학술논문
Validating the Galaxy and Quasar Catalog-Level Blinding Scheme for the DESI 2024 analysis
Document Type
Working Paper
Author
Andrade, U.; Mena-Fernández, J.; Awan, H.; Ross, A. J.; Brieden, S.; Pan, J.; de Mattia, A.; Aguilar, J.; Ahlen, S.; Alves, O.; Brooks, D.; Buckley-Geer, E.; Chaussidon, E.; Claybaugh, T.; Cole, S.; de la Macorra, A.; Dey, Arjun; Doel, P.; Fanning, K.; Forero-Romero, J. E.; Gaztañaga, E.; Gil-Marín, H.; Gontcho, S. Gontcho A; Guy, J.; Hahn, C.; Hanif, M. M. S; Honscheid, K.; Howlett, C.; Huterer, D.; Juneau, S.; Kremin, A.; Landriau, M.; Guillou, L. Le; Levi, M. E.; Manera, M.; Martini, P.; Meisner, A.; Miquel, R.; Moustakas, J.; Mueller, E.; Muñoz-Gutiérrez, A.; Myers, A. D.; Nadathur, S.; Newman, J. A.; Nie, J.; Niz, G.; Palanque-Delabrouille, N.; Percival, W. J.; Pinon, M.; Poppett, C.; Prada, F.; Rashkovetskyi, M.; Rezaie, M.; Rossi, G.; Sanchez, E.; Schlegel, D.; Schubnell, M.; Seo, H.; Sprayberry, D.; Tarlé, G.; Vargas-Magaña, M.; Verde, L.; Weaver, B. A.
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Subject
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Abstract
In the era of precision cosmology, ensuring the integrity of data analysis through blinding techniques is paramount -- a challenge particularly relevant for the Dark Energy Spectroscopic Instrument (DESI). DESI represents a monumental effort to map the cosmic web, with the goal to measure the redshifts of tens of millions of galaxies and quasars. Given the data volume and the impact of the findings, the potential for confirmation bias poses a significant challenge. To address this, we implement and validate a comprehensive blind analysis strategy for DESI Data Release 1 (DR1), tailored to the specific observables DESI is most sensitive to: Baryonic Acoustic Oscillations (BAO), Redshift-Space Distortion (RSD) and primordial non-Gaussianities (PNG). We carry out the blinding at the catalog level, implementing shifts in the redshifts of the observed galaxies to blind for BAO and RSD signals and weights to blind for PNG through a scale-dependent bias. We validate the blinding technique on mocks, as well as on data by applying a second blinding layer to perform a battery of sanity checks. We find that the blinding strategy alters the data vector in a controlled way such that the BAO and RSD analysis choices do not need any modification before and after unblinding. The successful validation of the blinding strategy paves the way for the unblinded DESI DR1 analysis, alongside future blind analyses with DESI and other surveys.
Comment: Supporting publication of "DESI 2024 II: Sample definitions, characteristics, and two-point clustering statistics", "DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars", and "DESI 2024 V: Analysis of the full shape of two-point clustering statistics from galaxies and quasars". (v2 - update DESI references)
Comment: Supporting publication of "DESI 2024 II: Sample definitions, characteristics, and two-point clustering statistics", "DESI 2024 III: Baryon Acoustic Oscillations from Galaxies and Quasars", and "DESI 2024 V: Analysis of the full shape of two-point clustering statistics from galaxies and quasars". (v2 - update DESI references)