Publication data of Li, Aigen: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion20002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications2000200520102015202020250153045607503691215
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20002005201020152020202505101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestOn Magnesium Sulfide as the Carrier of the 30micron Emission Feature in Evolved StarsOn Magnesium Sulfide as the Carrier of the 30micron Emission Feature in Ev…Physical Dust Models for the Extinction toward Supernova 2014J in M82The Spitzer Spectroscopic Survey of the Small Magellanic Cloud (S4MC): Probing the Physical State of Polycyclic Aromatic Hydrocarbons in a Low-Metallicity EnvironmentThe Spitzer Spectroscopic Survey of the Small Magellanic Cloud (S4MC): Prob…Cr-K Emission Line as a Constraint on the Progenitor Properties of Supernova RemnantsCr-K Emission Line as a Constraint on the Progenitor Properties of Supernova …Modeling the infrared emission from the HR 4796A diskPhase functions and light curves of wide separation extrasolar giant planetsModeling the infrared emission from the HD 141569A diskOn Dust Extinction of Gamma-ray Burst Host GalaxiesVariations in 24 micron morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: New insights into the Hubble sequenceVariations in 24 micron morphologies among galaxies in the Spitzer Infrared …The extinction curve of long gamma-ray burst host galaxies: are they two different types?The extinction curve of long gamma-ray burst host galaxies: are they two diff…Detections of the 2175 Angstrom dust feature at 1.4 <~ z <~ 1.5 from the Sloan Digital Sky SurveyDetections of the 2175 Angstrom dust feature at 1.4 <~ z <~ 1.5 from the …Infrared emission from interstellar dust. 3. The small magellanic cloudOn ultrasmall silicate grains in the diffuse interstellar mediumThe Spectral Energy Distribution of Dust Emission in the Edge-on Spiral Galaxy NGC 4631 as seen with Spitzer and JCMTThe Spectral Energy Distribution of Dust Emission in the Edge-on Spiral Gala…Do the infrared emission features need ultraviolet excitation? the pah model in uv-poor reflection nebulaeDo the infrared emission features need ultraviolet excitation? the pah model i…The Spitzer Survey of the Small Magellanic Cloud: S3MC Imaging and Photometry in the Mid- and Far-Infrared WavebandsThe Spitzer Survey of the Small Magellanic Cloud: S3MC Imaging and Photo…Infrared emission from interstellar dust. I. stochastic heating of small grainsInfrared emission from interstellar dust. 2. The diffuse interstellar mediumInfrared Emission from Interstellar Dust. 4. The Silicate-Graphite-PAH Model in the Post-Spitzer EraInfrared Emission from Interstellar Dust. 4. The Silicate-Graphite-PAH Model i…20002005201020152020202505001000150020002500
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)On Magnesium Sulfide as the Carrier of the 30micron Emission Feature in Evolved StarsOn Magnesium Sulfide as the Carrier of the 30micron Emission Feature in Ev…Physical Dust Models for the Extinction toward Supernova 2014J in M82The Spitzer Spectroscopic Survey of the Small Magellanic Cloud (S4MC): Probing the Physical State of Polycyclic Aromatic Hydrocarbons in a Low-Metallicity EnvironmentThe Spitzer Spectroscopic Survey of the Small Magellanic Cloud (S4MC): Prob…Cr-K Emission Line as a Constraint on the Progenitor Properties of Supernova RemnantsCr-K Emission Line as a Constraint on the Progenitor Properties of Supernova …Modeling the infrared emission from the HR 4796A diskPhase functions and light curves of wide separation extrasolar giant planetsModeling the infrared emission from the HD 141569A diskOn Dust Extinction of Gamma-ray Burst Host GalaxiesVariations in 24 micron morphologies among galaxies in the Spitzer Infrared Nearby Galaxies Survey: New insights into the Hubble sequenceVariations in 24 micron morphologies among galaxies in the Spitzer Infrared …The extinction curve of long gamma-ray burst host galaxies: are they two different types?The extinction curve of long gamma-ray burst host galaxies: are they two diff…Detections of the 2175 Angstrom dust feature at 1.4 <~ z <~ 1.5 from the Sloan Digital Sky SurveyDetections of the 2175 Angstrom dust feature at 1.4 <~ z <~ 1.5 from the …Infrared emission from interstellar dust. 3. The small magellanic cloudOn ultrasmall silicate grains in the diffuse interstellar mediumThe Spectral Energy Distribution of Dust Emission in the Edge-on Spiral Galaxy NGC 4631 as seen with Spitzer and JCMTThe Spectral Energy Distribution of Dust Emission in the Edge-on Spiral Gala…Do the infrared emission features need ultraviolet excitation? the pah model in uv-poor reflection nebulaeDo the infrared emission features need ultraviolet excitation? the pah model i…The Spitzer Survey of the Small Magellanic Cloud: S3MC Imaging and Photometry in the Mid- and Far-Infrared WavebandsThe Spitzer Survey of the Small Magellanic Cloud: S3MC Imaging and Photo…Infrared emission from interstellar dust. I. stochastic heating of small grainsInfrared emission from interstellar dust. 2. The diffuse interstellar mediumInfrared Emission from Interstellar Dust. 4. The Silicate-Graphite-PAH Model in the Post-Spitzer EraInfrared Emission from Interstellar Dust. 4. The Silicate-Graphite-PAH Model i…2000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average200020052010201520202025050100150200250