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Autor:
Carilli{1, C. L., Thyagarajan{1}, N., Kent{2}, J., Nikolic{2}, B., Gale-Sides{2}, K., Kern{3}, N. S., Bernardi{4, G., Mesinger{7}, A., Matika{5}, S., Observatory, the HERA TEAM {1}{National Radio Astronomy, Socorro, USA, edu, ccarilli@nrao., ORCID, Group, 0000-0001-6647-3861} {2}{Astrophysics, Laboratory, Cavendish, Avenue, JJ Thomson, Astronomy, UK} {3}{Department of, California, University of, Berkeley, di Radioastronomia, CA} {4}{INAF-Istituto, Bologna, Physics, Italy} {5}{Department of, Electronics, University, Rhodes, Grahamstown, Observatory, South Africa} {6}{The South African Radio Astronomy, Street, 2 Fir, Park, Black River, Observatory, Superiore, South Africa} {7}{Scuola Normale, Pisa, 56126, PI, Italy}
We analyze data from the Hydrogen Epoch of Reionization Array. This is the third in a series of papers on the closure phase delay-spectrum technique designed to detect the HI 21cm emission from cosmic reionization. We present the details of the data
Externí odkaz:
http://arxiv.org/abs/2002.07692
