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Title: The Volumetric Rate of Calcium-rich Transients in the Local Universe

Here, we present a measurement of the volumetric rate of "calcium-rich" optical transients in the local universe, using a sample of three events from the Palomar Transient Factory (PTF). This measurement builds on a detailed study of the PTF transient detection efficiencies and uses a Monte Carlo simulation of the PTF survey. We measure the volumetric rate of calcium-rich transients to be higher than previous estimates: 1.21 -0.39 +1.13 10 -5 events yr -1Mpc -3. This is equivalent to 33%-94% of the local volumetric Type Ia supernova rate. This calcium-rich transient rate is sufficient to reproduce the observed calcium abundances in galaxy clusters, assuming an asymptotic calcium yield per calcium-rich event of ~0.05 M . As a result, we also study the PTF detection efficiency of these transients as a function of position within their candidate host galaxies. We confirm as a real physical effect previous results that suggest that calcium-rich transients prefer large physical offsets from their host galaxies.
Authors:
ORCiD logo [1] ; ORCiD logo [2] ; ORCiD logo [3] ; ORCiD logo [4]
  1. Univ. of Southampton, Southampton (United Kingdom); Univ. of Portsmouth, Portsmouth (United Kingdom)
  2. Univ. of Southampton, Southampton (United Kingdom)
  3. Queen's Univ. Belfast, Belfast (United Kingdom)
  4. Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Publication Date:
Grant/Contract Number:
AC02-05CH11231
Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 858; Journal Issue: 1; Related Information: © 2018. The American Astronomical Society. All rights reserved.; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Research Org:
Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)
Sponsoring Org:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR) (SC-21)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; galaxies: clusters: general; galaxies: clusters: intracluster medium; supernovae: general
OSTI Identifier:
1457006

Frohmaier, Chris, Sullivan, Mark, Maguire, Kate, and Nugent, Peter. The Volumetric Rate of Calcium-rich Transients in the Local Universe. United States: N. p., Web. doi:10.3847/1538-4357/aabc0b.
Frohmaier, Chris, Sullivan, Mark, Maguire, Kate, & Nugent, Peter. The Volumetric Rate of Calcium-rich Transients in the Local Universe. United States. doi:10.3847/1538-4357/aabc0b.
Frohmaier, Chris, Sullivan, Mark, Maguire, Kate, and Nugent, Peter. 2018. "The Volumetric Rate of Calcium-rich Transients in the Local Universe". United States. doi:10.3847/1538-4357/aabc0b.
@article{osti_1457006,
title = {The Volumetric Rate of Calcium-rich Transients in the Local Universe},
author = {Frohmaier, Chris and Sullivan, Mark and Maguire, Kate and Nugent, Peter},
abstractNote = {Here, we present a measurement of the volumetric rate of "calcium-rich" optical transients in the local universe, using a sample of three events from the Palomar Transient Factory (PTF). This measurement builds on a detailed study of the PTF transient detection efficiencies and uses a Monte Carlo simulation of the PTF survey. We measure the volumetric rate of calcium-rich transients to be higher than previous estimates: 1.21-0.39+1.13 10-5 events yr-1Mpc-3. This is equivalent to 33%-94% of the local volumetric Type Ia supernova rate. This calcium-rich transient rate is sufficient to reproduce the observed calcium abundances in galaxy clusters, assuming an asymptotic calcium yield per calcium-rich event of ~0.05 M⊙. As a result, we also study the PTF detection efficiency of these transients as a function of position within their candidate host galaxies. We confirm as a real physical effect previous results that suggest that calcium-rich transients prefer large physical offsets from their host galaxies.},
doi = {10.3847/1538-4357/aabc0b},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 858,
place = {United States},
year = {2018},
month = {5}
}