Comparing Redundant and Sky-model-based Interferometric Calibration: A First Look with Phase II of the MWA

© 2018. The American Astronomical Society. All rights reserved.. Interferometric arrays seeking to measure the 21 cm signal from the epoch of reionization (EOR) must contend with overwhelmingly bright emission from foreground sources. Accurate recovery of the 21 cm signal will require precise calibr...

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Bibliographic Details
Main Authors: Li, W., Pober, J., Hazelton, B., Barry, N., Morales, M., Sullivan, I., Parsons, A., Ali, Z., Dillon, J., Beardsley, A., Bowman, J., Briggs, F., Byrne, R., Carroll, P., Crosse, B., Emrich, David, Ewall-Wice, A., Feng, L., Franzen, Thomas, Hewitt, J., Horsley, L., Jacobs, D., Johnston-Hollitt, M., Jordan, Christopher, Joseph, R., Kaplan, D., Kenney, David, Kim, H., Kittiwisit, P., Lanman, A., Line, J., McKinley, B., Mitchell, D., Murray, Steven, Neben, A., Offringa, A., Pallot, D., Paul, S., Pindor, B., Procopio, P., Rahimi, M., Riding, J., Sethi, S., Udaya Shankar, N., Steele, K., Subrahmanian, R., Tegmark, M., Thyagarajan, N., Tingay, Steven, Trott, Cathryn, Walker, M., Wayth, Randall, Webster, R., Williams, Andrew, Wu, C., Wyithe, S.
Format: Journal Article
Published: Institute of Physics Publishing 2018
Online Access:http://hdl.handle.net/20.500.11937/72500

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