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The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data

Adams, S. M. and Kochanek, C. S. and Gerke, J. R. and Stanek, K. Z. (2017) The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data. Monthly Notices of the Royal Astronomical Society, 469 (2). pp. 1445-1455. ISSN 0035-8711. https://resolver.caltech.edu/CaltechAUTHORS:20170828-081841800

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Abstract

We report updated results for the first 7 yr of our programme to monitor 27 galaxies within 10 Mpc using the Large Binocular Telescope to search for failed supernovae (SNe) – core collapses of massive stars that form black holes without luminous SNe. In the new data, we identify no new compelling candidates and confirm the existing candidate. Given the six successful core-collapse SNe in the sample and one likely failed SN, the implied fraction of core collapses that result in failed SNe is f=0.14^(+0.33)_(−0.10) at 90 per cent confidence. If the current candidate is a failed SN, the fraction of failed SN naturally explains the missing high-mass red supergiants SN progenitors and the black hole mass function. If the current candidate is ultimately rejected, the data imply a 90 per cent confidence upper limit on the failed SN fraction of f < 0.35.


Item Type:Article
Related URLs:
URLURL TypeDescription
https://doi.org/10.1093/mnras/stx898DOIArticle
https://arxiv.org/abs/1610.02402arXivDiscussion Paper
ORCID:
AuthorORCID
Adams, S. M.0000-0001-5855-5939
Kochanek, C. S.0000-0001-6017-2961
Alternate Title:The Search for Failed Supernovae with the Large Binocular Telescope: Constraints from 7 Years of Data
Additional Information:© 2017 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. Accepted 2017 April 10. Received 2017 April 10; in original form 2016 October 7. Published: 12 April 2017. We thank Adam Leroy for early access to his proprietary HST imaging. Financial support for this work was provided by NSF through grant AST-1515876. This work is based on observations made with the Large Binocular Telescope. The LBT is an international collaboration among institutions in the United States, Italy and Germany. The LBT Corporation partners are: the University of Arizona on behalf of the Arizona university system; the Istituto Nazionale di Astrofisica, Italy; the LBT Beteiligungsgesellschaft, Germany, representing the Max Planck Society, the Astrophysical Institute Potsdam and Heidelberg University; the Ohio State University and the Research Corporation, on behalf of the University of Notre Dame, the University of Minnesota and the University of Virginia. This work also utilized observations made with the NASA/ESA Hubble Space Telescope, obtained from the data archive at the Space Telescope Science Institute. STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555.
Funders:
Funding AgencyGrant Number
NSFAST-1515876
NASANAS 5-26555
Subject Keywords:black hole physics – surveys – stars: massive – supernovae: general
Issue or Number:2
Record Number:CaltechAUTHORS:20170828-081841800
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20170828-081841800
Official Citation:S. M. Adams, C. S. Kochanek, J. R. Gerke, K. Z. Stanek; The search for failed supernovae with the Large Binocular Telescope: constraints from 7 yr of data, Monthly Notices of the Royal Astronomical Society, Volume 469, Issue 2, 1 August 2017, Pages 1445–1455, https://doi.org/10.1093/mnras/stx898
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:80832
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:28 Aug 2017 19:12
Last Modified:05 Nov 2019 00:40

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