Publication data of Skelton, Rosalind E.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion198019851990199520002005201020152020202502004006008001000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1980199020002010202008162432400246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion198019851990199520002005201020152020202505101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestExploring the chemical link between local ellipticals and their high-redshift progenitorsExploring the chemical link between local ellipticals and their high-redshift pr…Measurement of the 7 Be branching ratioOn the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 $< z <$ 2.8On the importance of using appropriate spectral models to derive physical pr…The Structural Evolution of Milky-Way-like Star-forming Galaxies since z ~ 1.3The effect of dry mergers on the color-magnitude relation of early-type galaxiesThe effect of dry mergers on the color-magnitude relation of early-type galaxi…The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST SurveyThe Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST …Mg-26 (p, n) 26Al and (alpha23, n) 26Al reactionsDense cores in galaxies out to $z$=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fieldsDense cores in galaxies out to $z$=2.5 in SDSS, UltraVISTA, and the five 3D-…Observations of environmental quenching in groups in the $11$ Gyr since $z =$ 2.5: different quenching for central and satellite galaxiesObservations of environmental quenching in groups in the $11$ Gyr since $z…Spatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies at z~1 from 3D-HST: evidence for rapid inside-out assembly of disk galaxiesSpatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies…Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at $z sim 2$Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a La…Direct measurements of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation ratesDirect measurements of dust attenuation in z~1.5 star-forming galaxies from…The Assembly of Milky Way-like Galaxies Since z~2.5Forming Compact Massive GalaxiesHalpha Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar massHalpha Equivalent Widths from the 3D-HST survey: evolution with redshift an…Stellar Kinematics of z ~ 2 Galaxies and the Inside-out Growth of Quiescent GalaxiesStellar Kinematics of z ~ 2 Galaxies and the Inside-out Growth of Quiescent G…The merger-driven evolution of massive galaxiesThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosity Function, Cosmic Star-formation Rate, and the First Mass Density Estimate at 500 MyrThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosi…Constraining the Low-Mass Slope of the Star Formation Sequence at $0.5 < z < 2.5$Constraining the Low-Mass Slope of the Star Formation Sequence at $0.5 < z…198019851990199520002005201020152020202502004006008001000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Exploring the chemical link between local ellipticals and their high-redshift progenitorsExploring the chemical link between local ellipticals and their high-redshift pr…Measurement of the 7 Be branching ratioOn the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7 $< z <$ 2.8On the importance of using appropriate spectral models to derive physical pr…The Structural Evolution of Milky-Way-like Star-forming Galaxies since z ~ 1.3The effect of dry mergers on the color-magnitude relation of early-type galaxiesThe effect of dry mergers on the color-magnitude relation of early-type galaxi…The Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST SurveyThe Radial Distribution of Star Formation in Galaxies at z~1 from the 3D-HST …Mg-26 (p, n) 26Al and (alpha23, n) 26Al reactionsDense cores in galaxies out to $z$=2.5 in SDSS, UltraVISTA, and the five 3D-HST/CANDELS fieldsDense cores in galaxies out to $z$=2.5 in SDSS, UltraVISTA, and the five 3D-…Observations of environmental quenching in groups in the $11$ Gyr since $z =$ 2.5: different quenching for central and satellite galaxiesObservations of environmental quenching in groups in the $11$ Gyr since $z…Spatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies at z~1 from 3D-HST: evidence for rapid inside-out assembly of disk galaxiesSpatially resolved Halpha maps and sizes of 57 strongly star-forming galaxies…Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at $z sim 2$Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a La…Direct measurements of dust attenuation in z~1.5 star-forming galaxies from 3D-HST: Implications for dust geometry and star formation ratesDirect measurements of dust attenuation in z~1.5 star-forming galaxies from…The Assembly of Milky Way-like Galaxies Since z~2.5Forming Compact Massive GalaxiesHalpha Equivalent Widths from the 3D-HST survey: evolution with redshift and dependence on stellar massHalpha Equivalent Widths from the 3D-HST survey: evolution with redshift an…Stellar Kinematics of z ~ 2 Galaxies and the Inside-out Growth of Quiescent GalaxiesStellar Kinematics of z ~ 2 Galaxies and the Inside-out Growth of Quiescent G…The merger-driven evolution of massive galaxiesThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosity Function, Cosmic Star-formation Rate, and the First Mass Density Estimate at 500 MyrThe Most Luminous $z sim$ 9-10 Galaxy Candidates Yet Found: The Luminosi…Constraining the Low-Mass Slope of the Star Formation Sequence at $0.5 < z < 2.5$Constraining the Low-Mass Slope of the Star Formation Sequence at $0.5 < z…19801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average19801985199019952000200520102015202020250255075100125150