Pregled bibliografske jedinice broj: 1140801
Comparing foreground removal techniques for recovery of the LOFAR-EoR 21 cm power spectrum
Comparing foreground removal techniques for recovery of the LOFAR-EoR 21 cm power spectrum // Monthly notices of the Royal Astronomical Society, 500 (2021), 2; 2264-2277 doi:10.1093/mnras/staa3446 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 1140801 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Comparing foreground removal techniques for recovery
of the LOFAR-EoR 21 cm power spectrum
Autori
Hothi, Ian ; Chapman, Emma ; Pritchard, Jonathan R ; Mertens, F G ; Koopmans, L V E ; Ciardi, B ; Gehlot, B K ; Ghara, R ; Ghosh, A ; Giri, S K ; Iliev, I T ; Jelić, Vibor ; Zaroubi, S
Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 500
(2021), 2;
2264-2277
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
cosmology: theory - dark ages ; reionization ; first stars ; cosmology: observations ; techniques: interferometric ; methods: data analysis ; statistical
Sažetak
We compare various foreground removal techniques that are being utilised to remove bright foregrounds in various experiments aiming to detect the redshifted 21cm signal of neutral hydrogen from the Epoch of Reionization. In this work, we test the performance of removal techniques (FastICA, GMCA, and GPR) on 10 nights of LOFAR data and investigate the possibility of recovering the latest upper limit on the 21cm signal. Interestingly, we find that GMCA and FastICA reproduce the most recent 2σ upper limit of Δ221< (73)2 mK2 at k=0.075 hcMpc−1, which resulted from the application of GPR. We also find that FastICA and GMCA begin to deviate from the noise-limit at \textit{; ; ; k}; ; ; - scales larger than ∼0.1 hcMpc−1. We then replicate the data via simulations to see the source of FastICA and GMCA's limitations, by testing them against various instrumental effects. We find that no single instrumental effect, such as primary beam effects or mode-mixing, can explain the poorer recovery by FastICA and GMCA at larger \textit{; ; ; k}; ; ; -scales. We then test scale- independence of FastICA and GMCA, and find that lower \textit{; ; ; k}; ; ; -scales can be modelled by a smaller number of independent components. For larger scales (k≳0.1 hcMpc−1), more independent components are needed to fit the foregrounds. We conclude that, the current usage of GPR by the LOFAR collaboration is the appropriate removal technique. It is both robust and less prone to overfitting, with future improvements to GPR's fitting optimisation to yield deeper limits.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-IP-2018-01-2889 - Razumijevanje zračenja na niskim radio frekvencijama: ususret novoj generaciji radio teleskopa (LowFreqCRO) (Jelić, Vibor, HRZZ - 2018-01) ( CroRIS)
Ustanove:
Institut "Ruđer Bošković", Zagreb
Profili:
Vibor Jelić
(autor)
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus