5} = 0.75^{+0.04}_{-0.05}$. In addition, we
constrain the linear growth of cosmic structure as a function of redshift. Our
results are consistent with recent DES Y3 analyses and suggest a preference for
a lower $S_8$ compared to results from measurements of CMB anisotropies by the
Planck satellite, although at a mild level ($< 2 \sigma$) of statistical
significance.</description><identifier>DOI: 10.48550/arxiv.2306.17268</identifier><language>eng</language><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><creationdate>2023-06</creationdate><rights>http://arxiv.org/licenses/nonexclusive-distrib/1.0</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>228,230,780,885</link.rule.ids><linktorsrc>$$Uhttps://arxiv.org/abs/2306.17268$$EView_record_in_Cornell_University$$FView_record_in_$$GCornell_University$$Hfree_for_read</linktorsrc><backlink>$$Uhttps://doi.org/10.48550/arXiv.2306.17268$$DView paper in arXiv$$Hfree_for_read</backlink></links><search><creatorcontrib>Marques, G. A</creatorcontrib><creatorcontrib>Madhavacheril, M. 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A</creatorcontrib><creatorcontrib>Palmese, A</creatorcontrib><creatorcontrib>Malagón, A. A. Plazas</creatorcontrib><creatorcontrib>Porredon, A</creatorcontrib><creatorcontrib>Prat, J</creatorcontrib><creatorcontrib>Qu, F. J</creatorcontrib><creatorcontrib>Raveri, M</creatorcontrib><creatorcontrib>Ross, A. J</creatorcontrib><creatorcontrib>Rykoff, E. S</creatorcontrib><creatorcontrib>Farren, G. S</creatorcontrib><creatorcontrib>Samuroff, S</creatorcontrib><creatorcontrib>Sanchez, E</creatorcontrib><creatorcontrib>Schubnell, M</creatorcontrib><creatorcontrib>Sevilla-Noarbe, I</creatorcontrib><creatorcontrib>Sheldon, E</creatorcontrib><creatorcontrib>Sherwin, B. D</creatorcontrib><creatorcontrib>Sifón, C</creatorcontrib><creatorcontrib>Smith, M</creatorcontrib><creatorcontrib>Spergel, D. N</creatorcontrib><creatorcontrib>Staggs, S. T</creatorcontrib><creatorcontrib>Suchyta, E</creatorcontrib><creatorcontrib>Tarle, G</creatorcontrib><creatorcontrib>To, C</creatorcontrib><creatorcontrib>Van Engelen, A</creatorcontrib><creatorcontrib>Weaverdyck, N</creatorcontrib><creatorcontrib>Weller, J</creatorcontrib><creatorcontrib>Wenzl, L</creatorcontrib><creatorcontrib>Wiseman, P</creatorcontrib><creatorcontrib>Wollack, E. J</creatorcontrib><creatorcontrib>Yanny, B</creatorcontrib><title>Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4</title><description>We present a measurement of the cross-correlation between the MagLim galaxies
selected from the Dark Energy Survey (DES) first three years of observations
(Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology
Telescope (ACT) Data Release 4 (DR4), reconstructed over $\sim 436$ sq.deg. of
the sky. Our galaxy sample, which covers $\sim 4143$ sq.deg., is divided into
six redshift bins spanning the redshift range of $0.20<z<1.05$. We adopt a
blinding procedure until passing all consistency and systematics tests. After
imposing scale cuts for the cross-power spectrum measurement, we reject the
null hypothesis of no correlation at 9.1\sigma. We constrain cosmological
