0000000000852210

AUTHOR

D. Ball

showing 2 related works from this author

The IASLC Lung Cancer Staging Project: Proposals for Revision of the TNM Stage Groupings in the Forthcoming (Eighth) Edition of the TNM Classificatio…

2016

AbstractThe IASLC Staging and Prognostic Factors Committee has collected a new database of 94,708 cases donated from 35 sources in 16 countries around the globe. This has now been analysed by our statistical partners at Cancer Research And Biostatistics and, in close collaboration with the members of the committee proposals have been developed for the T, N, and M categories of the 8th edition of the TNM Classification for lung cancer due to be published late 2016. In this publication we describe the methods used to evaluate the resultant Stage groupings and the proposals put forward for the 8th edition.

0301 basic medicinePulmonary and Respiratory Medicinemedicine.medical_specialtyPathologyLung NeoplasmsStagingMedizinPrognostic factors1102 Cardiovascular Medicine And HaematologyLung cancer; Prognostic factors; Staging03 medical and health sciences0302 clinical medicineSeer programmedicineHumansOncology & CarcinogenesisStage (cooking)Lung cancerNeoplasm Stagingbusiness.industryGeneral surgeryInternational Association for the Study of Lung Cancer Staging and Prognostic Factors Committee Advisory Boards and Participating Institutions1103 Clinical SciencesPrognosismedicine.diseaseInternational Association for the Study of Lung Cancer Staging and Prognostic Factors Committee Advisory Boards and Participating Institutions030104 developmental biologyOncology030220 oncology & carcinogenesisNeoplasm stagingBiostatisticsLung cancer stagingLung cancerbusinessSEER Program
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3C 279 Event Horizon Telescope imaging

2020

3C 279 is an archetypal blazar with a prominent radio jet that show broadband flux density variability across the entire electromagnetic spectrum. We use an ultra-high angular resolution technique - global Very Long Baseline Interferometry (VLBI) at 1.3mm (230GHz) - to resolve the innermost jet of 3C 279 in order to study its fine-scale morphology close to the jet base where highly variable gamma-ray emission is thought to originate, according to various models. The source was observed during four days in April 2017 with the Event Horizon Telescope (EHT) at 230 GHz, including the phased Atacama Large Millimeter/submillimeter Array (ALMA), at an angular resolution of ~20uarcsec (at a redshif…

observational astronomygalactic and extragalactic astronomyAstrophysics and AstronomyInterferometryAstrophysics::High Energy Astrophysical PhenomenaRadio galaxiesPhysicsGalaxiesNatural Sciences
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