Publication data of Wright, Nicholas J.: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion19801985199019952000200520102015202020250200400600800
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications19801990200020102020015304560750246810
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion198019851990199520002005201020152020202505101520
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestIdentification of Galactic Bulge Survey X-ray Sources with Tycho-2 StarsThe Spectral and Temporal Properties of Transient Sources in Early-Type GalaxiesThe Spectral and Temporal Properties of Transient Sources in Early-Type Galax…Photoevaporating Proplyd-like objects in Cygnus OB2IPHAS discoveries of young stars towards Cyg OB2 and its southern peripheryStellar X-ray sources in the Chandra COSMOS surveyThe Massive Star Forming Region Cygnus OB2. I. Chandra catalogue of association membersThe Massive Star Forming Region Cygnus OB2. I. Chandra catalogue of associ…The evolutionary status of sher25 - implications for blue supergiants and the progenitor of sn1987aThe evolutionary status of sher25 - implications for blue supergiants and the …T Tauri candidates and accretion rates using IPHAS: method and application to IC1396T Tauri candidates and accretion rates using IPHAS: method and application …New Galactic supernova remnants discovered with IPHASDeep Chandra survey of the Small Magellanic Cloud. III. Formation efficiency of High-Mass X-ray binariesDeep Chandra survey of the Small Magellanic Cloud. III. Formation efficiency …The shaping of planetary nebula sh 2-188 through interaction with the interstellar mediumThe shaping of planetary nebula sh 2-188 through interaction with the inters…Knots in the Helix Nebula found in H2Physical and mechanical metallurgy of high purity Nb for accelerator cavitiesNeutron-proton elastic scattering between 200 and 500 MeV. 2. Measurement of Rt and AtNeutron-proton elastic scattering between 200 and 500 MeV. 2. Measuremen…The Massive Star Forming Region Cygnus OB2. II. Integrated Stellar Properties and the Star Formation HistoryThe Massive Star Forming Region Cygnus OB2. II. Integrated Stellar Propertie…Joint Efficient Dark-energy Investigation (JEDI): A Candidate implementation of the NASA-DOE Joint Dark Energy Mission (JDEM)Joint Efficient Dark-energy Investigation (JEDI): A Candidate implementation …Efficient Gravitational-wave Glitch Identification from Environmental Data Through Machine LearningEfficient Gravitational-wave Glitch Identification from Environmental Data Th…Neutron - Proton Elastic Scattering Between 200-{MeV} and 500-{MeV}. 3. Phase Shift AnalysisNeutron - Proton Elastic Scattering Between 200-{MeV} and 500-{MeV}. 3. …The stellar activity-rotation relationship and the evolution of stellar dynamos19801985199019952000200520102015202020250200400600800
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Identification of Galactic Bulge Survey X-ray Sources with Tycho-2 StarsThe Spectral and Temporal Properties of Transient Sources in Early-Type GalaxiesThe Spectral and Temporal Properties of Transient Sources in Early-Type Galax…Photoevaporating Proplyd-like objects in Cygnus OB2IPHAS discoveries of young stars towards Cyg OB2 and its southern peripheryStellar X-ray sources in the Chandra COSMOS surveyThe Massive Star Forming Region Cygnus OB2. I. Chandra catalogue of association membersThe Massive Star Forming Region Cygnus OB2. I. Chandra catalogue of associ…The evolutionary status of sher25 - implications for blue supergiants and the progenitor of sn1987aThe evolutionary status of sher25 - implications for blue supergiants and the …T Tauri candidates and accretion rates using IPHAS: method and application to IC1396T Tauri candidates and accretion rates using IPHAS: method and application …New Galactic supernova remnants discovered with IPHASDeep Chandra survey of the Small Magellanic Cloud. III. Formation efficiency of High-Mass X-ray binariesDeep Chandra survey of the Small Magellanic Cloud. III. Formation efficiency …The shaping of planetary nebula sh 2-188 through interaction with the interstellar mediumThe shaping of planetary nebula sh 2-188 through interaction with the inters…Knots in the Helix Nebula found in H2Physical and mechanical metallurgy of high purity Nb for accelerator cavitiesNeutron-proton elastic scattering between 200 and 500 MeV. 2. Measurement of Rt and AtNeutron-proton elastic scattering between 200 and 500 MeV. 2. Measuremen…The Massive Star Forming Region Cygnus OB2. II. Integrated Stellar Properties and the Star Formation HistoryThe Massive Star Forming Region Cygnus OB2. II. Integrated Stellar Propertie…Joint Efficient Dark-energy Investigation (JEDI): A Candidate implementation of the NASA-DOE Joint Dark Energy Mission (JDEM)Joint Efficient Dark-energy Investigation (JEDI): A Candidate implementation …Efficient Gravitational-wave Glitch Identification from Environmental Data Through Machine LearningEfficient Gravitational-wave Glitch Identification from Environmental Data Th…Neutron - Proton Elastic Scattering Between 200-{MeV} and 500-{MeV}. 3. Phase Shift AnalysisNeutron - Proton Elastic Scattering Between 200-{MeV} and 500-{MeV}. 3. …The stellar activity-rotation relationship and the evolution of stellar dynamos19801985199019952000200520102015202020250255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average1980198519901995200020052010201520202025020406080100