parameters from a joint analysis of galaxy and CMB lensing-galaxy power spectra
considering a flat \LCDM model, marginalized over 23 astrophysical and
systematic nuisance parameters. We find the clustering amplitude $S_8\equiv
\sigma_8 (\Omega_m/0.3)^{0.5} = 0.75^{+0.04}_{-0.05}$. In addition, we
constrain the linear growth of cosmic structure as a function of redshift. Our
results are consistent with recent DES Y3 analyses and suggest a preference for
a lower $S_8$ compared to results from measurements of CMB anisotropies by the
Planck satellite, although at a mild level ($< 2 \sigma$) of statistical
significance.</description><subject>Physics - Cosmology and Nongalactic Astrophysics</subject><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>GOX</sourceid><recordid>eNqFzr0OgjAYheEuDka9ACe_GwBBfmTVgnFxURYHQ76QUpq0lLSNwt0b0d3pLO9JHkLWYeDHWZIEWzSDePq7KEj9cL9Lszl5UG2VlpqLGiXUurPOoOichcZoBa5l4LTS3GDfjqAbyIubd4-Ao8RBMAsv4VqglyNI1lnR8e_vQEvIr_GSzBqUlq1-uyCbU1HSszdBqt4IhWasPqBqAkX_izcbyD_5</recordid><startdate>20230629</startdate><enddate>20230629</enddate><creator>Marques, G. A</creator><creator>Madhavacheril, M. S</creator><creator>Darwish, O</creator><creator>Shaikh, S</creator><creator>Aguena, M</creator><creator>Alves, O</creator><creator>Avila, S</creator><creator>Bacon, D</creator><creator>Baxter, E. J</creator><creator>Bechtol, K</creator><creator>Becker, M. R</creator><creator>Bertin, E</creator><creator>Blazek, J</creator><creator>Bond, J. Richard</creator><creator>Brooks, D</creator><creator>Cai, H</creator><creator>Calabrese, E</creator><creator>Rosell, A. Carnero</creator><creator>Carretero, M. Carrasco Kind J</creator><creator>Cawthon, R</creator><creator>Crocce, M</creator><creator>da Costa, L. N</creator><creator>Pereira, M. E. S</creator><creator>De Vicente, J</creator><creator>Desai, S</creator><creator>Diehl, H. T</creator><creator>Doel, P</creator><creator>Doux, C</creator><creator>Drlica-Wagner, A</creator><creator>Dunkley, J</creator><creator>Elvin-Poole, J</creator><creator>Everett, S</creator><creator>Ferraro, Simone</creator><creator>Ferrero, I</creator><creator>Flaugher, B</creator><creator>Fosalba, P</creator><creator>García-Bellido, J</creator><creator>Gatti, M</creator><creator>Giannini, G</creator><creator>Gluscevic, V</creator><creator>Gruen, D</creator><creator>Gruendl, R. A</creator><creator>Gutierrez, G</creator><creator>Harrison, I</creator><creator>Hill, J. Colin</creator><creator>Hinton, S. R</creator><creator>Hollowood, D. L</creator><creator>Honscheid, K</creator><creator>Huterer, D</creator><creator>Jeffrey, N</creator><creator>Kim, J</creator><creator>Kuehn, K</creator><creator>Lahav, O</creator><creator>Lemos, P</creator><creator>Lima, M</creator><creator>Huffenberger, K. M</creator><creator>MacCrann, N</creator><creator>Marshall, J. L</creator><creator>Mena-Fernández, J</creator><creator>Miquel, R</creator><creator>Mohr, J. J</creator><creator>Moodley, K</creator><creator>Muir, J</creator><creator>Naess, S</creator><creator>Nati, F</creator><creator>Page, L. A</creator><creator>Palmese, A</creator><creator>Malagón, A. A. Plazas</creator><creator>Porredon, A</creator><creator>Prat, J</creator><creator