Progress in Single Dish 21 cm Intensity Mapping

Autores/as

  • Christopher Joseph Anderson University of Wisconsin Madison

DOI:

https://doi.org/10.17307/wsc.v1i1.180

Palabras clave:

Hydrogen, 21 cm, Intensity Mapping

Resumen

Progress has been made in finalizing the design of a 7 element array to be installed on the Green Bank Telescope in the 700 to 900 MHz frequency range.  The new array should increase HI intensity mapping speed by a factor of 4.  The design review for the array is scheduled for October 19.  At the same time, 21 cm intensity mapping data collected from the Parkes radio telescope has been analyzed.  We have detected HI signal in cross-correlation with the 2df Galaxy Survey.

Biografía del autor/a

Christopher Joseph Anderson, University of Wisconsin Madison

Graduate student in the Physics department.

Citas

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son, K., Seljak, U., Stebbins, A., Steffen, J. H., Stoughton, C., Timbie,

P. T., Vallinotto, A., and Teche, C. 21-cm Intensity Mapping. In astro2010: The Astronomy and Astrophysics Decadal Survey (2009), vol. 2010 of ArXiv Astrophysics e-prints.

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Publicado

2017-01-01

Cómo citar

Anderson, C. J. (2017). Progress in Single Dish 21 cm Intensity Mapping. Proceedings of the Wisconsin Space Conference, 1(1). https://doi.org/10.17307/wsc.v1i1.180

Número

2016: Beyond the Horizon

Sección

Physics and Engineering

Licencia

Creative Commons License
This work is licensed under a Creative Commons Attribution-NonCommercial 4.0 International License.