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Table 1.Source Parameters for Faults Included in the Hazard Analysis 2017 Update for the Henderson Site <br /> Slip Rste6 <br /> Maximum (mmyr)/ <br /> Probability of Rupture Length Sense of Mchar Recurrence <br /> Faukl Rupture Model Activity a km Sli Dips Intervals Data Sources Comments <br /> Chase Gulch(West <br /> and East)and <br /> Eleven Mile faults 0.07(0.5) Due to their close spatial association and their short lengths(5 5 km),we grouped the <br /> (Q64,Q65, 6.6(0.2) 35°E(0.2) 0.2(0.5) West-side Chase Gulch and Eleven Mile faults with the much longer East-side Chase <br /> Q66/2316,2317, 6.9(0.6) 5W E(0.6) WM:0.14 Widmann et al.(1998);Shaffer gulch fault. Slip rates are based on 2.5 in of vertical offset on Pinedale-age(13 to 25 <br /> 2318) Linked 1.0 1.0 1 31 N 7.2(0.2)1 65°E 0.2 1980 ka deposits and 9.1 in on Bull Lake age 120 to 140 ka deposits Shaffer,1980 <br /> Our characterization and geometry is revised from Olig et al.(2013)to incorporate <br /> new data(Derouin,2014)and better address uncertainties regarding the southern <br /> extent of the fault.We include two rupture scenrios,A and B,and both extend along <br /> the Gore Range based on mapping done by the USBR using LIDAR data(L.W. <br /> Anderson,personal communication,2009;Derouin et al.,2010} Scenario A <br /> terminates near Frisco,is the some as the unsegmented model of Olig et al.(2013),and <br /> is favored based on evidence of similar amounts of late Quaternary offsets and <br /> Pinedale-age deposits offset along much of the Gore Range(Derouin,2014} Scenario <br /> B extends another 10 km to the southeast to include apparently older normal faults <br /> along the base of the Tenmile Range mapped by Kellogg et al.(2003)and Wallace et al. <br /> (2003}We did not include a scenario extending as far south as Alma as mapped by <br /> Tweto et al.(1978)and included in the USGS database and by Widmann et al.(1998) <br /> because neither Anderson or Wallace et al.(2003)found evidence for faulting this far <br /> southeast along the Blue River. <br /> Tweto et al.(1970)first identified evidence for Quaternary activity but West(1978) <br /> Tweto et al.(1970,1978);West believed that apparent displacement of Quaternary deposits along the fault was non- <br /> (1978);Widmann et al.(1998, tectonic. However,based on detailed surficial studies at two sites,Unruh et al.(1993) <br /> 2002);Unruh et al.(1993, concluded that Pinedale-age deposits were tectonically offset but Holocene deposits <br /> 0.02(0.2) 19%a);Kellogg et at.(2002); were in depositional contact with the fault.More recent detailed studies by the USBR <br /> 0.04(0.4) Wallace et al.(2003);O'Connell have confirmed repeated late Quaternary tectonic offsets and as much as 3.0 in of <br /> Frontal fault(or 6.9(0.2) 0.26(0.3) et al.(2005);Anderson(2007); offset on Pinedale-age surfaces(Derouin et al.,2010;Derouin,2014),and so we assign <br /> Gore Range Frontal 1.0 72(0.6) 35°E(0.2) 0.5(0.1) L.W.Anderson,USBR,personal a p(a)of 1.0. Our slip rates are based on the USBR surface offsets,relative and <br /> fault) Rupture Scenario A(0.7) 51 7.5(0.2) 50°E(0.6) WM:0.15 communication,2009;Derouin coseismogenic radionuclide ages(Derouin,2014;see Table 5).and converting surface <br /> 512302 N 65°E 02 et al. 2010•Derouin 2014 offsets to dip slip rates using the formula of Caake 199 . <br /> 6.9(0.2) <br /> 72(0.6) <br /> 7.5(0.2) <br /> Rupture Scenario B(03) 61 <br /> 0.001(02) <br /> 6.6(02) 35'E(0.2) 0.004(0.6) "Suspect fault"(Widmann et al.,1998),not considered active in deterministic analysis <br /> Golden halt 6.9(0.6) 50"E(0.6) 0.02(02) Widmann et al.(1998,2002); of Unruh et al.(19%b} <br /> 742324 Independent 1.0 02 1 30 N/SS? 72 02 65°E 0.2 WM:0.007 Unroh et at. 1996b;URS 2001 <br />