The Effects of Halo-to-halo Variation on Substructure Lensing

We explore the halo-to-halo variation of dark matter (DM) substructure in galaxy-sized DM halos, focusing on its implications for strongly gravitational lensed systems. We find that the median value for projected substructure mass fractions within projected radii of 3% of the host halo virial radius...

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Veröffentlicht in:The Astrophysical journal 2011-11, Vol.741 (2), p.117-jQuery1323901914973='48'
Hauptverfasser: Chen, Jacqueline, Koushiappas, Savvas M, Zentner, Andrew R
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Sprache:eng
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Zusammenfassung:We explore the halo-to-halo variation of dark matter (DM) substructure in galaxy-sized DM halos, focusing on its implications for strongly gravitational lensed systems. We find that the median value for projected substructure mass fractions within projected radii of 3% of the host halo virial radius is approximately f sub 0.25%, but that the variance is large with a 95 percentile range of 0
ISSN:0004-637X
1538-4357
DOI:10.1088/0004-637X/741/2/117