>Qu, F. J</creator><creator>Raveri, M</creator><creator>Ross, A. J</creator><creator>Rykoff, E. S</creator><creator>Farren, G. S</creator><creator>Samuroff, S</creator><creator>Sanchez, E</creator><creator>Schubnell, M</creator><creator>Sevilla-Noarbe, I</creator><creator>Sheldon, E</creator><creator>Sherwin, B. D</creator><creator>Sifón, C</creator><creator>Smith, M</creator><creator>Spergel, D. N</creator><creator>Staggs, S. T</creator><creator>Suchyta, E</creator><creator>Tarle, G</creator><creator>To, C</creator><creator>Van Engelen, A</creator><creator>Weaverdyck, N</creator><creator>Weller, J</creator><creator>Wenzl, L</creator><creator>Wiseman, P</creator><creator>Wollack, E. J</creator><creator>Yanny, B</creator><scope>GOX</scope></search><sort><creationdate>20230629</creationdate><title>Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4</title><author>Marques, G. A ; Madhavacheril, M. S ; Darwish, O ; Shaikh, S ; Aguena, M ; Alves, O ; Avila, S ; Bacon, D ; Baxter, E. J ; Bechtol, K ; Becker, M. R ; Bertin, E ; Blazek, J ; Bond, J. 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D ; Sifón, C ; Smith, M ; Spergel, D. N ; Staggs, S. T ; Suchyta, E ; Tarle, G ; To, C ; Van Engelen, A ; Weaverdyck, N ; Weller, J ; Wenzl, L ; Wiseman, P ; Wollack, E. J ; Yanny, B</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-arxiv_primary_2306_172683</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Physics - Cosmology and Nongalactic Astrophysics</topic><toplevel>online_resources</toplevel><creatorcontrib>Marques, G. A</creatorcontrib><creatorcontrib>Madhavacheril, M. S</creatorcontrib><creatorcontrib>Darwish, O</creatorcontrib><creatorcontrib>Shaikh, S</creatorcontrib><creatorcontrib>Aguena, M</creatorcontrib><creatorcontrib>Alves, O</creatorcontrib><creatorcontrib>Avila, S</creatorcontrib><creatorcontrib>Bacon, D</creatorcontrib><creatorcontrib>Baxter, E. J</creatorcontrib><creatorcontrib>Bechtol, K</creatorcontrib><creatorcontrib>Becker, M. 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T</creatorcontrib><creatorcontrib>Doel, P</creatorcontrib><creatorcontrib>Doux, C</creatorcontrib><creatorcontrib>Drlica-Wagner, A</creatorcontrib><creatorcontrib>Dunkley, J</creatorcontrib><creatorcontrib>Elvin-Poole, J</creatorcontrib><creatorcontrib>Everett, S</creatorcontrib><creatorcontrib>Ferraro, Simone</creatorcontrib><creatorcontrib>Ferrero, I</creatorcontrib><creatorcontrib>Flaugher, B</creatorcontrib><creatorcontrib>Fosalba, P</creatorcontrib><creatorcontrib>García-Bellido, J</creatorcontrib><creatorcontrib>Gatti, M</creatorcontrib><creatorcontrib>Giannini, G</creatorcontrib><creatorcontrib>Gluscevic, V</creatorcontrib><creatorcontrib>Gruen, D</creatorcontrib><creatorcontrib>Gruendl, R. A</creatorcontrib><creatorcontrib>Gutierrez, G</creatorcontrib><creatorcontrib>Harrison, I</creatorcontrib><creatorcontrib>Hill, J. Colin</creatorcontrib><creatorcontrib>Hinton, S. R</creatorcontrib><creatorcontrib>Hollowood, D. L</creatorcontrib><creatorcontrib>Honscheid, K</creatorcontrib><creatorcontrib>Huterer, D</creatorcontrib><creatorcontrib>Jeffrey, N</creatorcontrib><creatorcontrib>Kim, J</creatorcontrib><creatorcontrib>Kuehn, K</creatorcontrib><creatorcontrib>Lahav, O</creatorcontrib><creatorcontrib>Lemos, P</creatorcontrib><creatorcontrib>Lima, M</creatorcontrib><creatorcontrib>Huffenberger, K. M</creatorcontrib><creatorcontrib>MacCrann, N</creatorcontrib><creatorcontrib>Marshall, J. L</creatorcontrib><creatorcontrib>Mena-Fernández, J</creatorcontrib><creatorcontrib>Miquel, R</creatorcontrib><creatorcontrib>Mohr, J. J</creatorcontrib><creatorcontrib>Moodley, K</creatorcontrib><creatorcontrib>Muir, J</creatorcontrib><creatorcontrib>Naess, S</creatorcontrib><creatorcontrib>Nati, F</creatorcontrib><creatorcontrib>Page, L. A</creatorcontrib><creatorcontrib>Palmese, A</creatorcontrib><creatorcontrib>Malagón, A. A. Plazas</creatorcontrib><creatorcontrib>Porredon, A</creatorcontrib><creatorcontrib>Prat, J</creatorcontrib><creatorcontrib>Qu, F. J</creatorcontrib><creatorcontrib>Raveri, M</creatorcontrib><creatorcontrib>Ross, A. J</creatorcontrib><creatorcontrib>Rykoff, E. S</creatorcontrib><creatorcontrib>Farren, G. S</creatorcontrib><creatorcontrib>Samuroff, S</creatorcontrib><creatorcontrib>Sanchez, E</creatorcontrib><creatorcontrib>Schubnell, M</creatorcontrib><creatorcontrib>Sevilla-Noarbe, I</creatorcontrib><creatorcontrib>Sheldon, E</creatorcontrib><creatorcontrib>Sherwin, B. D</creatorcontrib><creatorcontrib>Sifón, C</creatorcontrib><creatorcontrib>Smith, M</creatorcontrib><creatorcontrib>Spergel, D. N</creatorcontrib><creatorcontrib>Staggs, S. T</creatorcontrib><creatorcontrib>Suchyta, E</creatorcontrib><creatorcontrib>Tarle, G</creatorcontrib><creatorcontrib>To, C</creatorcontrib><creatorcontrib>Van Engelen, A</creatorcontrib><creatorcontrib>Weaverdyck, N</creatorcontrib><creatorcontrib>Weller, J</creatorcontrib><creatorcontrib>Wenzl, L</creatorcontrib><creatorcontrib>Wiseman, P</creatorcontrib><creatorcontrib>Wollack, E. J</creatorcontrib><creatorcontrib>Yanny, B</creatorcontrib><collection>arXiv.org</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext_linktorsrc</fulltext></delivery><addata><au>Marques, G. A</au><au>Madhavacheril, M. S</au><au>Darwish, O</au><au>Shaikh, S</au><au>Aguena, M</au><au>Alves, O</au><au>Avila, S</au><au>Bacon, D</au><au>Baxter, E. J</au><au>Bechtol, K</au><au>Becker, M. R</au><au>Bertin, E</au><au>Blazek, J</au><au>Bond, J. Richard</au><au>Brooks, D</au><au>Cai, H</au><au>Calabrese, E</au><au>Rosell, A. Carnero</au><au>Carretero, M. Carrasco Kind J</au><au>Cawthon, R</au><au>Crocce, M</au><au>da Costa, L. N</au><au>Pereira, M. E. S</au><au>De Vicente, J</au><au>Desai, S</au><au>Diehl, H. T</au><au>Doel, P</au><au>Doux, C</au><au>Drlica-Wagner, A</au><au>Dunkley, J</au><au>Elvin-Poole, J</au><au>Everett, S</au><au>Ferraro, Simone</au><au>Ferrero, I</au><au>Flaugher, B</au><au>Fosalba, P</au><au>García-Bellido, J</au><au>Gatti, M</au><au>Giannini, G</au><au>Gluscevic, V</au><au>Gruen, D</au><au>Gruendl, R. A</au><au>Gutierrez, G</au><au>Harrison, I</au><au>Hill, J. Colin</au><au>Hinton, S. R</au><au>Hollowood, D. L</au><au>Honscheid, K</au><au>Huterer, D</au><au>Jeffrey, N</au><au>Kim, J</au><au>Kuehn, K</au><au>Lahav, O</au><au>Lemos, P</au><au>Lima, M</au><au>Huffenberger, K. M</