Publication data of Quercellini, Claudia: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2010202020052015202502505007501000125015001750
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201020202005201520250510152025012345
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20022004200620082010201220142016201820202022202405101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestMapping the galactic gravitational potential with peculiar accelerationPeculiar accelerationCosmic Parallax as a probe of late time anisotropic expansionForeground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year dataForeground influence on primordial non-Gaussianity estimates: needlet analy…Affine parameterization of the dark sector: costraints from WMAP5 and SDSSSkewness as a test of the equivalence principlePossibility of Detecting Anisotropic Expansion of the Universe by Very Accurate Astrometry MeasurementsPossibility of Detecting Anisotropic Expansion of the Universe by Very Accura…Affine equation of state from quintessence and k-essence fieldsLate universe dynamics with scale-independent linear couplings in the dark sectorLate universe dynamics with scale-independent linear couplings in the dark s…Lambda-alpha DM: Observational constraints on unified dark matter with constant speed of soundLambda-alpha DM: Observational constraints on unified dark matter with con…Measuring our peculiar velocity on the CMB with high-multipole off-diagonal correlationsMeasuring our peculiar velocity on the CMB with high-multipole off-diagonal c…Testing coupled dark energy with next-generation large-scale observationsThe time evolution of cosmological redshift as a test of dark energyConstraints on coupled dark energy using CMB data from WMAP and SPTConstraints on perfect fluid and scalar field dark energy models from future redshift surveysConstraints on perfect fluid and scalar field dark energy models from future r…Real-time CosmologyConstraints on the interaction and selfinteraction of dark energy from cosmic microwave backgroundConstraints on the interaction and selfinteraction of dark energy from cosmic…N-body simulations for coupled dark energy: Halo mass function and density profilesN-body simulations for coupled dark energy: Halo mass function and density …Tracking and coupled dark energy as seen by WMAP2010202020052015202502505007501000125015001750
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Mapping the galactic gravitational potential with peculiar accelerationPeculiar accelerationCosmic Parallax as a probe of late time anisotropic expansionForeground influence on primordial non-Gaussianity estimates: needlet analysis of WMAP 5-year dataForeground influence on primordial non-Gaussianity estimates: needlet analy…Affine parameterization of the dark sector: costraints from WMAP5 and SDSSSkewness as a test of the equivalence principlePossibility of Detecting Anisotropic Expansion of the Universe by Very Accurate Astrometry MeasurementsPossibility of Detecting Anisotropic Expansion of the Universe by Very Accura…Affine equation of state from quintessence and k-essence fieldsLate universe dynamics with scale-independent linear couplings in the dark sectorLate universe dynamics with scale-independent linear couplings in the dark s…Lambda-alpha DM: Observational constraints on unified dark matter with constant speed of soundLambda-alpha DM: Observational constraints on unified dark matter with con…Measuring our peculiar velocity on the CMB with high-multipole off-diagonal correlationsMeasuring our peculiar velocity on the CMB with high-multipole off-diagonal c…Testing coupled dark energy with next-generation large-scale observationsThe time evolution of cosmological redshift as a test of dark energyConstraints on coupled dark energy using CMB data from WMAP and SPTConstraints on perfect fluid and scalar field dark energy models from future redshift surveysConstraints on perfect fluid and scalar field dark energy models from future r…Real-time CosmologyConstraints on the interaction and selfinteraction of dark energy from cosmic microwave backgroundConstraints on the interaction and selfinteraction of dark energy from cosmic…N-body simulations for coupled dark energy: Halo mass function and density profilesN-body simulations for coupled dark energy: Halo mass function and density …Tracking and coupled dark energy as seen by WMAP2002200420062008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2002200420062008201020122014201620182020202220240255075100125150