Gregory J. Madsen, Ph.D.

Affiliations: 
2004 University of Wisconsin, Madison, Madison, WI 
Area:
Astronomy and Astrophysics
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"Gregory Madsen"
Mean distance: 5420.8
 

Parents

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Ronald J. Reynolds grad student 2004 UW Madison
 (An exploration of the heterogeneous nature of the warm ionized medium in the Galaxy.)
Bryan M. Gaensler post-doc 2008-2013 University of Sydney (Astronomy Tree)
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Publications

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Smart BM, Haffner LM, Barger KA, et al. (2019) The Diffuse Ionized Gas Halo of the Small Magellanic Cloud The Astrophysical Journal. 887: 16
Bannister KW, Madsen GJ. (2014) A Galactic origin for the fast radio burst FRB010621 Monthly Notices of the Royal Astronomical Society. 440: 353-358
Madsen GJ, Gaensler BM. (2013) A precision multi-band two-epoch photometric catalog of 44 million sources in the northern SKY from a combination of the USNO-B and Sloan Digital Sky survey catalogs Astrophysical Journal, Supplement Series. 209
Moss VA, Mcclure-Griffiths NM, Braun R, et al. (2012) GSH 006-15+7: A local Galactic supershell featuring transition from Hi emission to absorption Monthly Notices of the Royal Astronomical Society. 421: 3159-3169
Barger KA, Haffner LM, Wakker BP, et al. (2012) Present-day galactic evolution: Low-metallicity, warm, ionized gas inflow associated with high-velocity cloud complex A Astrophysical Journal. 761
Haffner LM, Duncan AK, Hoffman SM, et al. (2012) Ionization of infalling gas Eas Publications Series. 56: 319-322
Madsen GJ. (2012) Ionized gas in the Magellanic Stream Eas Publications Series. 56: 281-284
Reynolds RJ, Haffner LM, Madsen GJ, et al. (2012) Diffuse ionized gas in spiral galaxies and the disk-halo interaction Eas Publications Series. 56: 213-220
Harvey-Smith L, Madsen GJ, Gaensler BM. (2011) Magnetic fields in large-diameter H II regions revealed by the faraday rotation of compact extragalactic radio sources Astrophysical Journal. 736
McClure-Griffiths NM, Madsen GJ, Gaensler BM, et al. (2010) Measurement of a magnetic field in a leading arm high-velocity cloud Astrophysical Journal. 725: 275-281
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