[PDF] Top 20 Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
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Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
... Using the techniques described in [38], we have not been able to identify a coherent instrumental witness channel that would explain this large SNR. But the fact that the sky direction of the maximum SNR is close ... See full document
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Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs
... Using the techniques described in [38], we have not been able to identify a coherent instrumental witness channel that would explain this large SNR. But the fact that the sky direction of the maximum SNR is close ... See full document
15
Directional limits on persistent gravitational waves using LIGO S5 science data
... patches. Observing no evidence of GWs, we set upper limits on GW ...the limits are between 5 31 10 49 strain 2 Hz 1 sr 1 ; for SHD ¼ 0, the limits are between 6 35 10 49 strain 2 Hz 1 sr 1 ; ... See full document
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Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run
... The data segments are Fourier transformed and coarse- grained to produce power spectra with a resolution of 1=32 ...previous LIGO-Virgo stochastic searches [15,17] in order to remove many finely spaced ... See full document
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Directional Limits on Persistent Gravitational Waves from Advanced LIGO's First Observing Run
... time-series data are down- sampled to 4096 Hz from 16 kHz, and divided into 192 s, 50% overlapping, Hann-windowed segments, which are high-pass filtered with a 16th order Butterworth digital filter ... See full document
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Upper Limits on the Stochastic Gravitational Wave Background from Advanced LIGO's First Observing Run
... of gravitational waves. Data are also excluded when the detectors’ noise power spectra vary by more than 20% over the course of three 192s seg- ... See full document
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Search for gravitational waves from Scorpius X-1 in the first Advanced LIGO observing run with a hidden Markov model
... X-1 using data collected by Initial LIGO and Advanced LIGO ...detection. First, a coherent search, using a maximum likelihood detection statistic called the F -statistic ... See full document
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Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run
... stochastic gravitational-wave ...background from unresolved compact binary coalescences is expected to be particularly ...stochastic gravitational-wave background using data from ... See full document
12
Searching for Gravitational Waves from Compact Binary Coalescences in Advanced LIGO Data
... of gravitational waves [6] by the Advanced LIGO detectors [19] marked the beginning of an era of gravitational-wave ...These waves were emitted during the final fraction of a ... See full document
175
Search for multimessenger sources of gravitational waves and high-energy neutrinos with advanced LIGO during its first observing run, ANTARES, and IceCube
... candidate from the candidates identi fi ed in time-shifted GW ...candidate from the set of all observed neutrino candidates, and assign this to the selected GW ...the two events to be temporally ...’ ... See full document
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All sky search for continuous gravitational waves from isolated neutron stars using Advanced LIGO O2 data
... [43]) using O2 data from the Advanced LIGO ...different data analysis methods and covers differ- ent regions of the parameter space, although there ex- ists some overlap between ... See full document
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Search for eccentric binary black hole mergers with advanced LIGO and advanced Virgo during their first and second observing runs
... Template-based gravitational-wave searches used by Advanced LIGO and Advanced Virgo currently do not include eccentric orbital templates ( Abbott et ... See full document
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The Importance of Spin for Observing Gravitational Waves from Coalescing Compact Binaries with LIGO and Virgo
... emits data, or a sink, which accepts ...synchronize data streams, which otherwise may process ...the data on disk (or from a real-time broadcasting source) and stores it in ...The data ... See full document
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Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B
... the LIGO Laboratory and Advanced LIGO as well as the Science and Technology Facilities Council ( STFC ) of the United Kingdom, the Max- Planck-Society ( MPS ) , and the State of Niedersachsen / ... See full document
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Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo
... calculated from parameter-estimation studies (neglecting detector calibration uncertainty) [31, 99] using LALInference ...estimated from timing triangulation (highlighted by italics), which is known ... See full document
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Limits on Gravitational Wave Emission from Selected Pulsars Using LIGO Data
... curve: LIGO design sensitivity for 1 yr of data. Stars: upper limits found in this paper for 28 known ...upper limits for the pulsars with negative frequency derivative values if all the ... See full document
6
Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run
... The LIGO and Virgo Collaborations have already searched for this type of emission from known pulsars (both isolated and some in binaries) [11–19], for which accurate ephemerides were ...range using ... See full document
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Limits on gravitational-wave emission from selected pulsars using LIGO data
... strain data from each detector at the instantaneous frequency of the expected gravitational- wave signal, which is twice the observed radio rotation ...These data are then down-sampled to 1=60 ... See full document
6
Search for intermediate mass black hole binaries in the first and second observing runs of the Advanced LIGO and Virgo network
... [83] D. Mukherjee, S. Caudill, R. Magee, C. Messick, S. Privitera, S. Sachdev, K. Blackburn, P. Brady, P. Brockill, K. Cannon, S. J. Chamberlin, D. Chatter- jee, J. D. E. Creighton, H. Fong, ... See full document
19
Searches for gravitational waves from known pulsars at two harmonics in 2015–2017 LIGO data
... this data set the fi rst of its ...emission from YSO fl ...Sun. Two of the studied fl ares showed excess emission at ...upper limits on nonthermal emission allow for enough nonthermal energy to ... See full document
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