Using the Sun to Measure the Primary Beam Response of the Canadian Hydrogen Intensity Mapping Experiment

We present a beam pattern measurement of the Canadian Hydrogen Intensity Mapping Experiment (CHIME) made using the Sun as a calibration source. As CHIME is a pure drift scan instrument, we rely on the seasonal North-South motion of the Sun to probe the beam at different elevations. This semiannual r...

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Veröffentlicht in:arXiv.org 2022-05
Hauptverfasser: Collaboration, CHIME, Amiri, Mandana, Bandura, Kevin, Boskovic, Anja, Cliche, Jean-François, Deng, Meiling, Dobbs, Matt, Mateus Fandino, eman, Simon, Halpern, Mark, Hill, Alex S, Hinshaw, Gary, Höfer, Carolin, Kania, Joseph, Landecker, T L, MacEachern, Joshua, Masui, Kiyoshi, Mena-Parra, Juan, Newburgh, Laura, Ordog, Anna, Pinsonneault-Marotte, Tristan, Polzin, Ava, Reda, Alex, Shaw, J Richard, Siegel, Seth R, Singh, Saurabh, Vanderlinde, Keith, Wang, Haochen, Willis, James S, Wulf, Dallas
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Sprache:eng
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Zusammenfassung:We present a beam pattern measurement of the Canadian Hydrogen Intensity Mapping Experiment (CHIME) made using the Sun as a calibration source. As CHIME is a pure drift scan instrument, we rely on the seasonal North-South motion of the Sun to probe the beam at different elevations. This semiannual range in elevation, combined with the radio brightness of the Sun, enables a beam measurement which spans ~7,200 square degrees on the sky without the need to move the telescope. We take advantage of observations made near solar minimum to minimize the impact of solar variability, which is observed to be
ISSN:2331-8422
DOI:10.48550/arxiv.2201.11822