Brandon A. Allgood, Ph.D.
Affiliations: | 2005 | University of California, Santa Cruz, Santa Cruz, CA, United States |
Area:
cosmologyGoogle:
"Brandon Allgood"Mean distance: 13.54 | S | N | B | C | P |
Parents
Sign in to add mentor| Joel Robert Primack | grad student | 2005 | UC Santa Cruz | |
| (Shapes and orientations of dark matter halos.) | ||||
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Publications
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| Kassin SA, Devriendt J, Fall SM, et al. (2012) The radius of baryonic collapse in disc galaxy formation Monthly Notices of the Royal Astronomical Society. 424: 502-507 |
| Flores RA, Allgood B, Kravtsov AV, et al. (2007) The shape of galaxy cluster dark matter haloes: systematics of its imprint on cluster gas and comparison to observations Monthly Notices of the Royal Astronomical Society. 377: 883-896 |
| Allgood B, Flores RA, Primack JR, et al. (2006) The shape of dark matter haloes: Dependence on mass, redshift, radius and formation Monthly Notices of the Royal Astronomical Society. 367: 1781-1796 |
| Wechsler RH, Zentner AR, Bullock JS, et al. (2006) The dependence of halo clustering on halo formation history, concentration, and occupation Astrophysical Journal. 652: 71-84 |
| Faltenbacher A, Allgood B, Gottlöber S, et al. (2005) Imprints of mass accretion on properties of galaxy clusters Monthly Notices of the Royal Astronomical Society. 362: 1099-1108 |
| Kazantzidis S, Kravtsov AV, Zentner AR, et al. (2004) The effect of gas cooling on the shapes of dark matter halos Astrophysical Journal. 611: L73-L76 |
| Kravtsov AV, Berlind AA, Wechsler RH, et al. (2004) The dark side of the halo occupation distribution Astrophysical Journal. 609: 35-49 |