Publication data of Papadopoulos, Padelis P.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion2000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2000200520102015202020250153045607501.534.567.5
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Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestCO Spectral Line Energy Distributions of IR-luminous galaxies and AGNDetection of CO J = 1-0 in the z = 3.79 radio galaxy 4C60.07Molecular gas in spiral galaxies: A New warm phase at large galactocentric distances?Molecular gas in spiral galaxies: A New warm phase at large galactocentric di…Molecular gas, CO, and star formation in galaxies: emergent empirical relations, feedback, and the evolution of very gas-rich systemsMolecular gas, CO, and star formation in galaxies: emergent empirical relatio…Resolved nuclear co(1-0) emission in apm08279+5255: gravitational lensing by a naked cusp?Resolved nuclear co(1-0) emission in apm08279+5255: gravitational lensing …HCN versus HCO+ as dense molecular gas mass tracer in Luminous Infrared GalaxiesHCN versus HCO+ as dense molecular gas mass tracer in Luminous Infrared …The CI lines as tracers of molecular gas, and their prospects at high redshiftsThe molecular gas in Luminous Infrared Galaxies II: extreme physical conditions, and their effects on the X_{co} factorThe molecular gas in Luminous Infrared Galaxies II: extreme physical conditi…The molecular gas in Luminous Infrared Galaxies I: CO lines, extreme physical conditions, and their driversThe molecular gas in Luminous Infrared Galaxies I: CO lines, extreme physica…Gas, dust and stars in the SCUBA galaxy, SMM J02399-0136: the EVLA reveals a colossal galactic nurseryGas, dust and stars in the SCUBA galaxy, SMM J02399-0136: the EVLA reveal…A massive reservoir of low-excitation molecular gas at high redshiftIncorporating the molecular gas phase in galaxy-size numerical simulations: first applications in dwarf galaxiesIncorporating the molecular gas phase in galaxy-size numerical simulations: f…The ISM in distant star-forming galaxies: Turbulent pressure, fragmentation and cloud scaling relations in a dense gas disk at z=2.3The ISM in distant star-forming galaxies: Turbulent pressure, fragmentation a…Molecular Gas Disk Structures around AGNsMolecular gas in extreme star-forming environments: The starbursts Arp220 and NGC 6240 as case studiesMolecular gas in extreme star-forming environments: The starbursts Arp220 …A cosmic-ray dominated ISM in Ultra Luminous Infrared Galaxies: new initial conditions for star formationA cosmic-ray dominated ISM in Ultra Luminous Infrared Galaxies: new initial …Co(4-3) and dust emission in two powerful high-z radio galaxies, and co lines at high redshiftsCo(4-3) and dust emission in two powerful high-z radio galaxies, and co lines …Tracing the molecular gas in distant submillimetre galaxies via CO(1-0) imaging with the EVLATracing the molecular gas in distant submillimetre galaxies via CO(1-0) imagi…Optimal local implementation of nonlocal quantum gates2000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)CO Spectral Line Energy Distributions of IR-luminous galaxies and AGNDetection of CO J = 1-0 in the z = 3.79 radio galaxy 4C60.07Molecular gas in spiral galaxies: A New warm phase at large galactocentric distances?Molecular gas in spiral galaxies: A New warm phase at large galactocentric di…Molecular gas, CO, and star formation in galaxies: emergent empirical relations, feedback, and the evolution of very gas-rich systemsMolecular gas, CO, and star formation in galaxies: emergent empirical relatio…Resolved nuclear co(1-0) emission in apm08279+5255: gravitational lensing by a naked cusp?Resolved nuclear co(1-0) emission in apm08279+5255: gravitational lensing …HCN versus HCO+ as dense molecular gas mass tracer in Luminous Infrared GalaxiesHCN versus HCO+ as dense molecular gas mass tracer in Luminous Infrared …The CI lines as tracers of molecular gas, and their prospects at high redshiftsThe molecular gas in Luminous Infrared Galaxies II: extreme physical conditions, and their effects on the X_{co} factorThe molecular gas in Luminous Infrared Galaxies II: extreme physical conditi…The molecular gas in Luminous Infrared Galaxies I: CO lines, extreme physical conditions, and their driversThe molecular gas in Luminous Infrared Galaxies I: CO lines, extreme physica…Gas, dust and stars in the SCUBA galaxy, SMM J02399-0136: the EVLA reveals a colossal galactic nurseryGas, dust and stars in the SCUBA galaxy, SMM J02399-0136: the EVLA reveal…A massive reservoir of low-excitation molecular gas at high redshiftIncorporating the molecular gas phase in galaxy-size numerical simulations: first applications in dwarf galaxiesIncorporating the molecular gas phase in galaxy-size numerical simulations: f…The ISM in distant star-forming galaxies: Turbulent pressure, fragmentation and cloud scaling relations in a dense gas disk at z=2.3The ISM in distant star-forming galaxies: Turbulent pressure, fragmentation a…Molecular Gas Disk Structures around AGNsMolecular gas in extreme star-forming environments: The starbursts Arp220 and NGC 6240 as case studiesMolecular gas in extreme star-forming environments: The starbursts Arp220 …A cosmic-ray dominated ISM in Ultra Luminous Infrared Galaxies: new initial conditions for star formationA cosmic-ray dominated ISM in Ultra Luminous Infrared Galaxies: new initial …Co(4-3) and dust emission in two powerful high-z radio galaxies, and co lines at high redshiftsCo(4-3) and dust emission in two powerful high-z radio galaxies, and co lines …Tracing the molecular gas in distant submillimetre galaxies via CO(1-0) imaging with the EVLATracing the molecular gas in distant submillimetre galaxies via CO(1-0) imagi…Optimal local implementation of nonlocal quantum gates2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200250