Publication data of Decarli, Roberto: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20082010201220142016201820202022202401000200030004000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications200820102012201420162018202020222024025507510012502.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20082010201220142016201820202022202405101520253035
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestThe nature of massive black hole binary candidates: I. Spectral properties and evolutionThe nature of massive black hole binary candidates: I. Spectral properties an…On the geometry of broad emission region in quasarsPredicting Quasar Continua Near Lyman-$alpha$ with Principal Component AnalysisPredicting Quasar Continua Near Lyman-$alpha$ with Principal Component A…Detecting and Characterizing Young Quasars. I. Systemic Redshifts and Proximity Zone MeasurementsDetecting and Characterizing Young Quasars. I. Systemic Redshifts and Proxi…COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the UniverseCOLDz: Shape of the CO Luminosity Function at High Redshift and the Cold G…Detection of atomic carbon [CII] 158 micron and dust emission from a z=7.1 quasar host galaxyDetection of atomic carbon [CII] 158 micron and dust emission from a z=7.1…UV Dust Attenuation in Star-forming Galaxies: II Calibrating the A(UV) vs. L_TIR/L_UV relationUV Dust Attenuation in Star-forming Galaxies: II Calibrating the A(UV) vs. L_T…Bright [CII] and dust emission in three z>6.6 quasar host galaxies observed by ALMABright [CII] and dust emission in three z>6.6 quasar host galaxies observed …An Alma Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived From Ultraviolet-to-radio ModelingAn Alma Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Fie…On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observationsOn the effect of the Cosmic Microwave Background in high-redshift (sub-)mill…Massive black hole binaries: dynamical evolution and observational signaturesBlack hole mass estimates and emission-line properties of a sample of redshift z>6.5 quasarsBlack hole mass estimates and emission-line properties of a sample of redshif…The quasar M_bh - M_host relation through Cosmic Time II - Evidence for evolution from z=3 to the present ageThe quasar M_bh - M_host relation through Cosmic Time II - Evidence for evol…Evidence for non-evolving FeII/MgII ratios in rapidly accreting z~6 QSOsAn ALMA [CII] survey of 27 quasars at z>5.94A systematic search for massive black hole binaries in SDSS spectroscopic sampleA systematic search for massive black hole binaries in SDSS spectroscopic sa…A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Quasar J0252–0503A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Qua…Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7Quantitative Constraints on the Reionization History from the IGM Damping …An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5An 800-million-solar-mass black hole in a significantly neutral Universe at red…20082010201220142016201820202022202401000200030004000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)The nature of massive black hole binary candidates: I. Spectral properties and evolutionThe nature of massive black hole binary candidates: I. Spectral properties an…On the geometry of broad emission region in quasarsPredicting Quasar Continua Near Lyman-$alpha$ with Principal Component AnalysisPredicting Quasar Continua Near Lyman-$alpha$ with Principal Component A…Detecting and Characterizing Young Quasars. I. Systemic Redshifts and Proximity Zone MeasurementsDetecting and Characterizing Young Quasars. I. Systemic Redshifts and Proxi…COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the UniverseCOLDz: Shape of the CO Luminosity Function at High Redshift and the Cold G…Detection of atomic carbon [CII] 158 micron and dust emission from a z=7.1 quasar host galaxyDetection of atomic carbon [CII] 158 micron and dust emission from a z=7.1…UV Dust Attenuation in Star-forming Galaxies: II Calibrating the A(UV) vs. L_TIR/L_UV relationUV Dust Attenuation in Star-forming Galaxies: II Calibrating the A(UV) vs. L_T…Bright [CII] and dust emission in three z>6.6 quasar host galaxies observed by ALMABright [CII] and dust emission in three z>6.6 quasar host galaxies observed …An Alma Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical Properties Derived From Ultraviolet-to-radio ModelingAn Alma Survey of Sub-millimeter Galaxies in the Extended Chandra Deep Fie…On the effect of the Cosmic Microwave Background in high-redshift (sub-)millimeter observationsOn the effect of the Cosmic Microwave Background in high-redshift (sub-)mill…Massive black hole binaries: dynamical evolution and observational signaturesBlack hole mass estimates and emission-line properties of a sample of redshift z>6.5 quasarsBlack hole mass estimates and emission-line properties of a sample of redshif…The quasar M_bh - M_host relation through Cosmic Time II - Evidence for evolution from z=3 to the present ageThe quasar M_bh - M_host relation through Cosmic Time II - Evidence for evol…Evidence for non-evolving FeII/MgII ratios in rapidly accreting z~6 QSOsAn ALMA [CII] survey of 27 quasars at z>5.94A systematic search for massive black hole binaries in SDSS spectroscopic sampleA systematic search for massive black hole binaries in SDSS spectroscopic sa…A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Quasar J0252–0503A Significantly Neutral Intergalactic Medium Around the Luminous z = 7 Qua…Quantitative Constraints on the Reionization History from the IGM Damping Wing Signature in Two Quasars at z > 7Quantitative Constraints on the Reionization History from the IGM Damping …An 800-million-solar-mass black hole in a significantly neutral Universe at redshift 7.5An 800-million-solar-mass black hole in a significantly neutral Universe at red…2008201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average2008201020122014201620182020202220240100200300400500600