[PDF] Top 20 Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run

Directional Limits on Persistent Gravitational Waves from Advanced LIGO’s First Observing Run

... The possibility of a young neutron star in SN 1987A [20,21] and the likelihood of many unknown, isolated neutron stars in the Galactic Center region [22] indicate potentially interesting candidates for persistent ... See full document

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Directional Limits on Persistent Gravitational Waves from Advanced LIGO's First Observing Run

... support from these agencies as well as by the Council of Scien- tific and Industrial Research of India, Department of Science and Technology, India, Science & Engineering Research Board (SERB), India, Ministry ... See full document

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Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs

... resolvable, persistent point-sources emitting GWs across a wide frequency ...upper limits on the amplitude of the anisotropic SGWB, and on point sources with broad and narrow frequency ...upper ... See full document

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Directional limits on persistent gravitational waves using LIGO S5 science data

... data from LIGO’s 4 and 2 km detectors (H1 and H2) in Hanford, WA and the 4 km detector (L1) in Livingston Parish, LA during the S5 science run ...including limits on GWs from the Crab pulsar ... See full document

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Directional limits on persistent gravitational waves using data from Advanced LIGO's first two observing runs

... data from the first (O1) and second (O2) observing runs of Advanced LIGO’s 4 km detectors in Hanford, Washington (H1) and Livingston, Louisiana ...collected from 15:00 UTC on 18 ... See full document

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Search for multimessenger sources of gravitational waves and high-energy neutrinos with advanced LIGO during its first observing run, ANTARES, and IceCube

... considered observing period had an effective duration of just ∼ ...GW observing runs. In addition, we anticipate that LIGO ’ s sensitivity will improve by a factor of ∼ 2 upon reaching design ... See full document

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All sky search for short gravitational wave bursts in the second Advanced LIGO and Advanced Virgo run

... The Advanced LIGO and Advanced Virgo detectors [1, 2] have completed their second observing run (O2) which lasted from November 30, 2016 to August 25, ...O2, ... 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

... For BNS and NS-BH coalescences, we use point-particle post-Newtonian models that describe the inspiral stage, where the orbit of the binary slowly shrinks due to the emission of GWs. This is mainly motivated by the fact ... See full document

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First Search for Gravitational Waves from Known Pulsars with Advanced LIGO

... cheap gravitational- wave searches over the length of our observation ...data from the initial LIGO, Virgo, and GEO 600 detectors (summarized in Aasi et ...upper limits on their signal ... See full document

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Narrow band search for gravitational waves from known pulsars using the second LIGO observing run

... using LIGO O2 data for the continuous wave emission of 33 ...the gravitational wave amplitude, over the analyzed frequency and spin-down ranges, have been computed for each of the ...to gravitational ... See full document

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All-sky search for short gravitational-wave bursts in the first Advanced LIGO run

... results from an all-sky search for short-duration gravitational waves in the data of the first run of the Advanced LIGO detectors between September 2015 and January ... See full document

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First Search for Gravitational Waves from Known Pulsars with Advanced LIGO

... cheap gravitational-wave searches over the length of our observation ...data from the initial LIGO, Virgo, and GEO 600 detectors (summarized in Aasi et ...upper limits on their signal ... See full document

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Binary black hole mergers in the first Advanced LIGO observing run

... The first observing run (O1) of the Advanced LIGO detectors took place from September 12, 2015, to January 19, ...to gravitational waves over a range of frequencies ... See full document

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Constraints on cosmic strings using data from the first Advanced LIGO observing run

... of gravitational waves, thus offering an experimental signature for the existence of cosmic ...for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO ... See full document

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All sky search for long duration gravitational wave transients in the second Advanced LIGO observing run

... 500 s and span a frequency band of 24 – 2048 ...for gravitational waves typically cast the analysis as pattern recognition ...problems. Gravitational-wave time-series are Fourier transformed ... See full document

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Constraints on cosmic strings using data from the first Advanced LIGO observing run

... of gravitational waves, thus offering an experimental signature for the existence of cosmic ...for gravitational-wave bursts from cosmic string loops in the data of Advanced LIGO ... See full document

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Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run

... using LIGO O2 data for the continuous wave emission of 33 ...upper limits on the gravitational wave amplitude over the analyzed frequency and spin-down ranges are computed for each of the ...to ... See full document

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Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run

... 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/Germany for ... 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

... 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/Germany for ... See full document

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Upper Limits on the Stochastic Gravitational Wave Background from Advanced LIGO's First Observing Run

... the limits from ground-based interferometers from the final science run of Initial LIGO-Virgo, the co-located detectors at Hanford (H1-H2), Advanced LIGO (aLIGO) O1, and ... See full document

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