Publication data of Manera, Marc: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20042006200820102012201420162018202020222024010002000300040005000
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestEfficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy SurveysEfficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy Surv…The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the low-redshift sampleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…The power spectrum and bispectrum of SDSS DR11 BOSS galaxies – II. Cosmological interpretationThe power spectrum and bispectrum of SDSS DR11 BOSS galaxies – II. Cosm…Large scale structure and the generalised Chaplygin gas as dark energyThe local bias model in the large scale halo distributionLarge scale bias and the inaccuracy of the peak-background splitOn The Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics ExperimentsOn The Upper Bound of Neutrino Masses from Combined Cosmological Obser…COLA with scale-dependent growth: applications to screened modified gravity modelsCOLA with scale-dependent growth: applications to screened modified gravit…Error analysis in cross-correlation of sky maps: Application to the ISW detectionError analysis in cross-correlation of sky maps: Application to the ISW detecti…The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sampleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…Cross-correlation of wmap 3rd year and the sdss dr4 galaxy survey: new evidence for dark energyCross-correlation of wmap 3rd year and the sdss dr4 galaxy survey: new evid…The onion universe: all sky light-cone simulations in shellsCluster number counts dependence on dark energy inhomogeneities and coupling to dark matterCluster number counts dependence on dark energy inhomogeneities and co…L-PICOLA: A parallel code for fast dark matter simulationLarge-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-GaussianityLarge-scale Bias and Efficient Generation of Initial Conditions for Non-Local Pr…The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of normalized growth rate on constraining dark energyThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…The power spectrum and bispectrum of SDSS DR11 BOSS galaxies – I. Bias and gravityThe power spectrum and bispectrum of SDSS DR11 BOSS galaxies – I. Bias a…The clustering of the SDSS main galaxy sample – II. Mock galaxy catalogues and a measurement of the growth of structure from redshift space distortions at $z = 0.15$The clustering of the SDSS main galaxy sample – II. Mock galaxy catalogues …The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at $z = 0.15$The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distanc…20042006200820102012201420162018202020222024010002000300040005000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Efficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy SurveysEfficient Reconstruction of Linear Baryon Acoustic Oscillations in Galaxy Surv…The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: mock galaxy catalogues for the low-redshift sampleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…The power spectrum and bispectrum of SDSS DR11 BOSS galaxies – II. Cosmological interpretationThe power spectrum and bispectrum of SDSS DR11 BOSS galaxies – II. Cosm…Large scale structure and the generalised Chaplygin gas as dark energyThe local bias model in the large scale halo distributionLarge scale bias and the inaccuracy of the peak-background splitOn The Upper Bound of Neutrino Masses from Combined Cosmological Observations and Particle Physics ExperimentsOn The Upper Bound of Neutrino Masses from Combined Cosmological Obser…COLA with scale-dependent growth: applications to screened modified gravity modelsCOLA with scale-dependent growth: applications to screened modified gravit…Error analysis in cross-correlation of sky maps: Application to the ISW detectionError analysis in cross-correlation of sky maps: Application to the ISW detecti…The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: weighing the neutrino mass using the galaxy power spectrum of the CMASS sampleThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…Cross-correlation of wmap 3rd year and the sdss dr4 galaxy survey: new evidence for dark energyCross-correlation of wmap 3rd year and the sdss dr4 galaxy survey: new evid…The onion universe: all sky light-cone simulations in shellsCluster number counts dependence on dark energy inhomogeneities and coupling to dark matterCluster number counts dependence on dark energy inhomogeneities and co…L-PICOLA: A parallel code for fast dark matter simulationLarge-scale Bias and Efficient Generation of Initial Conditions for Non-Local Primordial Non-GaussianityLarge-scale Bias and Efficient Generation of Initial Conditions for Non-Local Pr…The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: single-probe measurements and the strong power of normalized growth rate on constraining dark energyThe clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Su…The power spectrum and bispectrum of SDSS DR11 BOSS galaxies – I. Bias and gravityThe power spectrum and bispectrum of SDSS DR11 BOSS galaxies – I. Bias a…The clustering of the SDSS main galaxy sample – II. Mock galaxy catalogues and a measurement of the growth of structure from redshift space distortions at $z = 0.15$The clustering of the SDSS main galaxy sample – II. Mock galaxy catalogues …The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distance measure at $z = 0.15$The clustering of the SDSS DR7 main Galaxy sample – I. A 4 per cent distanc…200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200420062008201020122014201620182020202220240100200300400500600700