The BINGO Project IV: Simulations for mission performance assessment and preliminary component separation steps

The large-scale distribution of neutral hydrogen (HI) in the Universe is luminous through its 21 cm emission. The goal of the Baryon Acoustic Oscillations from Integrated Neutral Gas Observations -- BINGO -- radio telescope is to detect baryon acoustic oscillations (BAOs) at radio frequencies throug...

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Bibliographic Details
Published in:arXiv.org 2021-10
Main Authors: Liccardo, Vincenzo, de Mericia, Eduardo J, Wuensche, Carlos A, Abdalla, Elcio, Abdalla, Filipe B, Barosi, Luciano, Brito, Francisco A, Queiroz, Amilcar, Villela, Thyrso, Peel, Michael W, Wang, Bin, Costa, Andre A, Ferreira, Elisa G M, nazier, Karin S F, Novaes, Camila P, Santos, Larissa, dos Santos, Marcelo V, Remazeilles, Mathieu, Zhang, Jiajun, Dickinson, Clive, Harper, Stuart, Landim, Ricardo G, Marins, Alessandro, Vieira, Frederico
Format: Article
Language:English
Subjects:
Acoustic mapping
Astronomical maps
Baryons
Design optimization
Field of view
Focal plane
Multipoles
Neutral gases
Oscillations
Performance assessment
Radio frequency
Radio telescopes
Red shift
Separation
Simulation
Telescopes
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Summary:The large-scale distribution of neutral hydrogen (HI) in the Universe is luminous through its 21 cm emission. The goal of the Baryon Acoustic Oscillations from Integrated Neutral Gas Observations -- BINGO -- radio telescope is to detect baryon acoustic oscillations (BAOs) at radio frequencies through 21 cm intensity mapping (IM). The telescope will span the redshift range 0.127 \(< z
ISSN:2331-8422
DOI:10.48550/arxiv.2107.01636