Publication data of de Barros, Stephane: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19701980199020002010202002004006008001000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications1970198019902000201020200612182430012345
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19701980199020002010202002468101214
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestAnalyse des paramètres de résonances du cobalt et du manganèse, induites par des neutrons d'énergie inférieure á 120 keVAnalyse des paramètres de résonances du cobalt et du manganèse, induites …Barriers for pion induced fission near A = 208Spectroscopic factors of negative-parity multiplet states in odd Sn isotopesFission probabilities across the pi nucleon Delta resonanceMass and energy dependence of pion induced fissionDétermination du spin et des paramètres des résonances pour 107, 109 Ag+n, 169 Tm+n, Pt+n de 4 eV À 830 eVDétermination du spin et des paramètres des résonances pour 107, 109 Ag…On Lya emission in z~3-6 UV-selected galaxiesDétermination du spin et des paramètres des résonances pour Cl+n, Cu+n, Ba+n et Nd+nDétermination du spin et des paramètres des résonances pour Cl+n, Cu+n, …A Coherent Study of Emission Lines from Broad-Band Photometry: Specific Star-Formation Rates and [OIII]/H{eta} Ratio at 3 < z < 6A Coherent Study of Emission Lines from Broad-Band Photometry: Specific St…Properties of z~3-6 Lyman break galaxies. II. Testing star formation histories and the SFR-mass relation with ALMA and near-IR spectroscopyProperties of z~3-6 Lyman break galaxies. II. Testing star formation histories …Capture radiative partielle des neutrons de résonance dans le tungstèneBeacons into the Cosmic Dark Ages: Boosted transmission of Ly$alpha$ from UV bright galaxies at $z gtrsim 7$Beacons into the Cosmic Dark Ages: Boosted transmission of Ly$alpha$ from …Variations de la larguer radiative totale Λ γ en fonction du nombre de masse A et de la valeur du spin J = I ± 1 2Variations de la larguer radiative totale Λ γ en fonction du nombre de masse …Kiloparsec-scale gaseous clumps and star formation at z = 5–7On the physical properties of z~6-8 galaxiesProperties of z ~ 3–6 Lyman break galaxies - II. Impact of nebular emission at high redshiftProperties of z ~ 3–6 Lyman break galaxies - II. Impact of nebular emission at…Escape of about five per cent of Lyman-alpha photons from high-redshift star-forming galaxiesEscape of about five per cent of Lyman-alpha photons from high-redshift star…The impact of nebular emission on the ages of z~6 galaxiesThe Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Ly$alpha$ Emission from GalaxiesThe Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fra…19701980199020002010202002004006008001000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Analyse des paramètres de résonances du cobalt et du manganèse, induites par des neutrons d'énergie inférieure á 120 keVAnalyse des paramètres de résonances du cobalt et du manganèse, induites …Barriers for pion induced fission near A = 208Spectroscopic factors of negative-parity multiplet states in odd Sn isotopesFission probabilities across the pi nucleon Delta resonanceMass and energy dependence of pion induced fissionDétermination du spin et des paramètres des résonances pour 107, 109 Ag+n, 169 Tm+n, Pt+n de 4 eV À 830 eVDétermination du spin et des paramètres des résonances pour 107, 109 Ag…On Lya emission in z~3-6 UV-selected galaxiesDétermination du spin et des paramètres des résonances pour Cl+n, Cu+n, Ba+n et Nd+nDétermination du spin et des paramètres des résonances pour Cl+n, Cu+n, …A Coherent Study of Emission Lines from Broad-Band Photometry: Specific Star-Formation Rates and [OIII]/H{eta} Ratio at 3 < z < 6A Coherent Study of Emission Lines from Broad-Band Photometry: Specific St…Properties of z~3-6 Lyman break galaxies. II. Testing star formation histories and the SFR-mass relation with ALMA and near-IR spectroscopyProperties of z~3-6 Lyman break galaxies. II. Testing star formation histories …Capture radiative partielle des neutrons de résonance dans le tungstèneBeacons into the Cosmic Dark Ages: Boosted transmission of Ly$alpha$ from UV bright galaxies at $z gtrsim 7$Beacons into the Cosmic Dark Ages: Boosted transmission of Ly$alpha$ from …Variations de la larguer radiative totale Λ γ en fonction du nombre de masse A et de la valeur du spin J = I ± 1 2Variations de la larguer radiative totale Λ γ en fonction du nombre de masse …Kiloparsec-scale gaseous clumps and star formation at z = 5–7On the physical properties of z~6-8 galaxiesProperties of z ~ 3–6 Lyman break galaxies - II. Impact of nebular emission at high redshiftProperties of z ~ 3–6 Lyman break galaxies - II. Impact of nebular emission at…Escape of about five per cent of Lyman-alpha photons from high-redshift star-forming galaxiesEscape of about five per cent of Lyman-alpha photons from high-redshift star…The impact of nebular emission on the ages of z~6 galaxiesThe Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fraction Using Ly$alpha$ Emission from GalaxiesThe Universe Is Reionizing at z ∼ 7: Bayesian Inference of the IGM Neutral Fra…1970198019902000201020200255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average197019801990200020102020020406080100