_version_ 1866909833140109312
author Kumwembe, Alexus Annika
Lamman, Claire
Eisenstein, Daniel
Aguilar, Jessica Nicole
Ahlen, Steven
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cuceu, Andrei
de la Macorra, Axel
Dey, Biprateep
Doel, Peter
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztanaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Ishak, Mustapha
Jimenez, Jorge
Joyce, Dick
Kehoe, Robert
Kisner, Theodore
Lahav, Ofer
Landriau, Martin
Manera, Marc
Miquel, Ramon
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Perez-Rafols, Ignasi
Prada, Francisco
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Seo, Hee-Jong
Silber, Joseph Harry
Sprayberry, David
Tarle, Gregory
Weaver, Benjamin Alan
author_facet Kumwembe, Alexus Annika
Lamman, Claire
Eisenstein, Daniel
Aguilar, Jessica Nicole
Ahlen, Steven
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cuceu, Andrei
de la Macorra, Axel
Dey, Biprateep
Doel, Peter
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztanaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Ishak, Mustapha
Jimenez, Jorge
Joyce, Dick
Kehoe, Robert
Kisner, Theodore
Lahav, Ofer
Landriau, Martin
Manera, Marc
Miquel, Ramon
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Perez-Rafols, Ignasi
Prada, Francisco
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Seo, Hee-Jong
Silber, Joseph Harry
Sprayberry, David
Tarle, Gregory
Weaver, Benjamin Alan
contents We demonstrate that measurements of the gravitational tidal field made with spectroscopic redshifts can be improved with information from imaging surveys. The average orientation of small groups of galaxies, or "multiplets" is correlated with large-scale structure and is used to measure the direction of tidal forces. Previously, multiplet intrinsic alignment has been measured in DESI using galaxies that have spectroscopic redshifts. The DESI Legacy Imaging catalog can be used to supplement multiplet catalogs. Our findings show that galaxy positions from the imaging catalog produce a measurement similar to the measurements made with only spectroscopic data. This demonstrates that imaging can improve our signal-to-noise ratio for multiplet alignment in DESI.
format Preprint
id arxiv_https___arxiv_org_abs_2510_08353
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Enhancing Multiplet Alignment Measurements with Imaging
Kumwembe, Alexus Annika
Lamman, Claire
Eisenstein, Daniel
Aguilar, Jessica Nicole
Ahlen, Steven
Bianchi, Davide
Brooks, David
Claybaugh, Todd
Cuceu, Andrei
de la Macorra, Axel
Dey, Biprateep
Doel, Peter
Font-Ribera, Andreu
Forero-Romero, Jaime E.
Gaztanaga, Enrique
Gontcho, Satya Gontcho A
Gutierrez, Gaston
Ishak, Mustapha
Jimenez, Jorge
Joyce, Dick
Kehoe, Robert
Kisner, Theodore
Lahav, Ofer
Landriau, Martin
Manera, Marc
Miquel, Ramon
Nadathur, Seshadri
Palanque-Delabrouille, Nathalie
Perez-Rafols, Ignasi
Prada, Francisco
Rossi, Graziano
Sanchez, Eusebio
Schlegel, David
Seo, Hee-Jong
Silber, Joseph Harry
Sprayberry, David
Tarle, Gregory
Weaver, Benjamin Alan
Cosmology and Nongalactic Astrophysics
We demonstrate that measurements of the gravitational tidal field made with spectroscopic redshifts can be improved with information from imaging surveys. The average orientation of small groups of galaxies, or "multiplets" is correlated with large-scale structure and is used to measure the direction of tidal forces. Previously, multiplet intrinsic alignment has been measured in DESI using galaxies that have spectroscopic redshifts. The DESI Legacy Imaging catalog can be used to supplement multiplet catalogs. Our findings show that galaxy positions from the imaging catalog produce a measurement similar to the measurements made with only spectroscopic data. This demonstrates that imaging can improve our signal-to-noise ratio for multiplet alignment in DESI.
title Enhancing Multiplet Alignment Measurements with Imaging
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2510.08353