Search results for "Ligo"

showing 10 items of 1427 documents

Progress in the characterization of insulin-like peptides in aphids: Immunohistochemical mapping of ILP4.

2021

Aphids were the first animals described as photoperiodic due to their seasonal switch from viviparous parthenogenesis to sexual reproduction (cyclical parthenogenesis) caused by the shortening of the photoperiod in autumn. This switch produces a single sexual generation of oviparous females and males that mate and lay diapausing cold-resistant eggs that can overcome the unfavourable environmental conditions typical of winter in temperate regions. Previous studies have hinted at a possible implication of two insulin-like peptides (ILP1 and ILP4) in the aphid seasonal response, changing their expression levels between different photoperiodic conditions. Moreover, in situ localization of their…

PhotoperiodParthenogenesisDiapauseBiologyBiochemistry03 medical and health sciences0302 clinical medicineCircadian ClocksAnimalsInsulinReproductive systemMolecular Biology030304 developmental biology0303 health sciencesAphidReproductionNeuropeptidesfood and beveragesBrainParthenogenesisbiology.organism_classificationImmunohistochemistryDiapauseSexual reproductionAcyrthosiphon pisumCell biologyPyrrolidonecarboxylic AcidInsect ScienceAphidsInsect HormonesMegoura viciaeInsect ProteinsOviparityPeptidesOligopeptides030217 neurology & neurosurgeryInsect biochemistry and molecular biology
researchProduct

Enhanced effects of variation of the fundamental constants in laser interferometers and application to dark matter detection

2015

We outline new laser interferometer measurements to search for variation of the electromagnetic fine-structure constant $\alpha$ and particle masses (including a non-zero photon mass). We propose a strontium optical lattice clock -- silicon single-crystal cavity interferometer as a novel small-scale platform for these new measurements. Multiple passages of a light beam inside an interferometer enhance the effects due to variation of the fundamental constants by the mean number of passages ($N_{\textrm{eff}} \sim 10^2$ for a large-scale gravitational-wave detector, such as LIGO, Virgo, GEO600 or TAMA300, while $N_{\textrm{eff}} \sim 10^5$ for a strontium clock -- silicon cavity interferomete…

Physics - Instrumentation and DetectorsPhotonField (physics)Atomic Physics (physics.atom-ph)Dark matterPhysics::OpticsFOS: Physical sciences01 natural sciencesPhysics - Atomic Physicslaw.inventionOpticsHigh Energy Physics - Phenomenology (hep-ph)law0103 physical sciencesAstronomical interferometer010306 general physicsPhysics010308 nuclear & particles physicsbusiness.industryAstrophysics::Instrumentation and Methods for AstrophysicsInstrumentation and Detectors (physics.ins-det)LaserGEO600LIGOHigh Energy Physics - PhenomenologyInterferometrybusinessPhysics - OpticsOptics (physics.optics)
researchProduct

GW190412: Observation of a binary-black-hole coalescence with asymmetric masses

2020

LIGO Scientific Collaboration and Virgo Collaboration: et al.

Physics and Astronomy (miscellaneous)AstronomyGravitational wave detection Gravitational wave sources Gravitational waves Astronomical black holesagn discsAstrophysicsdetector: network01 natural sciencesGeneral Relativity and Quantum CosmologyPhysics Particles & Fieldsstar-clustersgravitational waves black holesgravitational waves; black holesAGN DISCSgravitational waves; black holes; LIGO; Virgoblack holegeneral relativityLIGOgravitational waveQCQBPhysicsSettore FIS/01astro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)GRAVITATIONAL WAVE-FORMSPROGENITORSCOMPACT BINARIESblack hole: spinPhysicsPERTURBATIONSgravitational wavesPhysical Sciences[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational wave detectionAstrophysics - High Energy Astrophysical PhenomenaMETALLICITYmass: asymmetrymetallicitydata analysis methodGeneral relativityMERGERSgr-qcAstrophysics::High Energy Astrophysical PhenomenamultipolePREDICTIONSFOS: Physical sciencesgravitational wavesblack holesGeneral Relativity and Quantum Cosmology (gr-qc)Astronomy & Astrophysicsgravitational radiation: direct detectionGravitational wavesGeneral Relativity and Quantum CosmologyTheory of relativityBinary black holeSettore FIS/05 - Astronomia e AstrofisicaAstronomical black holesbinary: coalescence0103 physical sciencesnumerical methodsddc:530STAR-CLUSTERS010306 general physicsnumerical calculationsSTFCAstrophysiqueGravitational wave sourcesScience & Technologymass: solar010308 nuclear & particles physicsGravitational waveVirgogravitational radiationRCUKblack hole: massMass ratioblack holesLIGOEVOLUTIONgravitational radiation detectorBlack holedetector: sensitivityPhysics and Astronomyblack hole: binaryrelativity theorygravitational radiation: emissionmass ratioMultipole expansion[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics and astroparticle physics
researchProduct

