| dc.contributor.author | Bonaldi, A. | |
| dc.contributor.author | Hartley, P. | |
| dc.contributor.author | Braun, R. | |
| dc.contributor.author | Purser, S. | |
| dc.contributor.author | Acharya, A. | |
| dc.contributor.author | Ahn, K. | |
| dc.contributor.author | Aparicio Resco, M. | |
| dc.contributor.author | Bait, O. | |
| dc.contributor.author | Bianco, M. | |
| dc.contributor.author | Chakraborty, A. | |
| dc.contributor.author | Chapman, E. | |
| dc.contributor.author | Chatterjee, S. | |
| dc.contributor.author | Chege, K. | |
| dc.contributor.author | Chen, H. | |
| dc.contributor.author | Chen, X. | |
| dc.contributor.author | Cruz Rodríguez, Marcos | |
| dc.contributor.author | Ruiz Granda, Miguel | |
| dc.contributor.author | Herranz Muñoz, Diego | |
| dc.contributor.author | Remazeilles, Mathieu | |
| dc.contributor.author | Vielva Martínez, Patricio | |
| dc.contributor.other | Universidad de Cantabria | es_ES |
| dc.date.accessioned | 2025-12-03T12:34:01Z | |
| dc.date.available | 2025-12-03T12:34:01Z | |
| dc.date.issued | 2025-10 | |
| dc.identifier.issn | 0035-8711 | |
| dc.identifier.issn | 1365-2966 | |
| dc.identifier.other | PID2019-110610RB-C21 | es_ES |
| dc.identifier.other | PID2022-139223OB-C21; PID2022-140670NA-I00 ; CEX2021-001131-S ; PID2021-123930OB-C21 ; TED2021-130231B-I00 ; PRE2021-100660 ; PID2023-147883NB-C21 | es_ES |
| dc.identifier.uri | https://hdl.handle.net/10902/38387 | |
| dc.description.abstract | We present and analyse the results of the Science Data Challenge 3a (SDC3a, https://sdc3.skao.int/challenges/foregrounds), an epoch of reionization (EoR) foreground-removal exercise organized by the Square Kilometre Array Observatory (SKAO) on SKA simulated data. The challenge ran for 8 months, from 2023 March to October. Participants were provided with realistic simulations of SKA-Low data between 106 and 196 MHz, including foreground contamination from extragalactic and Galactic emission, instrumental, and systematic effects. They were asked to deliver cylindrical power spectra of the EoR signal, cleaned from all corruptions, and the corresponding confidence levels. Here, we describe the approaches taken by the 17 teams that completed the challenge, and we assess their performance using different metrics. The challenge results provide a positive outlook on the capabilities of current foreground-mitigation approaches to recover the faint EoR signal from SKA-Low observations. The median error committed in the EoR power spectrum recovery is below the true signal for seven teams, although in some cases, there are some significant outliers. The smallest residual overall is 4.2+20-4.2 × 10-4 K2h-3cMpc3 across all considered scales and frequencies. The estimation of confidence levels provided by the teams is overall less accurate, with the true error being typically underestimated, sometimes very significantly. The most accurate error bars account for 60 ± 20 per cent of the true errors committed. The challenge results provide a means for all teams to understand and improve their performance. This challenge indicates that the comparison between independent pipelines could be a powerful tool to assess residual biases and improve error estimation. | es_ES |
| dc.description.sponsorship | LVM, SS, JG, JM, TW, MGM, LD, and IL acknowledge financial support from the grant CEX2021-001131-S funded by MCIU/AEI/10.13039/501100011033 and from the grant PID2021-123930OB-C21 funded by MCIU/AEI/10.13039/501100011033 and by ERDF/EU. LVM, JG, TW, and MGM acknowledge financial support from the coordination of the participation in SKA-SPAIN, funded by the Ministry of Science, Innovation and Universities (MCIU). LVM, SS, JG, LD, and IL acknowledge financial support from the grant TED2021-130231B-I00 funded by MCIU/AEI/10.13039/501100011033 and by the European Union NextGenerationEU/PRTR. IL acknowledges financial support from the grant PRE2021-100660 funded by MCIU/AEI/10.13039/501100011033 and by ESF+. JM acknowledges financialsupport from grant PID2023-147883NB-C21, funded by MCIU/AEI/ 10.13039/501100011033 and by ERDF/EU. MRG, DH, MC, MR, and PV have been supported by MCIN/AEI/10.13039/501100011033, project refs. PID2019-110610RB-C21PID2022-139223OB-C21 (funded also by European Union NextGenerationEU/PRTR), and from Universidad de Cantabria and Consejería de Educación, ´ Formación Profesional y Universidades del Gobierno de Cantabria, via the "Actividad estructural para el desarrollo de la investigación del Instituto de Física de Cantabria". MRG acknowledges financial support from the Formación del Profesorado Universitario program of the Spanish Ministerio de Ciencia, Innovación y Universidades. MRG and DH thank the Spanish Agencia Estatal de Investigación (AEI, MICIU) for the financial support provided under the project with reference PID2022-140670NA-I00. | es_ES |
| dc.format.extent | 28 p. | es_ES |
| dc.language.iso | eng | es_ES |
| dc.publisher | Oxford University Press | es_ES |
| dc.rights | Attribution 4.0 International | es_ES |
| dc.rights.uri | http://creativecommons.org/licenses/by/4.0/ | * |
| dc.source | Monthly Notices of the Royal Astronomical Society, 2025, 543(2), 1092-1119 | es_ES |
| dc.title | Square kilometre array science data challenge 3a: foreground removal for an EoR experiment | es_ES |
| dc.type | info:eu-repo/semantics/article | es_ES |
| dc.relation.publisherVersion | https://doi.org/10.1093/mnras/staf1466 | es_ES |
| dc.rights.accessRights | openAccess | es_ES |
| dc.identifier.DOI | 10.1093/mnras/staf1466 | |
| dc.type.version | publishedVersion | es_ES |