Publication data of Peroux, Celine: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications20002005201020152020202502040608010001.534.567.5
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestMetal-rich Damped/sub-Damped Lyman-alpha Quasar Absorbers at z<1A Homogeneous Sample of Sub-DLAs. 4. Global Metallicity EvolutionThe most metal-rich intervening quasar absorber knownThe SINFONI MgII Program for Line Emitters (SIMPLE): Discovering starburts near QSO sight-linesThe SINFONI MgII Program for Line Emitters (SIMPLE): Discovering starburts …The Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of MetalsThe Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of M…The Dust obscuration bias in damped Lyman-alpha systemsThe missing metals problem. 3. How many metals are expelled from galaxies?Signatures of Cool Gas Fueling a Star-Forming Galaxy at Redshift 2.3Absorption systems in the spectra of 66 Z > 4 quasarsEarly stages of nitrogen enrichment in galaxies: Clues from measurements in damped lyman alpha systemsEarly stages of nitrogen enrichment in galaxies: Clues from measurements in…The scuba bright quasar survey (sbqs): 850micron observations of the z>4 sampleThe scuba bright quasar survey (sbqs): 850micron observations of the z>4 s…A homogeneous sample of sub-dlas. 2. Statistical, kinematic and chemical propertiesA homogeneous sample of sub-dlas. 2. Statistical, kinematic and chemical pr…A homogeneous sample of sub-dlas I: construction of the sample and chemical abundance measurementsA homogeneous sample of sub-dlas I: construction of the sample and chemic…New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equival…The Cosmic Baryon and Metal CyclesThe ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass DensityThe ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Ev…A Homogeneous sample of sub-DLAs. 3. Total gas mass Omega(HI+HeII) at z>2A Homogeneous sample of sub-DLAs. 3. Total gas mass Omega(HI+HeII) at z…A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption SystemsA Population of Faint Extended Line Emitters and the Host Galaxies of Optical…The evolution of omega(hi) and the epoch of formation of damped lyman-alpha absorbersThe evolution of omega(hi) and the epoch of formation of damped lyman-alp…20002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Metal-rich Damped/sub-Damped Lyman-alpha Quasar Absorbers at z<1A Homogeneous Sample of Sub-DLAs. 4. Global Metallicity EvolutionThe most metal-rich intervening quasar absorber knownThe SINFONI MgII Program for Line Emitters (SIMPLE): Discovering starburts near QSO sight-linesThe SINFONI MgII Program for Line Emitters (SIMPLE): Discovering starburts …The Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of MetalsThe Role of Sub-damped Lyman-alpha Absorbers in the Cosmic Evolution of M…The Dust obscuration bias in damped Lyman-alpha systemsThe missing metals problem. 3. How many metals are expelled from galaxies?Signatures of Cool Gas Fueling a Star-Forming Galaxy at Redshift 2.3Absorption systems in the spectra of 66 Z > 4 quasarsEarly stages of nitrogen enrichment in galaxies: Clues from measurements in damped lyman alpha systemsEarly stages of nitrogen enrichment in galaxies: Clues from measurements in…The scuba bright quasar survey (sbqs): 850micron observations of the z>4 sampleThe scuba bright quasar survey (sbqs): 850micron observations of the z>4 s…A homogeneous sample of sub-dlas. 2. Statistical, kinematic and chemical propertiesA homogeneous sample of sub-dlas. 2. Statistical, kinematic and chemical pr…A homogeneous sample of sub-dlas I: construction of the sample and chemical abundance measurementsA homogeneous sample of sub-dlas I: construction of the sample and chemic…New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equival…The Cosmic Baryon and Metal CyclesThe ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Evolution of the Neutral Gas Mass DensityThe ESO UVES Advanced Data Products Quasar Sample - II. Cosmological Ev…A Homogeneous sample of sub-DLAs. 3. Total gas mass Omega(HI+HeII) at z>2A Homogeneous sample of sub-DLAs. 3. Total gas mass Omega(HI+HeII) at z…A Population of Faint Extended Line Emitters and the Host Galaxies of Optically Thick QSO Absorption SystemsA Population of Faint Extended Line Emitters and the Host Galaxies of Optical…The evolution of omega(hi) and the epoch of formation of damped lyman-alpha absorbersThe evolution of omega(hi) and the epoch of formation of damped lyman-alp…2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200