Publication data of Sivarani, Thirupathi: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2000200520102015202020250500100015002000
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-citaion2000200520102015202020250510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestOn the genealogy of the Orphan StreamEstimation of stellar atmospheric parameters from SDSS/SEGUE spectraThe [Fe/H], [C/Fe], and [alpha/Fe] distributions of the Bootes I Dwarf Spheroidal GalaxyThe [Fe/H], [C/Fe], and [alpha/Fe] distributions of the Bootes I Dwarf Spheroid…The SEGUE Stellar Parameter Pipeline. IV. Validation with an Extended Sample of Galactic Globular and Open ClustersThe SEGUE Stellar Parameter Pipeline. IV. Validation with an Extended Sampl…First stars. 10. The nature of three unevolved Carbon-Enhanced Metal-Poor starsFirst stars. 10. The nature of three unevolved Carbon-Enhanced Metal-Poor st…First Stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876--032First Stars XI. Chemical composition of the extremely metal-poor dwarfs in th…Carbon-Enhanced Metal-Poor Stars. III. Main-Sequence Turn-Off Stars from the SDSS/SEGUE SampleCarbon-Enhanced Metal-Poor Stars. III. Main-Sequence Turn-Off Stars from th…Carbon-Enhanced Metal-Poor Stars in the Inner and Outer Halo Components of the Milky WayCarbon-Enhanced Metal-Poor Stars in the Inner and Outer Halo Components …From First Stars to the Spite Plateau: a Possible Reconciliation of Halo Stars Observations with Predictions from Big Bang NucleosynthesisFrom First Stars to the Spite Plateau: a Possible Reconciliation of Halo Stars O…First stars 4. CS 29497-030: Evidence for operation of the s-process at very low metallicityFirst stars 4. CS 29497-030: Evidence for operation of the s-process at very l…Mapping the Galactic Halo VIII: Quantifying substructureThe Case for the Dual Halo of the Milky WayThe Frequency of Carbon-Enhanced Metal-Poor Stars in the Galaxy from the HERES sampleThe Frequency of Carbon-Enhanced Metal-Poor Stars in the Galaxy from the …The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field StarsThe SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution S…The SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open ClustersThe SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular an…The SEGUE Stellar Parameter Pipeline. 1. Description and Initial Validation TestsThe SEGUE Stellar Parameter Pipeline. 1. Description and Initial Validation Tes…First stars. 7. Lithium in extremely metal poor dwarfsTwo stellar components in the halo of the Milky WayThe metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities and lithium abundancesThe metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities a…2000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)On the genealogy of the Orphan StreamEstimation of stellar atmospheric parameters from SDSS/SEGUE spectraThe [Fe/H], [C/Fe], and [alpha/Fe] distributions of the Bootes I Dwarf Spheroidal GalaxyThe [Fe/H], [C/Fe], and [alpha/Fe] distributions of the Bootes I Dwarf Spheroid…The SEGUE Stellar Parameter Pipeline. IV. Validation with an Extended Sample of Galactic Globular and Open ClustersThe SEGUE Stellar Parameter Pipeline. IV. Validation with an Extended Sampl…First stars. 10. The nature of three unevolved Carbon-Enhanced Metal-Poor starsFirst stars. 10. The nature of three unevolved Carbon-Enhanced Metal-Poor st…First Stars XI. Chemical composition of the extremely metal-poor dwarfs in the binary CS 22876--032First Stars XI. Chemical composition of the extremely metal-poor dwarfs in th…Carbon-Enhanced Metal-Poor Stars. III. Main-Sequence Turn-Off Stars from the SDSS/SEGUE SampleCarbon-Enhanced Metal-Poor Stars. III. Main-Sequence Turn-Off Stars from th…Carbon-Enhanced Metal-Poor Stars in the Inner and Outer Halo Components of the Milky WayCarbon-Enhanced Metal-Poor Stars in the Inner and Outer Halo Components …From First Stars to the Spite Plateau: a Possible Reconciliation of Halo Stars Observations with Predictions from Big Bang NucleosynthesisFrom First Stars to the Spite Plateau: a Possible Reconciliation of Halo Stars O…First stars 4. CS 29497-030: Evidence for operation of the s-process at very low metallicityFirst stars 4. CS 29497-030: Evidence for operation of the s-process at very l…Mapping the Galactic Halo VIII: Quantifying substructureThe Case for the Dual Halo of the Milky WayThe Frequency of Carbon-Enhanced Metal-Poor Stars in the Galaxy from the HERES sampleThe Frequency of Carbon-Enhanced Metal-Poor Stars in the Galaxy from the …The SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution Spectroscopy of SDSS/SEGUE Field StarsThe SEGUE Stellar Parameter Pipeline. III. Comparison with High-Resolution S…The SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular and Open ClustersThe SEGUE Stellar Parameter Pipeline. II. Validation with Galactic Globular an…The SEGUE Stellar Parameter Pipeline. 1. Description and Initial Validation TestsThe SEGUE Stellar Parameter Pipeline. 1. Description and Initial Validation Tes…First stars. 7. Lithium in extremely metal poor dwarfsTwo stellar components in the halo of the Milky WayThe metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities and lithium abundancesThe metal-poor end of the Spite plateau. 1: Stellar parameters, metallicities a…2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200250