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Main Authors: Lange, Johannes U., Wells, Alexandra, Hearin, Andrew, Beltz-Mohrmann, Gillian, Leauthaud, Alexie, Heydenreich, Sven, Blake, Chris, Aguilar, Jessica Nicole, Ahlen, Steven, Anand, Abhijeet, Bianchi, Davide, Brooks, David, Castander, Francisco Javier, Claybaugh, Todd, Cole, Shaun, Cuceu, Andrei, Dawson, Kyle, de la Macorra, Axel, Dey, Biprateep, Doel, Peter, Elliott, Ann, Emas, Ni Putu Audita Placida, Ferraro, Simone, Font-Ribera, Andreu, Forero-Romero, Jaime E., Garcia-Quintero, Cristhian, Gaztañaga, Enrique, Gontcho, Satya Gontcho A, Gutierrez, Gaston, Guy, Julien, Honscheid, Klaus, Huterer, Dragan, Ishak, Mustapha, Joudaki, Shahab, Joyce, Dick, Kehoe, Robert, Kirkby, David, Kisner, Theodore, Kremin, Anthony, Krolewski, Alex, Lahav, Ofer, Lamman, Claire, Landriau, Martin, Guillou, Laurent Le, Levi, Michael, Manera, Marc, Martini, Paul, Meisner, Aaron, Miquel, Ramon, Moustakas, John, Mueller, Eva-Maria, Nadathur, Seshadri, Newman, Jeffrey A., Niz, Gustavo, Palanque-Delabrouille, Nathalie, Percival, Will, Poppett, Claire, Porredon, Anna, Prada, Francisco, Pérez-Ràfols, Ignasi, Robertson, Amy, Rossi, Graziano, Ruggeri, Rossana, Sanchez, Eusebio, Saulder, Christoph, Schlegel, David, Schubnell, Michael, Semenaite, Agne, Seo, Hee-Jong, Silber, Joseph Harry, Sprayberry, David, Sun, Zechang, Tarlé, Gregory, Magana, Mariana Vargas, Weaver, Benjamin Alan, Wechsler, Risa, Zarrouk, Pauline, Zhou, Rongpu, Zou, Hu
Format: Preprint
Published: 2025
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Online Access:https://arxiv.org/abs/2512.15962
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author Lange, Johannes U.
Wells, Alexandra
Hearin, Andrew
Beltz-Mohrmann, Gillian
Leauthaud, Alexie
Heydenreich, Sven
Blake, Chris
Aguilar, Jessica Nicole
Ahlen, Steven
Anand, Abhijeet
Bianchi, Davide
Brooks, David
Castander, Francisco Javier
Claybaugh, Todd
Cole, Shaun
Cuceu, Andrei
Dawson, Kyle
de la Macorra, Axel
Dey, Biprateep
Doel, Peter
Elliott, Ann
Emas, Ni Putu Audita Placida
Ferraro, Simone
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Garcia-Quintero, Cristhian
Gaztañaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Guy, Julien
Honscheid, Klaus
Huterer, Dragan
Ishak, Mustapha
Joudaki, Shahab
Joyce, Dick
Kehoe, Robert
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Krolewski, Alex
Lahav, Ofer
Lamman, Claire
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Manera, Marc
Martini, Paul
Meisner, Aaron
Miquel, Ramon
Moustakas, John
Mueller, Eva-Maria
Nadathur, Seshadri
Newman, Jeffrey A.
Niz, Gustavo
Palanque-Delabrouille, Nathalie
Percival, Will
Poppett, Claire
Porredon, Anna
Prada, Francisco
Pérez-Ràfols, Ignasi
Robertson, Amy
Rossi, Graziano
Ruggeri, Rossana
Sanchez, Eusebio
Saulder, Christoph
Schlegel, David
Schubnell, Michael
Semenaite, Agne
Seo, Hee-Jong
Silber, Joseph Harry
Sprayberry, David
Sun, Zechang
Tarlé, Gregory
Magana, Mariana Vargas
Weaver, Benjamin Alan
Wechsler, Risa
Zarrouk, Pauline
Zhou, Rongpu
Zou, Hu
author_facet Lange, Johannes U.
Wells, Alexandra
Hearin, Andrew
Beltz-Mohrmann, Gillian
Leauthaud, Alexie
Heydenreich, Sven
Blake, Chris
Aguilar, Jessica Nicole
Ahlen, Steven
Anand, Abhijeet
Bianchi, Davide
Brooks, David
Castander, Francisco Javier
Claybaugh, Todd
Cole, Shaun
Cuceu, Andrei
Dawson, Kyle
de la Macorra, Axel
Dey, Biprateep
Doel, Peter
Elliott, Ann
Emas, Ni Putu Audita Placida
Ferraro, Simone
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Garcia-Quintero, Cristhian
Gaztañaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Guy, Julien
Honscheid, Klaus
Huterer, Dragan
Ishak, Mustapha
Joudaki, Shahab
Joyce, Dick
Kehoe, Robert
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Krolewski, Alex
Lahav, Ofer
Lamman, Claire
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Manera, Marc
Martini, Paul
Meisner, Aaron
Miquel, Ramon
Moustakas, John
Mueller, Eva-Maria
Nadathur, Seshadri
Newman, Jeffrey A.
