[PDF] Top 20 Searches for gravitational waves from known pulsars with science run 5 LIGO data
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Searches for gravitational waves from known pulsars with science run 5 LIGO data
... National Science Foundation for the construction and operation of the LIGO Laboratory, the Science and Technology Facilities Council of the United Kingdom, the Max-Planck- Society, and the State of ... See full document
15
Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015 2017 LIGO Data
... previous searches for gravitational waves from known pulsars described in Aasi et ...time-domain data to perform Bayesian parameter estimation for the unknown signal ... See full document
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Searches for gravitational waves from known pulsars at two harmonics in 2015–2017 LIGO data
... the run ( see Section ...the gravitational-wave ...the gravitational-wave amplitude and orienta- tion angles of the source ( inclination and polarization ) are assumed to remain fi xed over the ... See full document
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Binary system delays and timing noise in searches for gravitational waves from known pulsars
... been known about since the early days of pulsar observations and represents a random walk in phase, frequency or fre- quency derivative of the pulsar about the regular spin- down model given in ... See full document
10
Narrow band search for gravitational waves from known pulsars using the second LIGO observing run
... geted searches. 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 ... See full document
20
First Search for Gravitational Waves from Known Pulsars with Advanced LIGO
... of known pulsars, identified through electro- magnetic observations, provides an important possible source of continuous gravitational ...cheap gravitational-wave searches over the ... See full document
20
First Search for Gravitational Waves from Known Pulsars with Advanced LIGO
... cheap gravitational- wave searches over the length of our observation ...of known pulsars have already been targeted us- ing data from the initial LIGO, Virgo, and GEO 600 ... See full document
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Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut B with Advanced LIGO
... wave searches for isolated non-pulsing neutron stars in data from the first Advanced LIGO observing run ...coherent data analysis pipeline used in Abadie et ...initial ... See full document
21
First search for nontensorial gravitational waves from known pulsars
... of searches for generalized polarization states (tensor, vector, or scalar) in gravitational waves from spinning neutron ...the gravitational polarization content and, in so doing, ... See full document
13
Searches for continuous gravitational waves from 15 supernova remnants and Fomalhaut b with Advanced LIGO
... young pulsars are rapid enough to include signi fi cant continuous GW emission, as shown by the latest GW search for known pulsars ( Abbott et ...contain known pulsars ( Green 2014 ) ... See full document
15
First Search for Nontensorial Gravitational Waves from Known Pulsars
... almost-monochromatic waves expected from spinning neutron stars with an asymmetric moment of inertia ...[20]. Known galactic pulsars are one of the main candidates for searches for such ... See full document
17
Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run
... observing run. These types of searches are referred to as targeted ...The LIGO and Virgo Collaborations have already searched for this type of emission from known pulsars (both ... See full document
20
First narrow band search for continuous gravitational waves from known pulsars in advanced detector data
... continuous waves (CW), with a frequency at a given fixed ratio with respect to the star’s rotational frequency, ...CW searches exist, depending on the degree of knowl- edge on the source ...Targeted ... See full document
19
Gravitational waves from known pulsars : results from the initial detector era
... advanced LIGO (aLIGO) (Harry & LIGO Scientific Collaboration 2010) and Virgo (AdV) (Acernese et ...new pulsars (Lazarus 2013) and making use of distributed computing through Einstein@home (Allen ... See full document
18
Searches for periodic gravitational waves from unknown isolated sources and Scorpius X-1 : results from the second LIGO science run
... Each LIGO detector is a recycled Michelson interfer- ometer with Fabry-Perot arms, whose lengths are defined by suspended mirrors that double as test ...were known to be functioning not at the required ... See full document
35
Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data
... of searches for periodic gravitational waves have been carried out previously in LIGO data [1–10], including coherent searches for gravitational radiation from ... See full document
15
All-sky LIGO search for periodic gravitational waves in the early fifth-science-run data
... continuous-wave gravitational radiation of linear and circular polarization, corresponding to least favorable and most favorable pulsar orientations, ...to gravitational radiation approximately satisfies ... See full document
6
Comprehensive all-sky search for periodic gravitational waves in the sixth science run LIGO data
... L. Conti, 44 D. Cook, 39 T. R. Corbitt, 2 N. Cornish, 33 A. Corsi, 72 S. Cortese, 36 C. A. Costa, 13 M. W. Coughlin, 61 S. B. Coughlin, 82 J.-P. Coulon, 54 S. T. Countryman, 41 P. Couvares, 1 E. E. Cowan, 65 D. M. ... See full document
14
Application of a Hough search for continuous gravitational waves on data from the fifth LIGO science run
... But limitations on the memory of the computers constrain the volume of data (i.e., the number of SFTs) that can be analyzed at once and the parameter space (e.g., size and resolution of the sky-patches and number ... See full document
36
Search for gravitational-wave bursts in LIGO data from the fourth science run
... for gravitational-wave “bursts” that is designed to be able to detect short-duration (≪ 1 s) signals of arbitrary form as long as they have significant signal power in the most sensitive frequency band of ... See full document
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