Publication data of Salati, Pierre: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19851990199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications198519901995200020052010201520202025040801201602000246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion19851990199520002005201020152020202501020304050
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited Papersrest$gamma$-Ray Lines as a Probe for a Cold Dark Matter HaloA new look at the cosmic ray positron fractionNovel cosmic-ray electron and positron constraints on MeV dark matter particlesNovel cosmic-ray electron and positron constraints on MeV dark matter parti…Clumpiness of dark matter and positron annihilation signal: computing the odds of the galactic lotteryClumpiness of dark matter and positron annihilation signal: computing the o…Detection of neutralino annihilation photons from external galaxiesWhich fraction of the measured cosmic ray anti-protons might be due to neutralino annihilation in the galactic halo?Which fraction of the measured cosmic ray anti-protons might be due to neu…The galactic antiproton spectrum at high energies: Background expectation vs. exotic contributionsThe galactic antiproton spectrum at high energies: Background expectation …Quintessential haloes around galaxiesGalactic halos of fluid dark matterQuintessence and the relic density of neutralinosGalactic secondary positron flux at the EarthAnti-protons from spallations of cosmic rays on interstellar matterPositrons from dark matter annihilation in the galactic halo: Theoretical uncertaintiesPositrons from dark matter annihilation in the galactic halo: Theoretical unce…Constraints on WIMP Dark Matter from the High Energy PAMELA $ar{p}/p$ dataConstraints on WIMP Dark Matter from the High Energy PAMELA $ar{p}/p$ …Anti-deuterons as a signature of supersymmetric dark matterAMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark MatterAMS-02 antiprotons, at last! Secondary astrophysical component and immed…Indirect search for dark matter with micrOMEGAs2.4Antiprotons in cosmic rays from neutralino annihilationCosmic rays below z=30 in a diffusion model: new constraints on propagation parametersCosmic rays below z=30 in a diffusion model: new constraints on propagatio…19851990199520002005201020152020202502000400060008000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)$gamma$-Ray Lines as a Probe for a Cold Dark Matter HaloA new look at the cosmic ray positron fractionNovel cosmic-ray electron and positron constraints on MeV dark matter particlesNovel cosmic-ray electron and positron constraints on MeV dark matter parti…Clumpiness of dark matter and positron annihilation signal: computing the odds of the galactic lotteryClumpiness of dark matter and positron annihilation signal: computing the o…Detection of neutralino annihilation photons from external galaxiesWhich fraction of the measured cosmic ray anti-protons might be due to neutralino annihilation in the galactic halo?Which fraction of the measured cosmic ray anti-protons might be due to neu…The galactic antiproton spectrum at high energies: Background expectation vs. exotic contributionsThe galactic antiproton spectrum at high energies: Background expectation …Quintessential haloes around galaxiesGalactic halos of fluid dark matterQuintessence and the relic density of neutralinosGalactic secondary positron flux at the EarthAnti-protons from spallations of cosmic rays on interstellar matterPositrons from dark matter annihilation in the galactic halo: Theoretical uncertaintiesPositrons from dark matter annihilation in the galactic halo: Theoretical unce…Constraints on WIMP Dark Matter from the High Energy PAMELA $ar{p}/p$ dataConstraints on WIMP Dark Matter from the High Energy PAMELA $ar{p}/p$ …Anti-deuterons as a signature of supersymmetric dark matterAMS-02 antiprotons, at last! Secondary astrophysical component and immediate implications for Dark MatterAMS-02 antiprotons, at last! Secondary astrophysical component and immed…Indirect search for dark matter with micrOMEGAs2.4Antiprotons in cosmic rays from neutralino annihilationCosmic rays below z=30 in a diffusion model: new constraints on propagation parametersCosmic rays below z=30 in a diffusion model: new constraints on propagatio…1985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1985199019952000200520102015202020250100200300400500600