Pregled bibliografske jedinice broj: 766585
Foreground simulations for the LOFAR-epoch of reionization experiment
Foreground simulations for the LOFAR-epoch of reionization experiment // Monthly notices of the Royal Astronomical Society, 389 (2008), 3; 1319-1335 doi:10.1111/j.1365-2966.2008.13634.x (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 766585 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Foreground simulations for the LOFAR-epoch of reionization experiment
Autori
Jelić, Vibor ; Zaroubi, S. ; Labropoulos, P. ; Thomas, R.M. ; Bernardi, G. ; Brentjens, M.A. ; de Bruyn, A.G. ; Ciardi, B. ; Harker, G. ; Koopmans, L.V.E. ; Pandey, V.N. ; Schaye, J. ; Yatawatta, S.
Izvornik
Monthly notices of the Royal Astronomical Society (0035-8711) 389
(2008), 3;
1319-1335
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
instrumentation: interferometers ; cosmology: observation ; cosmology: theory ; diffuse radiation ; radio continuum: general ; radio lines: general
Sažetak
Future high-redshift 21-cm experiments will suffer from a high degree of contamination, due both to astrophysical foregrounds and to non-astrophysical and instrumental effects. In order to reliably extract the cosmological signal from the observed data, it is essential to understand very well all data components and their influence on the extracted signal. Here we present simulated astrophysical foregrounds data cubes and discuss their possible statistical effects on the data. The foreground maps are produced assuming 5° × 5° windows that match those expected to be observed by the LOFAR epoch of reionization (EoR) key science project. We show that with the expected LOFAR-EoR sky and receiver noise levels, which amount to ~52mK at 150 MHz after 400 h of total observing time, a simple polynomial fit allows a statistical reconstruction of the signal. We also show that the polynomial fitting will work for maps with realistic yet idealized instrument response, i.e. a response that includes only a uniform uv coverage as a function of frequency and ignores many other uncertainties. Polarized Galactic synchrotron maps that include internal polarization and a number of Faraday screens along the line of sight are also simulated. The importance of these stems from the fact that the LOFAR instrument, in common with all current interferometric EoR experiments, has an instrumentally polarized response.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
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