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

2018

Made available in DSpace on 2018-11-26T17:45:14Z (GMT). No. of bitstreams: 0 Previous issue date: 2018-03-22 Australian Research Council Council of Scientific and Industrial Research of India Department of Science and Technology, India Science AMP; Engineering Research Board (SERB), India Ministry of Human Resource Development, India Spanish Agencia Estatal de Investigacion Vicepresidencia i Conselleria d'Innovacio, Recerca i Turisme Conselleria d'Educacio i Universitat del Govern de les Illes Balears Conselleria d'Educacio, Investigacio, Cultura i Esport de la Generalitat Valenciana National Science Centre of Poland Swiss National Science Foundation (SNSF) Russian Foundation for Basic Rese…

Physics and Astronomy (miscellaneous)Astrophysics::High Energy Astrophysical PhenomenaAstronomyFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsLIGO-VirgoMagnetar01 natural sciencesGeneral Relativity and Quantum CosmologyGravitational waves long transients LIGOGravitational wavesGeneral Relativity and Quantum CosmologyUPPER LIMITSSearch algorithmSIGNALS0103 physical sciencesWaveformlong transientsHigh Energy PhysicsLIGO010306 general physicsgravitational wave010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSQCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsLIGO-Virgo; gravitational waves; long duration transient[PHYS]Physics [physics]Gravitational wavelong duration transientLIGOgravitational waves; LIGO-Virgo; long duration transient; Physics and Astronomy (miscellaneous)Black holeMODELNeutron starAmplitudegravitational wavesBLACK-HOLEComputingMethodologies_DOCUMENTANDTEXTPROCESSINGRADIATIONNEUTRINOAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

Exploring gravitational-wave detection and parameter inference using deep learning methods

2020

The data that support the findings of this study are openly available at the following URL/DOI: https://arxiv.org/abs/2011.10425.

Physics and Astronomy (miscellaneous)Ciências Naturais::Ciências FísicasFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyBinary black hole0103 physical sciencesblack holeRange (statistics)Chirpparameter inferenceLIGO010306 general physicsPhysicsScience & Technology010308 nuclear & particles physicsGravitational wavebusiness.industryVirgoDeep learningDetectordeep learningLIGOmachine learninggravitational wavesSpectrogramArtificial intelligencebusinessAlgorithmClassical and Quantum Gravity
researchProduct

Classification of gravitational-wave glitches via dictionary learning

2018

We present a new method for the classification of transient noise signals (or glitches) in advanced gravitational-wave interferometers. The method uses learned dictionaries (a supervised machine learning algorithm) for signal denoising, and untrained dictionaries for the final sparse reconstruction and classification. We use a data set of 3000 simulated glitches of three different waveform morphologies, comprising 1000 glitches per morphology. These data are embedded in non-white Gaussian noise to simulate the background noise of advanced LIGO in its broadband configuration. Our classification method yields a 96% accuracy for a large range of initial parameters, showing that learned diction…

