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Early Advanced LIGO binary neutron-star sky localization and parameter estimation

Berry, C. P. L. and Farr, B. and Farrell, W. M. and Haster, C.-J. and Mandel, I. and Middleton, H. and Singer, L. P. and Urban, A. L. and Vecchio, A. and Vitale, S. and Cannon, K. and Graff, P. B. and Hanna, C. and Mohapatra, S. and Pankow, C. and Price, L. R. and Sidery, T. and Veitch, J. (2016) Early Advanced LIGO binary neutron-star sky localization and parameter estimation. Journal of Physics: Conference Series, 716 . Art. No. 012031. ISSN 1742-6588. doi:10.1088/1742-6596/716/1/012031. https://resolver.caltech.edu/CaltechAUTHORS:20161206-080038832

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Abstract

2015 will see the first observations of Advanced LIGO and the start of the gravitational-wave (GW) advanced-detector era. One of the most promising sources for ground- based GW detectors are binary neutron-star (BNS) coalescences. In order to use any detections for astrophysics, we must understand the capabilities of our parameter-estimation analysis. By simulating the GWs from an astrophysically motivated population of BNSs, we examine the accuracy of parameter inferences in the early advanced-detector era. We find that sky location, which is important for electromagnetic follow-up, can be determined rapidly (~ 5 s), but that sky areas may be hundreds of square degrees. The degeneracy between component mass and spin means there is significant uncertainty for measurements of the individual masses and spins; however, the chirp mass is well measured (typically better than 0.1%).


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1088/1742-6596/716/1/012031DOIArticle
http://iopscience.iop.org/article/10.1088/1742-6596/716/1/012031/metaPublisherArticle
ORCID:
AuthorORCID
Mandel, I.0000-0002-6134-8946
Singer, L. P.0000-0001-9898-5597
Vecchio, A.0000-0002-6254-1617
Additional Information:© 2016 IOP Publishing. Content from this work may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and the title of the work, journal citation and DOI. This work was supported in part by STFC. This is LIGO document reference LIGO-P1500155. A catalogue of results is available at www.ligo.org/scientists/first2years/.
Group:LIGO
Funders:
Funding AgencyGrant Number
Science and Technology Facilities Council (STFC)UNSPECIFIED
Other Numbering System:
Other Numbering System NameOther Numbering System ID
LIGO DocumentLIGO-P1500155
DOI:10.1088/1742-6596/716/1/012031
Record Number:CaltechAUTHORS:20161206-080038832
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20161206-080038832
Official Citation:C P L Berry et al 2016 J. Phys.: Conf. Ser. 716 012031
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:72585
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:06 Dec 2016 19:58
Last Modified:11 Nov 2021 05:03

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