ﻻ يوجد ملخص باللغة العربية
We present a measurement of the rate of type Ia supernovae (SNe Ia) from the first of three seasons of data from the SDSS-II Supernova Survey. For this measurement, we include 17 SNe Ia at redshift $zle0.12$. Assuming a flat cosmology with $Omega_m = 0.3=1-Omega_Lambda$, we find a volumetric SN Ia rate of $[2.93^{+0.17}_{-0.04}({rm systematic})^{+0.90}_{-0.71}({rm statistical})] times 10^{-5} {rm SNe} {rm Mpc}^{-3} h_{70}^3 {rm year}^{-1}$, at a volume-weighted mean redshift of 0.09. This result is consistent with previous measurements of the SN Ia rate in a similar redshift range. The systematic errors are well controlled, resulting in the most precise measurement of the SN Ia rate in this redshift range. We use a maximum likelihood method to fit SN rate models to the SDSS-II Supernova Survey data in combination with other rate measurements, thereby constraining models for the redshift-evolution of the SN Ia rate. Fitting the combined data to a simple power-law evolution of the volumetric SN Ia rate, $r_V propto (1+z)^{beta}$, we obtain a value of $beta = 1.5 pm 0.6$, i.e. the SN Ia rate is determined to be an increasing function of redshift at the $sim 2.5 sigma$ level. Fitting the results to a model in which the volumetric SN rate, $r_V=Arho(t)+Bdot rho(t)$, where $rho(t)$ is the stellar mass density and $dot rho(t)$ is the star formation rate, we find $A = (2.8 pm 1.2) times 10^{-14} mathrm{SNe} mathrm{M}_{sun}^{-1} mathrm{year}^{-1}$, $B = (9.3^{+3.4}_{-3.1})times 10^{-4} mathrm{SNe} mathrm{M}_{sun}^{-1}$.
We present a measurement of the volumetric Type Ia supernova (SN Ia) rate based on data from the Sloan Digital Sky Survey II (SDSS-II) Supernova Survey. The adopted sample of supernovae (SNe) includes 516 SNe Ia at redshift z lesssim 0.3, of which 27
ABRIDGED We present measurements of the Type Ia supernova (SN) rate in galaxy clusters based on data from the Sloan Digital Sky Survey-II (SDSS-II) Supernova Survey. The cluster SN Ia rate is determined from 9 SN events in a set of 71 C4 clusters at
We present the type Ia rate measurement based on two EROS supernova search campaigns (in 1999 and 2000). Sixteen supernovae identified as type Ia were discovered. The measurement of the detection efficiency, using a Monte Carlo simulation, provides t
We present the cosmological analysis of 752 photometrically-classified Type Ia Supernovae (SNe Ia) obtained from the full Sloan Digital Sky Survey II (SDSS-II) Supernova (SN) Survey, supplemented with host-galaxy spectroscopy from the SDSS-III Baryon
The rate evolution of subluminous Type Ia Supernovae is presented using data from the Supernova Legacy Survey. This sub-sample represents the faint and rapidly-declining light-curves of the observed supernova Ia (SN Ia) population here defined by low