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dc.contributor.authorFonseca, Jose
dc.contributor.authorMaartens, Roy
dc.contributor.authorSantos, Mario G.
dc.date.accessioned2018-09-04T11:48:24Z
dc.date.available2018-09-04T11:48:24Z
dc.date.issued2018
dc.identifier.citationFonseca, J. et al. (2018). Synergies between intensity maps of hydrogen lines. Monthly Notices of the Royal Astronomical Society, 479: 3490en_US
dc.identifier.issn0035-8711
dc.identifier.urihttp://dx.doi.org/10.1093/mnras/sty1702
dc.identifier.urihttp://hdl.handle.net/10566/4004
dc.description.abstractWe study synergies between Hi 21cm and Hα intensity map observations, focusing on SKA1- like and SPHEREx-like surveys. We forecast how well such a combination can measure features in the angular power spectrum on the largest scales, that arise from primordial non- Gaussianity and from general relativistic effects. For the first time we consider Doppler, Sachs-Wolfe and integrated SW effects separately. We confirm that the single-tracer surveys on their own cannot detect general relativistic effects and can constrain the non-Gaussianity parameter fNL only slightly better than Planck. Using the multi-tracer technique, constraints on fNL can be pushed down to ~ 1. Amongst the general relativistic effects, the Doppler term is detectable with the multi-tracer. The Sachs-Wolfe terms and the integrated SW effect are still not detectable.en_US
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.rightsThis is the pre-print version of the article published online at: http://dx.doi.org/10.1093/mnras/sty1702
dc.subjectCosmologyen_US
dc.subjectLarge-scale structure of the Universeen_US
dc.subjectCosmological parametersen_US
dc.subjectMiscellaneous.en_US
dc.titleSynergies between intensity maps of hydrogen linesen_US
dc.typeArticleen_US
dc.privacy.showsubmitterFALSE
dc.status.ispeerreviewedTRUE
dc.description.accreditationISI


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