Publication data of Viana, Pedro T.P.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1995200020052010201520202025050010001500200025003000
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraintsThe XMM Cluster Survey: Forecasting cosmological and cluster scaling-relatio…Open cold dark matter modelsMeasuring alpha in the early universe. 1. CMB temperature, large scale structure and fisher matrix analysisMeasuring alpha in the early universe. 1. CMB temperature, large scale struc…Cold dark matter models with high baryon contentThe XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Galaxies at high redshiftThe XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Gal…Pursuing parameters for critical density dark matter modelsConstraining the matter power spectrum normalization using the SDSS/RASS and reflex cluster surveysConstraining the matter power spectrum normalization using the SDSS/RASS…Perturbation evolution in cosmologies with a decaying cosmological constantThe XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XMMXCS J2215.9-1738 at z=1.46The XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XM…Early assembly of the most massive galaxiesLooking for a varying alpha in the cosmic microwave backgroundMeasuring alpha in the early universe: cmb polarization, reionization and the fisher matrix analysisMeasuring alpha in the early universe: cmb polarization, reionization and the …Wmap constraints on varying alpha and the promise of reionizationThe XMM Cluster Survey: A Massive Galaxy Cluster at z=1.45Cold dark matter models with a cosmological constantEarly universe constraints on a time varying fine structure constantNext Generation Cosmology: Constraints from the Euclid Galaxy Cluster SurveyNext Generation Cosmology: Constraints from the Euclid Galaxy Cluster Surv…Galaxy cluster abundance evolution and cosmological parametersThe Cluster abundance in flat and open cosmologies1995200020052010201520202025050010001500200025003000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The XMM Cluster Survey: Forecasting cosmological and cluster scaling-relation parameter constraintsThe XMM Cluster Survey: Forecasting cosmological and cluster scaling-relatio…Open cold dark matter modelsMeasuring alpha in the early universe. 1. CMB temperature, large scale structure and fisher matrix analysisMeasuring alpha in the early universe. 1. CMB temperature, large scale struc…Cold dark matter models with high baryon contentThe XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Galaxies at high redshiftThe XMM Cluster Survey: The build up of stellar mass in Brightest Cluster Gal…Pursuing parameters for critical density dark matter modelsConstraining the matter power spectrum normalization using the SDSS/RASS and reflex cluster surveysConstraining the matter power spectrum normalization using the SDSS/RASS…Perturbation evolution in cosmologies with a decaying cosmological constantThe XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XMMXCS J2215.9-1738 at z=1.46The XMM Cluster Survey: Active Galactic Nuclei and Starburst Galaxies in XM…Early assembly of the most massive galaxiesLooking for a varying alpha in the cosmic microwave backgroundMeasuring alpha in the early universe: cmb polarization, reionization and the fisher matrix analysisMeasuring alpha in the early universe: cmb polarization, reionization and the …Wmap constraints on varying alpha and the promise of reionizationThe XMM Cluster Survey: A Massive Galaxy Cluster at z=1.45Cold dark matter models with a cosmological constantEarly universe constraints on a time varying fine structure constantNext Generation Cosmology: Constraints from the Euclid Galaxy Cluster SurveyNext Generation Cosmology: Constraints from the Euclid Galaxy Cluster Surv…Galaxy cluster abundance evolution and cosmological parametersThe Cluster abundance in flat and open cosmologies19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19952000200520102015202020250255075100125150175