Publication data of Costa, Edgardo: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2000200520102015202020250100200300400
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200020052010201520202025081624324001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion200020052010201520202025024681012
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestAge Determination of Fifteen Old to Intermediate-Age Small Magellanic Cloud Star ClustersAge Determination of Fifteen Old to Intermediate-Age Small Magellanic Cloud …First ground-based CCD proper motions for Fornax II: Final resultsNGC 6404 and NGC 6583: Two neglected intermediate-age open clusters located in the Galactic Center directionNGC 6404 and NGC 6583: Two neglected intermediate-age open clusters loc…Photometry of seven overlooked open clusters in the first and fourth galactic quadrantsPhotometry of seven overlooked open clusters in the first and fourth galactic…Photometry of the five marginally studied open clusters Collinder 74, Berkeley 27, Haffner 8, NGC 2509 and VdB-Hagen 4Photometry of the five marginally studied open clusters Collinder 74, Berkele…Three active M dwarfs within 8 pc: L 449-1, L 43-72, & LP 949-15The extended star formation history of the star cluster NGC 2154 in the Large Magellanic CloudThe extended star formation history of the star cluster NGC 2154 in the Larg…The Solar Neighborhood. XXII. Parallax Results from the CTIOPI 0.9m Program: Trigonometric Parallaxes of 64 Nearby Systems with 0 arcs5 $leq mu leq$ 1 arcs0 yr$^{-1}$ (SLOWMO sample)The Solar Neighborhood. XXII. Parallax Results from the CTIOPI 0.9m Program…Ctq 839: candidate for the smallest projected separation binary quasarThe proper motion of the large magellanic cloud: a reanalysisThe edge of the young Galactic discSearching for spiral features in the outer Galactic disk. The field towards WR38 and WR38aSearching for spiral features in the outer Galactic disk. The field towards WR…Old Main-Sequence Turnoff Photometry in the Small Magellanic Cloud. I. Constraints on the Star Formation History in Different FieldsOld Main-Sequence Turnoff Photometry in the Small Magellanic Cloud. I. Cons…The Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9m Program: 20 New Members of the 25 Parsec White Dwarf SampleThe Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9m Program:…Old Main Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star Formation History and Its Spatial GradientsOld Main Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star…The Chemical Enrichment History of the Small Magellanic Cloud and Its GradientsThe Chemical Enrichment History of the Small Magellanic Cloud and Its Gradi…The Solar neighborhood. 13. Parallax results from the CTIOPI 0.9-m program - Stars with mu >= 1.0 second per year (MOTION sample)The Solar neighborhood. 13. Parallax results from the CTIOPI 0.9-m program …Carbon Stars in the Large Magellanic Cloud: Luminosities, Colors, and Implications for the History of Star FormationCarbon Stars in the Large Magellanic Cloud: Luminosities, Colors, and Implica…The Solar Neighborhood. 17. Parallax Results from the CTIOPI 0.9m Program: Twenty New Members of the RECONS 10 Parsec SampleThe Solar Neighborhood. 17. Parallax Results from the CTIOPI 0.9m Program: …2000200520102015202020250100200300400
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Age Determination of Fifteen Old to Intermediate-Age Small Magellanic Cloud Star ClustersAge Determination of Fifteen Old to Intermediate-Age Small Magellanic Cloud …First ground-based CCD proper motions for Fornax II: Final resultsNGC 6404 and NGC 6583: Two neglected intermediate-age open clusters located in the Galactic Center directionNGC 6404 and NGC 6583: Two neglected intermediate-age open clusters loc…Photometry of seven overlooked open clusters in the first and fourth galactic quadrantsPhotometry of seven overlooked open clusters in the first and fourth galactic…Photometry of the five marginally studied open clusters Collinder 74, Berkeley 27, Haffner 8, NGC 2509 and VdB-Hagen 4Photometry of the five marginally studied open clusters Collinder 74, Berkele…Three active M dwarfs within 8 pc: L 449-1, L 43-72, & LP 949-15The extended star formation history of the star cluster NGC 2154 in the Large Magellanic CloudThe extended star formation history of the star cluster NGC 2154 in the Larg…The Solar Neighborhood. XXII. Parallax Results from the CTIOPI 0.9m Program: Trigonometric Parallaxes of 64 Nearby Systems with 0 arcs5 $leq mu leq$ 1 arcs0 yr$^{-1}$ (SLOWMO sample)The Solar Neighborhood. XXII. Parallax Results from the CTIOPI 0.9m Program…Ctq 839: candidate for the smallest projected separation binary quasarThe proper motion of the large magellanic cloud: a reanalysisThe edge of the young Galactic discSearching for spiral features in the outer Galactic disk. The field towards WR38 and WR38aSearching for spiral features in the outer Galactic disk. The field towards WR…Old Main-Sequence Turnoff Photometry in the Small Magellanic Cloud. I. Constraints on the Star Formation History in Different FieldsOld Main-Sequence Turnoff Photometry in the Small Magellanic Cloud. I. Cons…The Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9m Program: 20 New Members of the 25 Parsec White Dwarf SampleThe Solar Neighborhood. XXI. Parallax Results from the CTIOPI 0.9m Program:…Old Main Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star Formation History and Its Spatial GradientsOld Main Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star…The Chemical Enrichment History of the Small Magellanic Cloud and Its GradientsThe Chemical Enrichment History of the Small Magellanic Cloud and Its Gradi…The Solar neighborhood. 13. Parallax results from the CTIOPI 0.9-m program - Stars with mu >= 1.0 second per year (MOTION sample)The Solar neighborhood. 13. Parallax results from the CTIOPI 0.9-m program …Carbon Stars in the Large Magellanic Cloud: Luminosities, Colors, and Implications for the History of Star FormationCarbon Stars in the Large Magellanic Cloud: Luminosities, Colors, and Implica…The Solar Neighborhood. 17. Parallax Results from the CTIOPI 0.9m Program: Twenty New Members of the RECONS 10 Parsec SampleThe Solar Neighborhood. 17. Parallax Results from the CTIOPI 0.9m Program: …2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025020406080