Effects of model incompleteness on the drift-scan calibration of radio telescopes

@article{Gehlot2021EffectsOM,
  title={Effects of model incompleteness on the drift-scan calibration of radio telescopes},
  author={B K Gehlot and Daniel C. Jacobs and Judd D. Bowman and Nivedita Mahesh and S. Murray and Matthew Kolopanis and Adam P. Beardsley and Zara Abdurashidova and James E. Aguirre and Paul Alexander and Zaki S. Ali and Yanga Balfour and Gianni Bernardi and Tashalee S. Billings and Richard F. Bradley and Philip Bull and Jacob Burba and Steve H. Carey and Christopher L. Carilli and Carina Cheng and David R. DeBoer and Matt Dexter and Eloy de Lera Acedo and Joshua S. Dillon and J. A. Ely and Aaron Ewall-Wice and Nicolas Fagnoni and Randall Fritz and Steven R. Furlanetto and Kingsley Gale-Sides and B. E. Glendenning and Deepthi Gorthi and Bradley Greig and Jasper Grobbelaar and Ziyaad Halday and Bryna J. Hazelton and Jacqueline N. Hewitt and Jack Hickish and Austin Julius and Nicholas S. Kern and Joshua Kerrigan and Piyanat Kittiwisit and Saul A. Kohn and Adam E. Lanman and Paul La Plante and Telalo Lekalake and David Lewis and Adrian Liu and Yin-Zhe Ma and David Macmahon and Lourence Malan and Cresshim Malgas and M. D. J. Maree and Zachary E. Martinot and Eunice Matsetela and Andrei Mesinger and Mathakane Molewa and Ra{\'u}l A. Monsalve and Miguel F. Morales and Tshegofalang Mosiane and Abraham R. Neben and Bojan Nikoli{\'c} and Aaron Parsons and Robert Pascua and Nipanjana Patra and Samantha Pieterse and Jonathan C. Pober and Nima Razavi-Ghods and Jon Ringuette and James Robnett and Kathryn Rosie and Mario G Santos and Peter H Sims and Craig H. Smith and Angelo Syce and Max Tegmark and Nithyanandan Thyagarajan and Peter K. G. Williams and Haoxuan Zheng School of Earth and Space Exploration and Arizona State University and Department of Physics Astronomy and University of Southern California and Berkeley and Dep. of Physics and Astronomy and University of Pennsylvania and CA Department of Astrophysics and University of Cambridge and Cambridge and South African astronomical Observatory and Electronics and R. S. de Jong Liverpool John Moores University and Inaf Istituto di Radioastronomia and Italy. and National Radio Astronomy Observatory and Charlottesville and Queen Mary University London and Brown University and Socorro and Mit Kavli Institute for Astrophysics and Space Research and Mit and Los P Angeles and School of Cosmic Physics and University of Melbourne and University of Washington and Seattle and E. J. Schreier Sternberg Astronomical Institute and School of Chemistry and Physics and University of KwaZulu-Natal and McGill Space institute and M. Zemcov Cardiff University and Scuola Normale Superiore and University of Western Cape and Cape Town and Center for Computational Astrophysics and Harvard and Smithsonian and American Astronomical Society and Washington and Dc and Facultad de Ingenierı́a and Universidad de Concepcion and Chile.},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2021}
}
  • B. Gehlot, D. Jacobs, Chile.
  • Published 25 April 2021
  • Physics
  • Monthly Notices of the Royal Astronomical Society
Precision calibration poses challenges to experiments probing the redshifted 21-cm signal of neutral hydrogen from the Cosmic Dawn and Epoch of Reionization (z ∼ 30–6). In both interferometric and global signal experiments, systematic calibration is the leading source of error. Though many aspects of calibration have been studied, the overlap between the two types of instruments has received less attention. We investigate the sky based calibration of total power measurements with a HERA dish… 

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