THE HUBBLE SPACE TELESCOPE CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS.

We report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < ɀ < 1.46 from the Hubble Space Telescope Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected ɀ > 0.9 SNe. Finding 8 ± 1 cluster SNe Ia, we determine an SN Ia rate of 0.50 Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. (stat) Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. (sys) Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. SNuB (SNUB ≡ 10^-12 SNe Lʘ^-1 yr^-1). In units of stellar mass, this translates to. 0.13 Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. (stat) Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. (sys) Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. SNuM (SNuM ≡ 10^-12 SNe Mʘ^-1 yr^-1 ). This represents a factor of ≈5 ± 2 increase over measurements of the cluster rate at ɀ < 0.2. We parameterize the late-time SN Ia delay time distribution (DTD) with a power law: ψ (_t) _t Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. ₅ Under the approximation of a single-burst cluster formation redshift of ɀ_f = 3, our rate measurement in combination with lower-redshift cluster SN Ia rates constrains s = - 1.41 Due to image rights restrictions, multiple line equation(s) cannot be graphically displayed. consistent with measurements of the DTD in the field. This measurement is generally consistent with expectations for the "double degenerate" scenario and inconsistent with some models for the "single degenerate" scenario predicting a steeper DTD at large delay times. We check for environmental dependence and the influence of younger stellar populations by calculating the rate specifically in cluster red-sequence galaxies and in morphologically early-type galaxies, finding results similar to the full cluster rate. Finally, the upper limit of one hostless cluster SN Ia detected in the survey implies that the fraction of stars in the intra-cluster medium is less than 0.47 (95% confidence), consistent with measurements at lower redshifts. [ABSTRACT FROM AUTHOR]