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Nevertheless, the 21cm radiation we would like to map out is literally buried under foregrounds which are 3-5 orders of magnitude more intense. Before starting to do any cosmology, we need to face the challenge of cleaning the intensity maps. This is the reason why I am now in CosmoStat. We are now tackling this problem, doing blind source separation of the different components contaminating our 21cm intensity maps, using sparse representations of the signals, optimising it for the 21cm IM and assessing what are the limitations on the science we are able to do with this probe.
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Papers共 26 篇Author StatisticsCo-AuthorSimilar Experts
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MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 2 (2023): 3517-3531
Physics of the Dark Universe (2023): 101151-101151
Steven Cunnington,Laura Wolz,Philip Bull,Isabella P. Carucci,Keith Grainge,Melis O. Irfan,Yichao Li,Alkistis Pourtsidou, Mario G. Santos,Marta Spinelli,Jingying Wang, MeerKLASS Collaborat
Monthly Notices of the Royal Astronomical Societyno. 2 (2023): 2453-2477
Monthly Notices of the Royal Astronomical Societyno. 1 (2021): 208-227
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETYno. 1 (2020): 304-319
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