Publication data of de Oliveira-Costa, Angelica: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250500100015002000250030003500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1995200020052010201520202025081624324001.22.43.64.86
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19952000200520102015202020250510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestA high-resolution map of the cosmic microwave background around the north celestial poleA high-resolution map of the cosmic microwave background around the nort…Mapping the CMB. 2. The Second flight of the QMAP experimentMapping the CMB. 1. The First flight of the QMAP experimentA limit on the large angular scale polarization of the cosmic microwave backgroundA limit on the large angular scale polarization of the cosmic microwave backg…Galactic emission at 19 ghzMapping the CMB. 3. Combined analysis of QMAP flightsA New spin on Galactic dustRemoving point sources from cmb mapsThe Quest for microwave Foreground XCross correlation of Tenerife data with galactic templates: Evidence for spinning dust?Cross correlation of Tenerife data with galactic templates: Evidence for spinni…Can the lack of symmetry in the COBE / DMR maps constrain the topology of the universe?Can the lack of symmetry in the COBE / DMR maps constrain the topology of …Cmb multipole measurements in the presence of foregroundsGalactic microwave emission at degree angular scalesE/B decomposition of finite pixelized CMB mapsHow to measure CMB polarization power spectra without losing informationForegrounds and forecasts for the cosmic microwave backgroundA model of diffuse Galactic Radio Emission from 10 MHz to 100 GHzA high resolution foreground cleaned CMB map from WMAPThe Significance of the largest scale CMB fluctuations in WMAP19952000200520102015202020250500100015002000250030003500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)A high-resolution map of the cosmic microwave background around the north celestial poleA high-resolution map of the cosmic microwave background around the nort…Mapping the CMB. 2. The Second flight of the QMAP experimentMapping the CMB. 1. The First flight of the QMAP experimentA limit on the large angular scale polarization of the cosmic microwave backgroundA limit on the large angular scale polarization of the cosmic microwave backg…Galactic emission at 19 ghzMapping the CMB. 3. Combined analysis of QMAP flightsA New spin on Galactic dustRemoving point sources from cmb mapsThe Quest for microwave Foreground XCross correlation of Tenerife data with galactic templates: Evidence for spinning dust?Cross correlation of Tenerife data with galactic templates: Evidence for spinni…Can the lack of symmetry in the COBE / DMR maps constrain the topology of the universe?Can the lack of symmetry in the COBE / DMR maps constrain the topology of …Cmb multipole measurements in the presence of foregroundsGalactic microwave emission at degree angular scalesE/B decomposition of finite pixelized CMB mapsHow to measure CMB polarization power spectra without losing informationForegrounds and forecasts for the cosmic microwave backgroundA model of diffuse Galactic Radio Emission from 10 MHz to 100 GHzA high resolution foreground cleaned CMB map from WMAPThe Significance of the largest scale CMB fluctuations in WMAP19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025050100150200250