Publication data of Tatsumi, Daisuke: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19952000200520102015202020250153045607502.557.51012.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion199520002005201020152020202505101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestOptimal Location of Two Laser-interferometric Detectors for Gravitational Wave Backgrounds at 100-MHzOptimal Location of Two Laser-interferometric Detectors for Gravitational Wav…Measurement of optical losses in a high-finesse 300 m filter cavity for broadband quantum noise reduction in gravitational-wave detectorsMeasurement of optical losses in a high-finesse 300 m filter cavity for broadb…Prospects for true calorimetry on Kerr black holes in core-collapse supernovae and mergersProspects for true calorimetry on Kerr black holes in core-collapse supernova…Thermal-noise-limited underground interferometer CLIOCryogenic contamination speed for cryogenic laser interferometric gravitational wave detectorCryogenic contamination speed for cryogenic laser interferometric gravitatio…Online calibration and pre-processing of TAMA dataDetermining the cosmic equation of state using future gravitational wave detectorsDetermining the cosmic equation of state using future gravitational wave det…Ultrastable performance of an underground based laser interferometer observatory for gravitational wavesUltrastable performance of an underground based laser interferometer obser…On detection of black hole quasi-normal ringdowns: Detection efficiency and waveform parameter determination in matched filteringOn detection of black hole quasi-normal ringdowns: Detection efficiency and …Cryogenic measurement of the optical absorption coefficient in sapphire crystals at 1.064 micrometers for the large scale cryogenic gravitational wave telescopeCryogenic measurement of the optical absorption coefficient in sapphire crys…Operational status of TAMA300 with the Seismic Attenuation System (SAS)Estimation of losses in a 300 m filter cavity and quantum noise reduction in the KAGRA gravitational-wave detectorEstimation of losses in a 300 m filter cavity and quantum noise reduction in …Mechanical quality factor of a sapphire fiber at cryogenic temperaturesReduction of thermal fluctuations in a cryogenic laser interferometric gravitational wave detectorReduction of thermal fluctuations in a cryogenic laser interferometric gravita…Cryogenic cooling of a sapphire mirror - suspension for interferometric gravitational wave detectorsCryogenic cooling of a sapphire mirror - suspension for interferometric gravit…Mechanical quality factor of a cryogenic sapphire test mass for gravitational wave detectorsMechanical quality factor of a cryogenic sapphire test mass for gravitational …Laser-interferometric Detectors for Gravitational Wave Background at 100 MHz: Detector Design and SensitivityLaser-interferometric Detectors for Gravitational Wave Background at 100 MH…Search for a stochastic background of 100-MHz gravitational waves with laser interferometersSearch for a stochastic background of 100-MHz gravitational waves with lase…Interferometer design of the KAGRA gravitational wave detector19952000200520102015202020250500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Optimal Location of Two Laser-interferometric Detectors for Gravitational Wave Backgrounds at 100-MHzOptimal Location of Two Laser-interferometric Detectors for Gravitational Wav…Measurement of optical losses in a high-finesse 300 m filter cavity for broadband quantum noise reduction in gravitational-wave detectorsMeasurement of optical losses in a high-finesse 300 m filter cavity for broadb…Prospects for true calorimetry on Kerr black holes in core-collapse supernovae and mergersProspects for true calorimetry on Kerr black holes in core-collapse supernova…Thermal-noise-limited underground interferometer CLIOCryogenic contamination speed for cryogenic laser interferometric gravitational wave detectorCryogenic contamination speed for cryogenic laser interferometric gravitatio…Online calibration and pre-processing of TAMA dataDetermining the cosmic equation of state using future gravitational wave detectorsDetermining the cosmic equation of state using future gravitational wave det…Ultrastable performance of an underground based laser interferometer observatory for gravitational wavesUltrastable performance of an underground based laser interferometer obser…On detection of black hole quasi-normal ringdowns: Detection efficiency and waveform parameter determination in matched filteringOn detection of black hole quasi-normal ringdowns: Detection efficiency and …Cryogenic measurement of the optical absorption coefficient in sapphire crystals at 1.064 micrometers for the large scale cryogenic gravitational wave telescopeCryogenic measurement of the optical absorption coefficient in sapphire crys…Operational status of TAMA300 with the Seismic Attenuation System (SAS)Estimation of losses in a 300 m filter cavity and quantum noise reduction in the KAGRA gravitational-wave detectorEstimation of losses in a 300 m filter cavity and quantum noise reduction in …Mechanical quality factor of a sapphire fiber at cryogenic temperaturesReduction of thermal fluctuations in a cryogenic laser interferometric gravitational wave detectorReduction of thermal fluctuations in a cryogenic laser interferometric gravita…Cryogenic cooling of a sapphire mirror - suspension for interferometric gravitational wave detectorsCryogenic cooling of a sapphire mirror - suspension for interferometric gravit…Mechanical quality factor of a cryogenic sapphire test mass for gravitational wave detectorsMechanical quality factor of a cryogenic sapphire test mass for gravitational …Laser-interferometric Detectors for Gravitational Wave Background at 100 MHz: Detector Design and SensitivityLaser-interferometric Detectors for Gravitational Wave Background at 100 MH…Search for a stochastic background of 100-MHz gravitational waves with laser interferometersSearch for a stochastic background of 100-MHz gravitational waves with lase…Interferometer design of the KAGRA gravitational wave detector19952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1995200020052010201520202025050100150200