The Hubble Space Telescope Cluster Supernova Survey. II. The Type la Supernova rate in high-redshift galaxy clusters
Journal Article
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· The Astrophysical Journal
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- Univ. of California, Berkeley, CA (United States). Dept. of Physics; Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
- Univ. of California, Berkeley, CA (United States). Dept. of Physics; Oskar Klein Centre for Cosmo Particle Physics, AlbaNova, Stockholm (Sweden)
- Harvard-Smithsonian Center for Astrophysics, Cambridge, MA (United States)
- Hamilton College, Clinton, NY (United States). Dept. of Physics
- Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States); Univ. of Utah, Salt Lake City, UT (United States). Dept. of Physics and Astronomy
- Univ. of Tokyo (Japan). Inst. of Astronomy. Graduate School of Science
- California Inst. of Technology (CalTech), La Canada Flintridge, CA (United States). Jet Propulsion Lab.
- Univ. of California, Santa Cruz, CA (United States). Santa Cruz Inst. for Particle Physics
- Space Telescope Science Inst., Baltimore, MD (United States)
- Univ. of Waterloo, ON (Canada). Dept. of Physics and Astronomy
- Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics
- Oskar Klein Centre for Cosmo Particle Physics, AlbaNova, Stockholm (Sweden); Stockholm Univ. (Sweden). Albanova University Center, Dept. of Physics
- National Astronomical Observatory of Japan, Hilo, HI (United States). Subaru Telescope
- Univ. of California, Berkeley, CA (United States). Dept. of Physics
- Univ. of Tokyo (Japan). Inst. of Astronomy. Graduate School of Science
- National Astronomical Observatory of Japan, Tokyo (Japan)
- Univ. of Chicago, IL (United States). Dept. of Astronomy and Astrophysics; Univ. of Chicago, IL (United States). Kavli Inst. for Cosmological Physics (KICP)
- Univ. of Tokyo (Japan). Inst. for Cosmic Ray Research
- Univ. of Bonn (Germany). Physikalisches Inst.
- Australian Astronomical Observatory, Epping, NSW (Australia)
- Univ. of California, Davis, CA (United States). Dept. of Physics
- Univ. of Tokyo (Japan). Inst. of Astronomy. Graduate School of Science; National Astronomical Observatory of Japan, Tokyo (Japan)
- Kyoto Univ., Kyoto (Japan). Dept. of Astronomy
- European Southern Observatory (ESO), Garching (Germany)
- Univ. of California, Davis, CA (United States). Dept. of Physics; Lawrence Livermore National Lab. (LLNL), Livermore, CA (United States). Inst. of Geophysics and Planetary Physics
Here we report a measurement of the Type Ia supernova (SN Ia) rate in galaxy clusters at 0.9 < z < 1.46 from the Hubble Space Telescope Cluster Supernova Survey. This is the first cluster SN Ia rate measurement with detected z > 0.9 SNe. Finding 8 ± 1 cluster SNe Ia, we determine an SN Ia rate of 0.50+0.23-0.19 (stat) +0.10 -0.09 (sys) h2 70 SNuB (SNuB ≡ 10-12 SNe L-1 ⊙,B yr-1). In units of stellar mass, this translates to 0.36 + 0.16 -0.13 (stat) +0.07 -0.06 (sys) h2 70 SNuM (SNuM ≡ 10-12 SNe M –1 ⊙ yr–1). This represents a factor of ≈ 5 ± 2 increase over measurements of the cluster rate at z < 0.2. We parameterize the late-time SN Ia delay time distribution (DTD) with a power law: Ψ(t)∝ts . Under the approximation of a single-burst cluster formation redshift of zf = 3, our rate measurement in combination with lower-redshift cluster SN Ia rates constrains s = –1.41+0.47 –0.40, 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.
- Research Organization:
- Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
- Sponsoring Organization:
- Australian Research Council (ARC); Japan Society for the Promotion of Science (JSPS); National Aeronautic and Space Administration (NASA); USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25); USDOE Office of Science (SC), Nuclear Physics (NP) (SC-26)
- Contributing Organization:
- The Supernova Cosmology Project (SCP)
- Grant/Contract Number:
- AC02-05CH11231
- OSTI ID:
- 1407144
- Alternate ID(s):
- OSTI ID: 22011995
- Journal Information:
- The Astrophysical Journal, Journal Name: The Astrophysical Journal Journal Issue: 1 Vol. 745; ISSN 0004-637X
- Publisher:
- Institute of Physics (IOP)Copyright Statement
- Country of Publication:
- United States
- Language:
- English
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