_version_ 1866916649287811072
author Saulder, Christoph
Song, Yong-Seon
Oh, Minji
Zheng, Yi
Ross, Ashley J.
Zhou, Rongpu
Newman, Jeffrey A.
Chuang, Chia-Hsun
Aguilar, Jessica Nicole
Ahlen, Steven
Blum, Robert
Brooks, David
Claybaugh, Todd
de la Macorra, Axel
Dey, Biprateep
Ding, Zhejie
Doel, Peter
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Juneau, Stephanie
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Lambert, Andrew
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Meisner, Aaron
Mueller, Eva-Maria
Muñoz-Gutiérrez, Andrea
Niz, Gustavo
Prada, Francisco
Rezaie, Mehdi
Rossi, Graziano
Sanchez, Eusebio
Schubnell, Michael
Silber, Joseph Harry
Sprayberry, David
Tarlé, Gregory
Valdes, Francisco
Weaver, Benjamin Alan
Zou, Hu
author_facet Saulder, Christoph
Song, Yong-Seon
Oh, Minji
Zheng, Yi
Ross, Ashley J.
Zhou, Rongpu
Newman, Jeffrey A.
Chuang, Chia-Hsun
Aguilar, Jessica Nicole
Ahlen, Steven
Blum, Robert
Brooks, David
Claybaugh, Todd
de la Macorra, Axel
Dey, Biprateep
Ding, Zhejie
Doel, Peter
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Juneau, Stephanie
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Lambert, Andrew
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Meisner, Aaron
Mueller, Eva-Maria
Muñoz-Gutiérrez, Andrea
Niz, Gustavo
Prada, Francisco
Rezaie, Mehdi
Rossi, Graziano
Sanchez, Eusebio
Schubnell, Michael
Silber, Joseph Harry
Sprayberry, David
Tarlé, Gregory
Valdes, Francisco
Weaver, Benjamin Alan
Zou, Hu
contents Context.The Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Survey DR9 (DR9 hereafter), with its extensive dataset of galaxy locations and photometric redshifts, presents an opportunity to study baryon acoustic oscillations (BAOs) in the region covered by the ongoing spectroscopic survey with DESI. Aims. We aim to investigate differences between different parts of the DR9 footprint. Furthermore, we want to measure the BAO scale for luminous red galaxies within them. Our selected redshift range of 0.6 to 0.8 corresponds to the bin in which a tension between DESI Y1 and eBOSS was found. Methods. We calculated the anisotropic two-point correlation function in a modified binning scheme to detect the BAOs in DR9 data. We then used template fits based on simulations to measure the BAO scale in the imaging data. Results. Our analysis reveals the expected correlation function shape in most of the footprint areas, showing a BAO scale consistent with Planck's observations. Aside from identified mask-related data issues in the southern region of the South Galactic Cap, we find a notable variance between the different footprints. Conclusions. We find that this variance is consistent with the difference between the DESI Y1 and eBOSS data, and it supports the argument that that tension is caused by sample variance. Additionally, we also uncovered systematic biases not previously accounted for in photometric BAO studies. We emphasize the necessity of adjusting for the systematic shift in the BAO scale associated with typical photometric redshift uncertainties to ensure accurate measurements.
format Preprint
id arxiv_https___arxiv_org_abs_2501_10759
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
Saulder, Christoph
Song, Yong-Seon
Oh, Minji
Zheng, Yi
Ross, Ashley J.
Zhou, Rongpu
Newman, Jeffrey A.
Chuang, Chia-Hsun
Aguilar, Jessica Nicole
Ahlen, Steven
Blum, Robert
Brooks, David
Claybaugh, Todd
de la Macorra, Axel
Dey, Biprateep
Ding, Zhejie
Doel, Peter
Forero-Romero, Jaime E.
Gaztañaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Juneau, Stephanie
Kirkby, David
Kisner, Theodore
Kremin, Anthony
Lambert, Andrew
Landriau, Martin
Guillou, Laurent Le
Levi, Michael
Meisner, Aaron
Mueller, Eva-Maria
Muñoz-Gutiérrez, Andrea
Niz, Gustavo
Prada, Francisco
Rezaie, Mehdi
Rossi, Graziano
Sanchez, Eusebio
Schubnell, Michael
Silber, Joseph Harry
Sprayberry, David
Tarlé, Gregory
Valdes, Francisco
Weaver, Benjamin Alan
Zou, Hu
Cosmology and Nongalactic Astrophysics
Context.The Dark Energy Spectroscopic Instrument (DESI) Legacy Imaging Survey DR9 (DR9 hereafter), with its extensive dataset of galaxy locations and photometric redshifts, presents an opportunity to study baryon acoustic oscillations (BAOs) in the region covered by the ongoing spectroscopic survey with DESI. Aims. We aim to investigate differences between different parts of the DR9 footprint. Furthermore, we want to measure the BAO scale for luminous red galaxies within them. Our selected redshift range of 0.6 to 0.8 corresponds to the bin in which a tension between DESI Y1 and eBOSS was found. Methods. We calculated the anisotropic two-point correlation function in a modified binning scheme to detect the BAOs in DR9 data. We then used template fits based on simulations to measure the BAO scale in the imaging data. Results. Our analysis reveals the expected correlation function shape in most of the footprint areas, showing a BAO scale consistent with Planck's observations. Aside from identified mask-related data issues in the southern region of the South Galactic Cap, we find a notable variance between the different footprints. Conclusions. We find that this variance is consistent with the difference between the DESI Y1 and eBOSS data, and it supports the argument that that tension is caused by sample variance. Additionally, we also uncovered systematic biases not previously accounted for in photometric BAO studies. We emphasize the necessity of adjusting for the systematic shift in the BAO scale associated with typical photometric redshift uncertainties to ensure accurate measurements.
title Studying baryon acoustic oscillations using photometric redshifts from the DESI Legacy Imaging survey DR9
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2501.10759