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Title: Type Ia supernova rate studies from the SDSS-II Supernova Study

Abstract

The author presents new measurements of the type Ia SN rate from the SDSS-II Supernova Survey. The SDSS-II Supernova Survey was carried out during the Fall months (Sept.-Nov.) of 2005-2007 and discovered ~ 500 spectroscopically confirmed SNe Ia with densely sampled (once every ~ 4 days), multi-color light curves. Additionally, the SDSS-II Supernova Survey has discovered several hundred SNe Ia candidates with well-measured light curves, but without spectroscopic confirmation of type. This total, achieved in 9 months of observing, represents ~ 15-20% of the total SNe Ia discovered worldwide since 1885. The author describes some technical details of the SN Survey observations and SN search algorithms that contributed to the extremely high-yield of discovered SNe and that are important as context for the SDSS-II Supernova Survey SN Ia rate measurements.

Authors:
 [1]
+ Show Author Affiliations
  1. Univ. of Chicago, IL (United States)
Publication Date:
Research Org.:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE
OSTI Identifier:
948603
Report Number(s):
FERMILAB-THESIS-2008-80
TRN: US200907%%129
DOE Contract Number:
AC02-07CH11359
Resource Type:
Thesis/Dissertation
Country of Publication:
United States
Language:
English
Subject:
71 CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS, 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; ALGORITHMS; ASTROPHYSICS; FERMILAB; Astrophysics, Experiment-HEP

Citation Formats

Dilday, Benjamin. Type Ia supernova rate studies from the SDSS-II Supernova Study. United States: N. p., 2008. Web. doi:10.2172/948603.
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Dilday, Benjamin. Type Ia supernova rate studies from the SDSS-II Supernova Study. United States. doi:10.2172/948603.
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Dilday, Benjamin. Fri . "Type Ia supernova rate studies from the SDSS-II Supernova Study". United States. doi:10.2172/948603. https://www.osti.gov/servlets/purl/948603.
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@article{osti_948603,
title = {Type Ia supernova rate studies from the SDSS-II Supernova Study},
author = {Dilday, Benjamin},
abstractNote = {The author presents new measurements of the type Ia SN rate from the SDSS-II Supernova Survey. The SDSS-II Supernova Survey was carried out during the Fall months (Sept.-Nov.) of 2005-2007 and discovered ~ 500 spectroscopically confirmed SNe Ia with densely sampled (once every ~ 4 days), multi-color light curves. Additionally, the SDSS-II Supernova Survey has discovered several hundred SNe Ia candidates with well-measured light curves, but without spectroscopic confirmation of type. This total, achieved in 9 months of observing, represents ~ 15-20% of the total SNe Ia discovered worldwide since 1885. The author describes some technical details of the SN Survey observations and SN search algorithms that contributed to the extremely high-yield of discovered SNe and that are important as context for the SDSS-II Supernova Survey SN Ia rate measurements.},
doi = {10.2172/948603},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Fri Aug 01 00:00:00 EDT 2008},
month = {Fri Aug 01 00:00:00 EDT 2008}
}
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Thesis/Dissertation:
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DOI:  10.2172/948603
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  • ; ; ; ...
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  • ; ; ; ... - Astrophys.J.713:1026-1036,2010
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  • ; ; ; ... - Astrophysical Journal
    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 z {<=} 0.17 and 27 SN events in 492 maxBCG clusters at 0.1 {<=} z {<=} 0.3. We find values for the cluster SN Ia rate of (0.37{sup +0.17+0.01} {sub -0.12-0.01}) SNur h {sup 2} and (0.55{sup +0.13+0.02} {sub -0.11-0.01}) SNur h {sup 2} (SNux = 10{sup -12} L {sup -1} {sub xsun} yr{sup -1}) inmore » C4 and maxBCG clusters, respectively, where the quoted errors are statistical and systematic, respectively. The SN rate for early-type galaxies is found to be (0.31{sup +0.18+0.01} {sub -0.12-0.01}) SNur h {sup 2} and (0.49{sup +0.15+0.02} {sub -0.11-0.01}) SNur h {sup 2} in C4 and maxBCG clusters, respectively. The SN rate for the brightest cluster galaxies (BCG) is found to be (2.04{sup +1.99+0.07} {sub -1.11-0.04}) SNur h {sup 2} and (0.36{sup +0.84+0.01} {sub -0.30-0.01}) SNur h {sup 2} in C4 and maxBCG clusters, respectively. The ratio of the SN Ia rate in cluster early-type galaxies to that of the SN Ia rate in field early-type galaxies is 1.94{sup +1.31+0.043} {sub -0.91-0.015} and 3.02{sup +1.31+0.062} {sub -1.03-0.048}, for C4 and maxBCG clusters, respectively. The SN rate in galaxy clusters as a function of redshift, which probes the late time SN Ia delay distribution, shows only weak dependence on redshift. Combining our current measurements with previous measurements, we fit the cluster SN Ia rate data to a linear function of redshift, and find r{sub L} = [(0.49{sup +0.15} {sub -0.14})+(0.91{sup +0.85} {sub -0.81}) x z] SNuB h {sup 2}. A comparison of the radial distribution of SNe in cluster to field early-type galaxies shows possible evidence for an enhancement of the SN rate in the cores of cluster early-type galaxies. With an observation of at most three hostless, intra-cluster SNe Ia, we estimate the fraction of cluster SNe that are hostless to be (9.4{sup +8.3} {sub -5.1})%.« less

  • ; ; ; ... - Astrophysical Journal
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  • To determine the in vitro lactate-to-glycogen conversion potential of human muscle, samples were incubated in U-/sup 14/C-lactate. Because evidence existed suggesting that lactate-to-glycogen conversion occurred at a faster rate in Type II muscle in vivo glycogen resynthesis was calculated by the difference in muscle glycogen concentrations over the initial half-hour recovery period in the FT (Type II, fast-twitch) and ST (Type I, slow-twitch) muscle fiber pools from two of the original eight subjects.