Niz, Gustavo
Palanque-Delabrouille, Nathalie
Percival, Will
Poppett, Claire
Porredon, Anna
Prada, Francisco
Pérez-Ràfols, Ignasi
Robertson, Amy
Rossi, Graziano
Ruggeri, Rossana
Sanchez, Eusebio
Saulder, Christoph
Schlegel, David
Schubnell, Michael
Semenaite, Agne
Seo, Hee-Jong
Silber, Joseph Harry
Sprayberry, David
Sun, Zechang
Tarlé, Gregory
Magana, Mariana Vargas
Weaver, Benjamin Alan
Wechsler, Risa
Zarrouk, Pauline
Zhou, Rongpu
Zou, Hu
contents We present constraints on cosmic structure growth from the analysis of galaxy clustering and galaxy-galaxy lensing with galaxies from the Dark Energy Spectroscopic Instrument (DESI) Data Release 1. We analyze four samples drawn from the Bright Galaxy Survey (BGS) and the Luminous Red Galaxy (LRG) target classes. Projected galaxy clustering measurements from DESI are supplemented with lensing measurements from the Dark Energy Survey (DES), the Kilo-Degree Survey (KiDS), and the Hyper Suprime-Cam (HSC) survey around the same targets. Our method relies on a simulation-based modeling framework using the AbacusSummit simulations and a complex halo occupation distribution model that incorporates assembly bias. We analyze scales down to $0.4 \, h^{-1} \, \mathrm{Mpc}$ for clustering and $2.5 \, h^{-1} \, \mathrm{Mpc}$ for lensing, leading to stringent constraints on $S_8 = σ_8 \sqrt{Ω_\mathrm{m} / 0.3}$ and $Ω_\mathrm{m}$ when fixing other cosmological parameters to those preferred by the CMB. We find $S_8 = 0.794 \pm 0.023$ and $Ω_\mathrm{m} = 0.295 \pm 0.012$ when using lensing measurements from DES and KiDS. Similarly, for HSC, we find $S_8 = 0.793 \pm 0.017$ and $Ω_\mathrm{m} = 0.303 \pm 0.010$ when assuming the best-fit photometric redshift offset suggested by the HSC collaboration. Overall, our results are in good agreement with other results in the literature while continuing to highlight the constraining power of non-linear scales.
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publishDate 2025
record_format arxiv
spellingShingle Cosmological Constraints from Full-Scale Clustering and Galaxy-Galaxy Lensing with DESI DR1
Lange, Johannes U.
Wells, Alexandra
Hearin, Andrew
Beltz-Mohrmann, Gillian
Leauthaud, Alexie
Heydenreich, Sven
Blake, Chris
Aguilar, Jessica Nicole
Ahlen, Steven
Anand, Abhijeet
Bianchi, Davide
Brooks, David
Castander, Francisco Javier
Claybaugh, Todd
Cole, Shaun
Cuceu, Andrei
Dawson, Kyle
de la Macorra, Axel
Dey, Biprateep
Doel, Peter
Elliott, Ann
Emas, Ni Putu Audita Placida
Ferraro, Simone
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Garcia-Quintero, Cristhian
Gaztañaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Guy, Julien
Honscheid, Klaus
Huterer, Dragan
Ishak, Mustapha
Joudaki, Shahab
Joyce, Dick
Kehoe, Robert
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Krolewski, Alex
Lahav, Ofer
Lamman, Claire
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Manera, Marc
Martini, Paul
Meisner, Aaron
Miquel, Ramon
Moustakas, John
Mueller, Eva-Maria
Nadathur, Seshadri
Newman, Jeffrey A.
Niz, Gustavo
Palanque-Delabrouille, Nathalie
Percival, Will
Poppett, Claire
Porredon, Anna
Prada, Francisco
Pérez-Ràfols, Ignasi
Robertson, Amy
Rossi, Graziano
Ruggeri, Rossana
Sanchez, Eusebio
Saulder, Christoph
Schlegel, David
Schubnell, Michael
Semenaite, Agne
Seo, Hee-Jong
Silber, Joseph Harry
Sprayberry, David
Sun, Zechang
Tarlé, Gregory
Magana, Mariana Vargas
Weaver, Benjamin Alan
Wechsler, Risa
Zarrouk, Pauline
Zhou, Rongpu
Zou, Hu
Cosmology and Nongalactic Astrophysics
We present constraints on cosmic structure growth from the analysis of galaxy clustering and galaxy-galaxy lensing with galaxies from the Dark Energy Spectroscopic Instrument (DESI) Data Release 1. We analyze four samples drawn from the Bright Galaxy Survey (BGS) and the Luminous Red Galaxy (LRG) target classes. Projected galaxy clustering measurements from DESI are supplemented with lensing measurements from the Dark Energy Survey (DES), the Kilo-Degree Survey (KiDS), and the Hyper Suprime-Cam (HSC) survey around the same targets. Our method relies on a simulation-based modeling framework using the AbacusSummit simulations and a complex halo occupation distribution model that incorporates assembly bias. We analyze scales down to $0.4 \, h^{-1} \, \mathrm{Mpc}$ for clustering and $2.5 \, h^{-1} \, \mathrm{Mpc}$ for lensing, leading to stringent constraints on $S_8 = σ_8 \sqrt{Ω_\mathrm{m} / 0.3}$ and $Ω_\mathrm{m}$ when fixing other cosmological parameters to those preferred by the CMB. We find $S_8 = 0.794 \pm 0.023$ and $Ω_\mathrm{m} = 0.295 \pm 0.012$ when using lensing measurements from DES and KiDS. Similarly, for HSC, we find $S_8 = 0.793 \pm 0.017$ and $Ω_\mathrm{m} = 0.303 \pm 0.010$ when assuming the best-fit photometric redshift offset suggested by the HSC collaboration. Overall, our results are in good agreement with other results in the literature while continuing to highlight the constraining power of non-linear scales.
title Cosmological Constraints from Full-Scale Clustering and Galaxy-Galaxy Lensing with DESI DR1
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2512.15962