Physics and Astronomy (miscellaneous)Noise reductionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Data_CODINGANDINFORMATIONTHEORY01 natural sciencesGeneral Relativity and Quantum CosmologyBackground noiseTransient noisesymbols.namesake0103 physical sciencesWaveformAstrophysics::Solar and Stellar Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Physics010308 nuclear & particles physicsbusiness.industryDetectorAstrophysics::Instrumentation and Methods for AstrophysicsPattern recognitionLIGOGlitchGaussian noisesymbolsArtificial intelligenceAstrophysics - Instrumentation and Methods for Astrophysicsbusiness
researchProduct

Application of dictionary learning to denoise LIGO’s blip noise transients

2020

Data streams of gravitational-wave detectors are polluted by transient noise features, or ``glitches,'' of instrumental and environmental origin. In this work we investigate the use of total variation methods and learned dictionaries to mitigate the effect of those transients in the data. We focus on a specific type of transient, ``blip" glitches, as this is the most common type of glitch present in the LIGO detectors and their waveforms are easy to identify. We randomly select 100 blip glitches scattered in the data from advanced LIGO's O1 run, as provided by the citizen-science project Gravity Spy. Our results show that dictionary-learning methods are a valid approach to model and subtrac…

Physics010308 nuclear & particles physicsData stream miningAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsFOS: Physical sciencesBinary numberGeneral Relativity and Quantum Cosmology (gr-qc)Type (model theory)01 natural sciencesGeneral Relativity and Quantum CosmologyLIGOGlitchNoiseTransient noise0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsTransient (computer programming)010306 general physicsAlgorithmPhysical Review D
researchProduct

New method to observe gravitational waves emitted by core collapse supernovae

2018

While gravitational waves have been detected from mergers of binary black holes and binary neutron stars, signals from core collapse supernovae, the most energetic explosions in the modern Universe, have not been detected yet. Here we present a new method to analyse the data of the LIGO, Virgo, and KAGRA network to enhance the detection efficiency of this category of signals. The method takes advantage of a peculiarity of the gravitational wave signal emitted in the core collapse supernova and it is based on a classification procedure of the time-frequency images of the network data performed by a convolutional neural network trained to perform the task to recognize the signal. We validate …

Physics010308 nuclear & particles physicsGravitational waveAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsType II supernova01 natural sciencesSignalGeneral Relativity and Quantum CosmologyLIGOGravitational wavesGravitational waves; SupernovaeGeneral Relativity and Quantum CosmologySupernovaNeutron starSupernovaeBinary black hole0103 physical sciencesKAGRAAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysics
researchProduct

Total-variation methods for gravitational-wave denoising: Performance tests on Advanced LIGO data

2018

We assess total-variation methods to denoise gravitational-wave signals in real noise conditions, by injecting numerical-relativity waveforms from core-collapse supernovae and binary black hole mergers in data from the first observing run of Advanced LIGO. This work is an extension of our previous investigation where only Gaussian noise was used. Since the quality of the results depends on the regularization parameter of the model, we perform an heuristic search for the value that produces the best results. We discuss various approaches for the selection of this parameter, either based on the optimal, mean, or multiple values, and compare the results of the denoising upon these choices. Mor…

PhysicsArtificial neural network010308 nuclear & particles physicsGravitational waveNoise reductionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum CosmologyLIGOsymbols.namesakeAstrophysics - Solar and Stellar AstrophysicsBinary black holeGaussian noiseLagrange multiplier0103 physical sciencessymbolsWaveformAstrophysics - Instrumentation and Methods for Astrophysics010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)AlgorithmSolar and Stellar Astrophysics (astro-ph.SR)Physical Review D
researchProduct

OPTICAL SPECTROSCOPY OF CANDIDATES IN THE LIGO/VIRGO BINARY MERGER ERROR BOXES

2021

We performed optical spectroscopy of the candidates inside the gravitational wave errorboxes (S190408an, S190425z, S190426c, S190510g, S190728q, S190814bv). The spectral classification of 34 transients observed with the 10.4m Gran Telescopio de Canarias prior to 1 Sep 2019 is presented. We ruled out the association of these candidates with gravitational wave events.

PhysicsBinary numberGeneral MedicineAstrophysicsSpectroscopyLIGORevista Mexicana de Astronomía y Astrofísica Serie de Conferencias
researchProduct