Upper limits from directed searches in O1 data
First upper limits from LIGO on gravitational wave bursts
... them from seismic ...the data collected in science mode are available for gravitational wave ...wave data channel 兲 is derived from the error signal of the feedback loop used to control the ...
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Upper limits on gravitational wave emission from 78 radio pulsars
... wave searches as their positions and frequencies are generally well-known through radio or X-ray observa- ...nals from unknown sources, giving a lower significance ...waves from the majority of known ...
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Upper limits on gravitational wave emission from 78 radio pulsars
... present upper limits on the gravitational wave emission from 78 radio pulsars based on data from the third and fourth science runs of the LIGO and GEO 600 gravitational wave ...The ...
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Upper limits on gravitational wave emission from 78 radio pulsars
... the upper limit deduced from the observed spin-down via ...wave data, including upper limits, have a likely bearing on the nature of the neutron ...spin-down upper limit will ...
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Upper limits on gravitational wave emission from 78 radio pulsars
... All upper limit results from the individual S3 and S4 runs along with results from the combined run, with and without GEO 600 included, are given in Appendix B in Tables III and ...600 data ...
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Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-based Cross-correlation Search in Advanced LIGO Data
... frequency-dependent upper limits were set using a combination of sensitivity estimates and simulated signal ...stringent upper limit was set at 175 Hz, with comparable limits set across the ...
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Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts
... coincident data collected during early ...analyzed data only from periods when at least three interferometers (including the two LIGO- Hanford interferometers) were operating, and we required ...
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Upper limits on the strength of periodic gravitational waves from PSR J1939+2134
... the data from all four interferometers to be combined to give an improved joint upper limit, although the relative phase calibration of the instruments was not sufficiently reliable to do this for ...
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ULEDS-SVMs: Upper/Lower Limits and Error Data Supposted Support Vector Machines
... of data by following the conditions that satisfy the trainability, as described ...prepared data are fed to conventional SVMs for training. When both limits and errors exist, the above scenario can ...
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MAGIC upper limits on the GRB 090102 afterglow
... emission from GRBs are known since the EGRET ob- servations during the 1990’s and they have been confirmed by the data of the Fermi ...GRBs from several tens up to hundreds of GeV energy ...GeV) ...
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Limits on active to sterile neutrino oscillations from disappearance searches in the MINOS, Daya Bay, and Bugey 3 experiments
... σ b 2 , (7) where A is the overall normalization, a i is the relative detec- tion efficiency, b is an empirical factor to include the uncer- tainties of the energy scale, i represents the data from three ...
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Interacting partially directed self avoiding walk: scaling limits
... sampled from P ( · | V ⌧ L = 0, G ⌧ L (V ) = L ⌧ L ) ...scaling limits of the upper and lower envelopes of the path much harder to investigate at = c ...the upper and lower envelopes of the ...
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Upper Limits on the Stochastic Gravitational-Wave Background from Advanced LIGO’s First Observing Run
... stochastic signal, we place an upper limit of Ω 0 < 1 . 7 × 10 −7 on the GW energy density, for a spectral index α ¼ 0 . This is ∼33 times more sensitive than previous direct measurements in this frequency band. ...
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Upper Limits on the Stochastic Gravitational Wave Background from Advanced LIGO's First Observing Run
... background from unresolved compact binary coalescences is expected to be particularly ...using data from Advanced LIGO’s first observing run. The data display no evidence of a stochastic ...
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Upper limits on the stochastic gravitational-wave background from Advanced LIGO’s first observing run
... We remove times due to known instrumental artifacts, such as radio frequency (RF) glitching and electronics saturations [? ], or due to simulated signals (referred to as hardware injections) generated by coherently ...
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Setting upper limits on the strength of periodic gravitational waves from PSR J1939+2134 using the first science data from the GEO 600 and LIGO detectors
... targeted searches of systems with an arbi- trary but known phase ...an upper limit on the amplitude of the periodic gravitational wave signal: a Bayesian approach for the time domain analysis and a fre- ...
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Inclusive searches for SUSY from CMS
... of searches for physics beyond the SM in two final ...of data collected in pp collisions at a center of mass energy of 8 TeV in the year of 2012 by the CMS detector [4] at the ...exclusion limits on ...
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Automated measurement of upper thermal limits in small aquatic animals
... assessed from individual movement data ...UTLs from movement ...tracking data to find optimal and objective criteria for detecting the loss of locomotory function at high ...
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Searches for gravitational waves from known pulsars with science run 5 LIGO data
... detection from any of the targets and therefore interpret our results as upper limits on the gravitational wave signal ...interesting limits are those for young pulsars. We present updated ...
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Searches for gravitational waves from known pulsars with science run 5 ligo data
... S5 data for a signal from the Crab pulsar (Abbott et ...of data analyzed was dictated by a timing glitch in the pulsar on 2006 August 23, which was used as the end point of the ...the data and ...
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