[PDF] Top 20 Multi-messenger Observations of a Binary Neutron Star Merger
Has 10000 "Multi-messenger Observations of a Binary Neutron Star Merger" found on our website. Below are the top 20 most common "Multi-messenger Observations of a Binary Neutron Star Merger".
Multi-messenger Observations of a Binary Neutron Star Merger
... ( Las Cumbres ) Support for I.A. and J.B. was provided by NASA through the Einstein Fellowship Program, grants PF6- 170148 and PF7-180162, respectively. D.A.H., C.M., and G.H. are supported by NSF grant AST-1313484. D.P. ... See full document
59
Multi messenger observations of a binary neutron star merger
... Collaboration, AstroSat Cadmium Zinc Telluride Imager Team, IPN Collaboration, The Insight- Hxmt Collaboration, ANTARES Collaboration, The Swift Collaboration, AGILE Team, The 1M2H Team, The Dark Energy Camera GW-EM ... See full document
60
Determination of Multi-Messenger Signals from Matter Outflows of Merger Systems
... a neutron star - neutron star ...of neutron star mergers are significant because the multi-messenger signals in the form of gravitational waves and electromagnetic ... See full document
26
Upper limits on the rates of binary neutron star and neutron star–black hole mergers from Advanced LIGO's first observing run
... from binary pulsar observations were reviewed in 2010 to produce rate estimates for canonical ...in binary evolution, hence underestimating the underlying uncertainties; ...and binary pulsar ... See full document
15
An r−process macronova/kilonova in GRB 060614: evidence for the merger of a neutron star-black hole binary
... to the forward shock (FS) and subsequently fitted all VLT V / R / I-band data at t > 1 . 7 day with the same decline rate. In such an analysis, only one F814W-band point at t ∼ 13.6 days was found to be significantly in ... See full document
6
Analysis methods for gravitational wave from binary neutron star coalescences: investigation on the post-merger phase
... of neutron stars and NS ...their observations followed by a short description of the NS internal structure, the observed values of mass and ...of binary system, followed by some general comments ... See full document
218
Search for Neutrinos in Super-Kamiokande Associated with the GW170817 Neutron-star Merger
... after merger. Neutrino observations associated with a binary neutron-star merger using the unique characteristics in SK would validate such proposed mechan- ...the merger ... See full document
7
General relativistic magnetohydrodynamic simulations of binary neutron star mergers
... the coefficients of the spin-weighted spherical harmonics expansion. In order to obtain the actual strain that would be measured by a GW detector, one should multiply our value by the spin-weighted spherical harmonics in ... See full document
90
Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
... In addition to limited gamma-ray detector sensitivity, determining the redshift from EM observations alone is more dif fi cult for SGRBs than for long GRBs. The fraction of SGRBs with detected X-ray afterglows for ... See full document
27
The electromagnetic counterpart of the binary neutron star merger LIGO/Virgo GW170817 I Discovery of the optical counterpart using the Dark Energy Camera
... fast multi- component fi tting software ( Im fi t; Erwin 2015 ) followed by point-spread function ( PSF ) photometry and a Pan-STARRS PS1 calibration to double check the ... See full document
7
r-process observations
... heavy neutron-capture elements in explosive events by optical spectroscopy to measure spectral lines, or by observations of γ-ray from radio-active nuclei, are desired to identify the sites of the r-process ... See full document
6
Properties of the Binary Neutron Star Merger GW170817
... analysis. It should also be noted that GEO600 was not in science mode due to investigations into a degraded squeezer phase error point signal leading to a reduced level of squeezing. At the time of the event, the inves- ... See full document
32
Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817
... In situations with great theoretical uncertainties, where no complete set of accurate GW template waveforms is available, a matched- fi lter search is not feasible. Instead, an ef fi cient solution is to search for excess ... See full document
13
Properties of the binary neutron star merger GW170817
... analysis. It should also be noted that GEO600 was not in science mode due to investigations into a degraded squeezer phase error point signal leading to a reduced level of squeezing. At the time of the event, the inves- ... See full document
32
Multimessenger Probes of High-energy Sources
... Multimessenger observations may hold the key to learn about the most ener- getic sources in the ...neutrino observations and electromagnetic signals to obtain a comprehensive picture of some of the most ... See full document
9
Evidence for dynamically driven formation of the GW170817 neutron star binary in NGC 4993
... galaxy merger with still visible ...and observations show that the maximum drop to the outer parts of ellipticals near the effective radius is ∼ 40% of the central value ( Emsellem et ... See full document
8
Accretion in supergiant High Mass X-ray Binaries
... heavier neutron star, more gas will accumulate and the absorption will get ...the neutron star, the more bended the accretion ...the neutron star is in the range M NS = ... See full document
6
KIC 2856960 : the impossible triple star
... triple star observed by Kepler. Listed as an eclipsing binary by Prˇsa et ...the binary (Armstrong et al. 2012). The binary in KIC 2856960 reveals itself through ∼ 1%-deep eclipses (primary ... See full document
12
From nuclear structure to neutron stars
... above, neutron star radius measurements have proven more di ffi cult, because they require both a distance measurement and some degree of modeling of the neutron star X-ray ...are ... See full document
14
Accurate X ray position and multiwavelength observations of the isolated neutron star RBS 1774
... We acknowledge the director of the Chandra X-ray Obser- vatory, Harvey Tananbaum, for according us the RBS 1774 observation through its Director Discretionary Time. These results are based on observations ... See full document
9
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