Calibration and Beam-Mapping Techniques for the Tianlai Pathfinder Dish Array

Authors

DOI:

https://doi.org/10.17307/wsc.v1i1.308

Keywords:

cosmology, HI, intensity mapping, radio interferometry

Abstract

Hydrogen intensity mapping is a promising technique to measuring large-scale structure.  By detecting the integrated emission of the 21cm HI signal from many galaxies simultaneously, astronomers can survey larger volumes of the universe than ever before.  However, systematics related to foreground subtraction, variable antenna beam patterns, and calibration must be overcome before maps can be made of the 21cm signal.  The Tianlai Pathfinder array, a first-generation hydrogen intensity mapping experiment, is being constructed in order to practice and demonstrate our ability to overcome these challenges.  We demonstrate two methods, delay-delay rate filtering and point source calibration, in order to understand the systematics of the Tianlai instrument.  The methods used here will be used to help demonstrate the feasibility of full-scale hydrogen intensity mapping experiments, while contributing to the experimental toolset used for such experiments.

Author Biography

Trevor Oxholm, University of Wisconsin-Madison

Doctoral Candidate

Department of Physics

University of Wisconsin-Madison

References

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Published

2020-03-16

How to Cite

Oxholm, T. (2020). Calibration and Beam-Mapping Techniques for the Tianlai Pathfinder Dish Array. Proceedings of the Wisconsin Space Conference, 1(1). https://doi.org/10.17307/wsc.v1i1.308

Issue

Section

Astronomy and Cosmology