Parameter estimation for binary neutron-star coalescences with realistic noise during the Advanced LIGO era

Document #:

LIGO-P1400232-v8

Document type:

P - Publications

Abstract:

Advanced ground-based gravitational-wave (GW) detectors shall begin operation imminently. Their intended goal is not only to make the first direct detection of GWs, but also to make inferences about the source systems. Binary neutron-star mergers are among the most promising sources. We investigate the performance of the parameter-estimation pipeline that will be used during the first observing run of the Advanced Laser Interferometer Gravitational-wave Observatory (aLIGO) in 2015: we concentrate on the ability to reconstruct the source location on the sky, but also consider the ability to measure masses and the distance. Accurate, rapid sky-localization is necessary to alert electromagnetic (EM) observatories so that they can perform follow-up searches for counterpart transient events. We consider parameter-estimation accuracy in the presence of realistic, non-Gaussian noise. We find that the character of the noise makes negligible difference to the parameter-estimation performance. The source luminosity distance can only be poorly constrained, the median 90% (50%) credible interval scaled with respect to the true distance is 0.85 (0.38). However, the chirp mass is well measured. Our chirp-mass estimates are subject to systematic error because we used gravitational-waveform templates without component spin to carry out inference on signals with moderate spins, but the total error is typically less than 0.001 solar masses. The median 90% (50%) confidence region is ~600 deg^2 (~150 deg^2), with 3% (30%) of detected events localized within 100 deg^2. Early aLIGO, with only two detectors, will have a sky-localization accuracy for binary neutron stars of hundreds of square degrees; this makes EM follow-up challenging, but not impossible.

Files in Document:

• Manuscript (recoloured_sky_localization.pdf, 1.5 MB)

Other Files:

• All simulated BNS signals, including those that are not detected (2015_recoloured_all_inj.txt, 3.8 MB)
• Chirp mass and distance parameter estimation (recoloured noise) (2015_pe.txt, 19.7 kB)
• Chirp mass and distance parameter estimation (recoloured noise) (2015_recoloured_pe.txt, 25.6 kB)
• Detections and sky localization areas (2015_recoloured_coinc.txt, 34.2 kB)
• FITS sky maps (2015_recoloured_fits.tar, 1.3 GB)
• Raw SQLite database from GSTLAL analysis (H1L1-ALL_LLOID_1_injections-966384015-5184000.sqlite, 83.2 MB)
• Simulated BNS signals (2015_recoloured_inj.txt, 35.0 kB)

Topics:

• Astrophysics / Multi-messenger
• Data analysis software
• Compact Binaries

Authors:

• Christopher Berry
• Ilya Mandel
• Hannah Middleton
• Leo Singer
• Alexander Urban
• Alberto Vecchio
• Salvatore Vitale
• Kipp Cannon
• Benjamin Farr
• Will Farr
• Philip Graff
• Chad Hanna
• Carl-Johan Haster
• Satyanarayan Ray Pitambar Mohapatra
• Chris Pankow
• Larry Price
• Trevor Sidery
• John Veitch

Keywords:

sky-localization parameter-estimation recoloured-noise

Notes and Changes:

Published version

Related Documents:

• LIGO-P1300187: The First Two Years of Electromagnetic Follow-Up with Advanced LIGO and Virgo
• LIGO-P1200087: Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO, Advanced Virgo and KAGRA

Referenced by:

• LIGO-G1500120-v1: Gravitational-wave parameter estimation for binary neutron-star coalescences during the advanced-detector era
• LIGO-G1500527-v1: Parameter estimation with Advanced LIGO
• LIGO-G1500553-v3: Binary neutron-star parameter estimation with Advanced LIGO
• LIGO-G1500555-v2: Early Advanced LIGO binary neutron-star sky localization and parameter estimation
• LIGO-P1500155-v4: Early Advanced LIGO binary neutron-star sky localization and parameter estimation

Journal References:

Published in ApJ vol. 804 pg. 114.

Publication Information:

arXiv:1411.6934 [astro-ph.HE] http://arxiv.org/abs/1411.6934

Data release http://www.ligo.org/scientists/first2years/

ApJ; 804(2):114(24); 2015 http://dx.doi.org/10.1088/0004-637X/804/2/114