학술논문

Direct Optimal Mapping Image Power Spectrum and its Window Functions
Document Type
Working Paper
Author
Xu, ZhileiKim, HonggeunHewitt, Jacqueline N.Chen, Kai-FengKern, Nicholas S.Rath, EleanorByrne, RubyGorce, AdéliePascua, RobertMartinot, Zachary E.Dillon, Joshua S.Hazelton, Bryna J.Liu, AdrianMorales, Miguel F.Abdurashidova, ZaraAdams, TyroneAguirre, James E.Alexander, PaulAli, Zaki S.Baartman, RushelleBalfour, YangaBeardsley, Adam P.Bernardi, GianniBillings, Tashalee S.Bowman, Judd D.Bradley, Richard F.Bull, PhilipBurba, JacobCarey, StevenCarilli, Chris L.Cheng, CarinaDeBoer, David R.Acedo, Eloy de LeraDexter, MattEksteen, NicoEly, JohnEwall-Wice, AaronFagnoni, NicolasFritz, RandallFurlanetto, Steven R.Gale-Sides, KingsleyGlendenning, BrianGorthi, DeepthiGreig, BradleyGrobbelaar, JasperHalday, ZiyaadHickish, JackJacobs, Daniel C.Julius, AustinKariseb, MacCalvinKerrigan, JoshuaKittiwisit, PiyanatKohn, Saul A.Kolopanis, MatthewLanman, AdamLa Plante, PaulLoots, AnitaMacMahon, David Harold EdwardMalan, LourenceMalgas, CresshimMalgas, KeithMarero, BradleyMesinger, AndreiMolewa, MathakaneMosiane, TshegofalangMurray, Steven G.Neben, Abraham R.Nikolic, BojanNuwegeld, HansParsons, Aaron R.Patra, NipanjanaPieterse, SamanthaRazavi-Ghods, NimaRobnett, JamesRosie, KathrynSims, PeterSmith, CraigSwarts, HiltonThyagarajan, Nithyanandanvan Wyngaarden, PieterWilliams, Peter K. G.Zheng, Haoxuan
Source
Subject
Astrophysics - Instrumentation and Methods for Astrophysics
Astrophysics - Cosmology and Nongalactic Astrophysics
Language
Abstract
The key to detecting neutral hydrogen during the epoch of reionization (EoR) is to separate the cosmological signal from the dominating foreground radiation. We developed direct optimal mapping (DOM) to map interferometric visibilities; it contains only linear operations, with full knowledge of point spread functions from visibilities to images. Here, we demonstrate a fast Fourier transform-based image power spectrum and its window functions computed from the DOM images. We use noiseless simulation, based on the Hydrogen Epoch of Reionization Array Phase I configuration, to study the image power spectrum properties. The window functions show $<10^{-11}$ of the integrated power leaks from the foreground-dominated region into the EoR window; the 2D and 1D power spectra also verify the separation between the foregrounds and the EoR.
Comment: Published in ApJ