Publication data of Baldwin, Jack A.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion1985199019952000200520102015202020250500100015002000250030003500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1985199019952000200520102015202020250122436486001.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion1985199019952000200520102015202020250510152025
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestIntroducing emili: computer aided emission line identificationStructure and Feedback in 30 Doradus II. Structure and Chemical AbundancesStructure and Feedback in 30 Doradus II. Structure and Chemical Abundanc…Star formation in self-gravitating disks in active galactic nuclei. II. Episodic formation of broad line regionsStar formation in self-gravitating disks in active galactic nuclei. II. Episodic fo…s-Process Abundances in Planetary NebulaeStar formation in self-gravitating disks in active galactic nuclei. I. Metallicity gradients in broad line regionsStar formation in self-gravitating disks in active galactic nuclei. I. Metallicity g…The Mass of quasar broad emission line regionsA Magnetically-Supported PDR in M17Implications of infalling Fe II - emitting clouds in AGN: anisotropic propertiesChemical abundances in broad emission line regions: the nitrogen-loud qso 0353-383Chemical abundances in broad emission line regions: the nitrogen-loud qso 0…Testing cosmological variability of the proton to electron mass ratio using the spectrum of PKS 0528-250Testing cosmological variability of the proton to electron mass ratio using the…Locally optimally-emitting clouds and the narrow emission lines in seyfert galaxiesLocally optimally-emitting clouds and the narrow emission lines in seyfert gal…Do the broad emission line clouds see the same continuum that we see?High resolution observations of the qso br1202-0725: deuterium and ionic abundances at redshifts above z=4High resolution observations of the qso br1202-0725: deuterium and ionic a…Quasars as cosmological probes: the ionizing continuum, gas metallicity and the ew-l relationQuasars as cosmological probes: the ionizing continuum, gas metallicity and …The Origin of FeII emission in AGNMetallicities and abundance ratios from quasar broad emission linesAn atlas of computed equivalent widths of quasar broad emission linesLocally optimally emitting clouds and the origin of quasar emission linesClassification parameters for the emission-line spectra of extragalactic objects1985199019952000200520102015202020250500100015002000250030003500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Introducing emili: computer aided emission line identificationStructure and Feedback in 30 Doradus II. Structure and Chemical AbundancesStructure and Feedback in 30 Doradus II. Structure and Chemical Abundanc…Star formation in self-gravitating disks in active galactic nuclei. II. Episodic formation of broad line regionsStar formation in self-gravitating disks in active galactic nuclei. II. Episodic fo…s-Process Abundances in Planetary NebulaeStar formation in self-gravitating disks in active galactic nuclei. I. Metallicity gradients in broad line regionsStar formation in self-gravitating disks in active galactic nuclei. I. Metallicity g…The Mass of quasar broad emission line regionsA Magnetically-Supported PDR in M17Implications of infalling Fe II - emitting clouds in AGN: anisotropic propertiesChemical abundances in broad emission line regions: the nitrogen-loud qso 0353-383Chemical abundances in broad emission line regions: the nitrogen-loud qso 0…Testing cosmological variability of the proton to electron mass ratio using the spectrum of PKS 0528-250Testing cosmological variability of the proton to electron mass ratio using the…Locally optimally-emitting clouds and the narrow emission lines in seyfert galaxiesLocally optimally-emitting clouds and the narrow emission lines in seyfert gal…Do the broad emission line clouds see the same continuum that we see?High resolution observations of the qso br1202-0725: deuterium and ionic abundances at redshifts above z=4High resolution observations of the qso br1202-0725: deuterium and ionic a…Quasars as cosmological probes: the ionizing continuum, gas metallicity and the ew-l relationQuasars as cosmological probes: the ionizing continuum, gas metallicity and …The Origin of FeII emission in AGNMetallicities and abundance ratios from quasar broad emission linesAn atlas of computed equivalent widths of quasar broad emission linesLocally optimally emitting clouds and the origin of quasar emission linesClassification parameters for the emission-line spectra of extragalactic objects1985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average198519901995200020052010201520202025050100150200250