au><au>MacCrann, N</au><au>Marshall, J. L</au><au>Mena-Fernández, J</au><au>Miquel, R</au><au>Mohr, J. J</au><au>Moodley, K</au><au>Muir, J</au><au>Naess, S</au><au>Nati, F</au><au>Page, L. A</au><au>Palmese, A</au><au>Malagón, A. A. Plazas</au><au>Porredon, A</au><au>Prat, J</au><au>Qu, F. J</au><au>Raveri, M</au><au>Ross, A. J</au><au>Rykoff, E. S</au><au>Farren, G. S</au><au>Samuroff, S</au><au>Sanchez, E</au><au>Schubnell, M</au><au>Sevilla-Noarbe, I</au><au>Sheldon, E</au><au>Sherwin, B. D</au><au>Sifón, C</au><au>Smith, M</au><au>Spergel, D. N</au><au>Staggs, S. T</au><au>Suchyta, E</au><au>Tarle, G</au><au>To, C</au><au>Van Engelen, A</au><au>Weaverdyck, N</au><au>Weller, J</au><au>Wenzl, L</au><au>Wiseman, P</au><au>Wollack, E. J</au><au>Yanny, B</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4</atitle><date>2023-06-29</date><risdate>2023</risdate><abstract>We present a measurement of the cross-correlation between the MagLim galaxies
selected from the Dark Energy Survey (DES) first three years of observations
(Y3) and cosmic microwave background (CMB) lensing from the Atacama Cosmology
Telescope (ACT) Data Release 4 (DR4), reconstructed over $\sim 436$ sq.deg. of
the sky. Our galaxy sample, which covers $\sim 4143$ sq.deg., is divided into
six redshift bins spanning the redshift range of $0.20<z<1.05$. We adopt a
blinding procedure until passing all consistency and systematics tests. After
imposing scale cuts for the cross-power spectrum measurement, we reject the
null hypothesis of no correlation at 9.1\sigma. We constrain cosmological
parameters from a joint analysis of galaxy and CMB lensing-galaxy power spectra
considering a flat \LCDM model, marginalized over 23 astrophysical and
systematic nuisance parameters. We find the clustering amplitude $S_8\equiv
\sigma_8 (\Omega_m/0.3)^{0.5} = 0.75^{+0.04}_{-0.05}$. In addition, we
constrain the linear growth of cosmic structure as a function of redshift. Our
results are consistent with recent DES Y3 analyses and suggest a preference for
a lower $S_8$ compared to results from measurements of CMB anisotropies by the
Planck satellite, although at a mild level ($< 2 \sigma$) of statistical
significance.</abstract><doi>10.48550/arxiv.2306.17268</doi><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext_linktorsrc |
| identifier | DOI: 10.48550/arxiv.2306.17268 |
| ispartof | |
| issn | |
| language | eng |
| recordid | cdi_arxiv_primary_2306_17268 |
| source | arXiv.org |
| subjects | Physics - Cosmology and Nongalactic Astrophysics |
| title | Cosmological constraints from the tomography of DES-Y3 galaxies with CMB lensing from ACT DR4 |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T16%3A13%3A01IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-arxiv_GOX&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Cosmological%20constraints%20from%20the%20tomography%20of%20DES-Y3%20galaxies%20with%20CMB%20lensing%20from%20ACT%20DR4&rft.au=Marques,%20G.%20A&rft.date=2023-06-29&rft_id=info:doi/10.48550/arxiv.2306.17268&rft_dat=%3Carxiv_GOX%3E2306_17268%3C/arxiv_GOX%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_id=info:pmid/&rfr_iscdi=true |