Publication data of Lentati, Lindley: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2010201220142016201820202022202402004006008001000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20102012201420162018202020222024051015202501.534.567.5
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestUsing Swarm Intelligence To Accelerate Pulsar Timing AnalysisCO(1–0) line imaging of massive star-forming disc galaxies at z=1.5–2.2Proper motions of 15 pulsars: a comparison between Bayesian and frequentist algorithmsProper motions of 15 pulsars: a comparison between Bayesian and frequentis…Variations in the Fundamental constants in the QSO Host J1148+5251 at z = 6.4 and the BR1202-0725 System at z = 4.7Variations in the Fundamental constants in the QSO Host J1148+5251 at z =…Bayesian power spectrum estimation at the Epoch of ReionizationBayesian Estimation of Non-Gaussianity in Pulsar Timing AnalysisWeighing The Evidence For A Gravitational-Wave Background In The First International Pulsar Timing Array Data ChallengeWeighing The Evidence For A Gravitational-Wave Background In The First Int…Field and Globular Cluster LMXBs in NGC 4278Contamination of the Epoch of Reionization power spectrum in the presence of foregroundsContamination of the Epoch of Reionization power spectrum in the presence …The anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed by ALMAThe anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed…Robust Estimation of Scattering in Pulsar Timing AnalysisModel-based asymptotically optimal dispersion measure correction for pulsar timingModel-based asymptotically optimal dispersion measure correction for pulsar …Timing of young radio pulsars – II. Braking indices and their interpretationEvidence for a clumpy, rotating gas disk in a submillimeter galaxy at z=4All correlations must die: Assessing the significance of a stochastic gravitational-wave background in pulsar-timing arraysAll correlations must die: Assessing the significance of a stochastic gravitatio…Timing of young radio pulsars – I. Timing noise, periodic modulation, and proper motionTiming of young radio pulsars – I. Timing noise, periodic modulation, and pro…Star Formation and Gas Kinematics of Quasar Host Galaxies at $z sim$ 6: New Insights from ALMAStar Formation and Gas Kinematics of Quasar Host Galaxies at $z sim$ 6: Ne…Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing dataHyper-efficient model-independent Bayesian method for the analysis of pulsa…TempoNest: A Bayesian approach to pulsar timing analysis2010201220142016201820202022202402004006008001000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Using Swarm Intelligence To Accelerate Pulsar Timing AnalysisCO(1–0) line imaging of massive star-forming disc galaxies at z=1.5–2.2Proper motions of 15 pulsars: a comparison between Bayesian and frequentist algorithmsProper motions of 15 pulsars: a comparison between Bayesian and frequentis…Variations in the Fundamental constants in the QSO Host J1148+5251 at z = 6.4 and the BR1202-0725 System at z = 4.7Variations in the Fundamental constants in the QSO Host J1148+5251 at z =…Bayesian power spectrum estimation at the Epoch of ReionizationBayesian Estimation of Non-Gaussianity in Pulsar Timing AnalysisWeighing The Evidence For A Gravitational-Wave Background In The First International Pulsar Timing Array Data ChallengeWeighing The Evidence For A Gravitational-Wave Background In The First Int…Field and Globular Cluster LMXBs in NGC 4278Contamination of the Epoch of Reionization power spectrum in the presence of foregroundsContamination of the Epoch of Reionization power spectrum in the presence …The anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed by ALMAThe anatomy of an extreme starburst within 1.3Gyr of the Big Bang revealed…Robust Estimation of Scattering in Pulsar Timing AnalysisModel-based asymptotically optimal dispersion measure correction for pulsar timingModel-based asymptotically optimal dispersion measure correction for pulsar …Timing of young radio pulsars – II. Braking indices and their interpretationEvidence for a clumpy, rotating gas disk in a submillimeter galaxy at z=4All correlations must die: Assessing the significance of a stochastic gravitational-wave background in pulsar-timing arraysAll correlations must die: Assessing the significance of a stochastic gravitatio…Timing of young radio pulsars – I. Timing noise, periodic modulation, and proper motionTiming of young radio pulsars – I. Timing noise, periodic modulation, and pro…Star Formation and Gas Kinematics of Quasar Host Galaxies at $z sim$ 6: New Insights from ALMAStar Formation and Gas Kinematics of Quasar Host Galaxies at $z sim$ 6: Ne…Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing dataHyper-efficient model-independent Bayesian method for the analysis of pulsa…TempoNest: A Bayesian approach to pulsar timing analysis201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average201020122014201620182020202220240255075100125150175