Publication data of Jog, Chanda J.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20002005201020152020202502004006008001000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2000200520102015202020250122436486001.22.43.64.86
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20002005201020152020202505101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe Milky Way's dark matter halo appears to be lopsidedLuminosity profiles of advanced mergers of galaxies using 2mass dataGeneration of rotationally dominated galaxies by mergers of pressure-supported progenitorsGeneration of rotationally dominated galaxies by mergers of pressure-suppor…Theoretical determination of HI vertical scale heights in the dwarf galaxies: DDO 154, HoII, IC2574 & NGC2366Theoretical determination of HI vertical scale heights in the dwarf galaxies: D…Global lopsided instability in a purely stellar galactic discDark matter dominance at all radii in the superthin galaxy UGC 7321Origin of disc lopsidedness in the eridanus group of galaxiesSelf-consistent response of a galactic disk to an elliptical perturbation halo potentialSelf-consistent response of a galactic disk to an elliptical perturbation halo po…Constraints on the halo density profile using HI flaring in the outer galaxyLarge scale asymmetry of rotation curves in lopsided spiral galaxiesProgressively more prolate dark matter halo in the outer Galaxy as traced by flaring HI gasProgressively more prolate dark matter halo in the outer Galaxy as traced by …Origin of radially increasing stellar scaleheight in a galactic diskThe Flattened Dark Matter Halo of M31 as Deduced from the Observed HI Scale HeightsThe Flattened Dark Matter Halo of M31 as Deduced from the Observed HI Sc…Lopsided Spiral GalaxiesUnequal - mass galaxy merger remnants: Spiral - like morphology but elliptical - like kinematicsUnequal - mass galaxy merger remnants: Spiral - like morphology but elliptic…Vertical scaleheights in a gravitationally coupled, three-component galactic diskVertical scaleheights in a gravitationally coupled, three-component galactic d…Lopsided spiral galaxies: evidence for gas accretionMultiple minor mergers: Formation of elliptical galaxies and constraints for the growth of spiral disksMultiple minor mergers: Formation of elliptical galaxies and constraints for th…Galaxy mergers with various mass ratios: Properties of remnants20002005201020152020202502004006008001000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The Milky Way's dark matter halo appears to be lopsidedLuminosity profiles of advanced mergers of galaxies using 2mass dataGeneration of rotationally dominated galaxies by mergers of pressure-supported progenitorsGeneration of rotationally dominated galaxies by mergers of pressure-suppor…Theoretical determination of HI vertical scale heights in the dwarf galaxies: DDO 154, HoII, IC2574 & NGC2366Theoretical determination of HI vertical scale heights in the dwarf galaxies: D…Global lopsided instability in a purely stellar galactic discDark matter dominance at all radii in the superthin galaxy UGC 7321Origin of disc lopsidedness in the eridanus group of galaxiesSelf-consistent response of a galactic disk to an elliptical perturbation halo potentialSelf-consistent response of a galactic disk to an elliptical perturbation halo po…Constraints on the halo density profile using HI flaring in the outer galaxyLarge scale asymmetry of rotation curves in lopsided spiral galaxiesProgressively more prolate dark matter halo in the outer Galaxy as traced by flaring HI gasProgressively more prolate dark matter halo in the outer Galaxy as traced by …Origin of radially increasing stellar scaleheight in a galactic diskThe Flattened Dark Matter Halo of M31 as Deduced from the Observed HI Scale HeightsThe Flattened Dark Matter Halo of M31 as Deduced from the Observed HI Sc…Lopsided Spiral GalaxiesUnequal - mass galaxy merger remnants: Spiral - like morphology but elliptical - like kinematicsUnequal - mass galaxy merger remnants: Spiral - like morphology but elliptic…Vertical scaleheights in a gravitationally coupled, three-component galactic diskVertical scaleheights in a gravitationally coupled, three-component galactic d…Lopsided spiral galaxies: evidence for gas accretionMultiple minor mergers: Formation of elliptical galaxies and constraints for the growth of spiral disksMultiple minor mergers: Formation of elliptical galaxies and constraints for th…Galaxy mergers with various mass ratios: Properties of remnants2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2000200520102015202020250255075100125