Non$Thermal,Phenomenain,Clusters,of,Galaxies,(MA4), · SKA,science,case:, 135,chapters,...
Transcript of Non$Thermal,Phenomenain,Clusters,of,Galaxies,(MA4), · SKA,science,case:, 135,chapters,...
Non-‐Thermal Phenomena in Clusters of Galaxies (MA4)
Research at INAF: theory (plasma astrophysics: cosmic rays, acceleraCon mechanisms, etc. ) and observaCons (in the radio, X-‐rays (soI+hard), γ-‐rays bands). TheoreCcal research would benefit of a more transversal view within MA4, i.e.; plasma astrophysics from clusters of galaxies to supernova remnants and AGN/radio galaxies. INAF should recognize the importance of plasma astrophysics (and theory in general) thus promoCng the coordinaCon of theorists through different channels (PRIN, PhD scholarships, staff permanent posiCons). Golden Age of radioastronomy Pathway to SKA (Italy: full member, through INAF)
The Italian community should be officially involved in SKA pathfinders/precursors to gain the scienCfic and more technical (data analysis and calibraCon…) experCses necessary to use SKA .
What about the research on non-‐thermal phenomena at high energy ? NuSTAR… CTA, Athena… Is the Italian community ready/interested/coordinated?
LOFAR, MWA (now) ASKAP, MeerKAT (1 year Cmescale) SKA1-‐LOW, SKA1-‐MID
Individual INAF researchers take part in Science Working Groups (LOFAR, SKA…). INAF=> Italian SKA Science Coordina3on Board to coordinate the Italian research in view of the definiCon of the SKA Key Science Projects. What acCons so far? How this board interact with the scienCfic community?
Non-‐Thermal Phenomena in Clusters of Galaxies (MA4)
Research at INAF: theory (plasma astrophysics: cosmic rays, acceleraCon mechanisms, etc. ) and observaCons (in the radio, X-‐rays (soI+hard), γ-‐rays bands). TheoreCcal research would benefit of a more transversal view within MA4, i.e.; plasma astrophysics from clusters of galaxies to supernova remnants and AGN/radio galaxies. INAF should recognize the importance of plasma astrophysics (and theory in general) thus promoCng the coordinaCon of theorists through different channels (PRIN, PhD scholarships, staff permanent posiCons). Golden Age of radioastronomy Pathway to SKA (Italy: full member, through INAF)
The Italian community should be officially involved in SKA pathfinders/precursors to gain the scienCfic and more technical (data analysis and calibraCon…) experCses necessary to use SKA .
What about the research on non-‐thermal phenomena at high energy ? NuSTAR… CTA, Athena… Is the Italian community ready/interested/coordinated?
LOFAR, MWA (now) ASKAP, MeerKAT (1 year Cmescale) SKA1-‐LOW, SKA1-‐MID
Individual INAF researchers take part in Science Working Groups (LOFAR, SKA…). INAF=> Italian SKA Science Coordina3on Board to coordinate the Italian research in view of the definiCon of the SKA Key Science Projects. What acCons so far? How this board interact with the scienCfic community?
SKA science case: 135 chapters
First Author Affilia.ons by Country UK IT DE AU NL ZA CN US FR PT CA ES NZ SE HR IN JP KR
LOFAR
LOFAR MeerKAT
MWA ASKAP
LOFAR MeerKAT
MeerKAT
MWA
MWA
MWA MWA MWA LOFAR
LOFAR
Credit: S. Tingay, Sait, Roma 2-‐6 Maggio 2016
Fenomeni non-‐termici in ammassi di galassie (MA4)
Are there interesCng themes
for MA4 (?)
website: hgps://indico.skatelescope.org/event/391/
Non-‐Thermal Phenomena in Clusters of Galaxies (MA4)
Research at INAF: theory (plasma astrophysics: cosmic rays, acceleraCon mechanisms, etc. ) and observaCons (in the radio, X-‐rays (soI+hard), γ-‐rays bands). TheoreCcal research would benefit of a more transversal view within MA4, i.e.; plasma astrophysics from clusters of galaxies to supernova remnants and AGN/radio galaxies. INAF should recognize the importance of plasma astrophysics (and theory in general) thus promoCng the coordinaCon of theorists through different channels (PRIN, PhD scholarships, staff permanent posiCons). Golden Age of radioastronomy Pathway to SKA (Italy: full member, through INAF)
The Italian community should be officially involved in SKA pathfinders/precursors to gain the scienCfic and more technical (data analysis and calibraCon…) experCses necessary to use SKA .
What about the research on non-‐thermal phenomena at high energy ? NuSTAR… CTA, Athena… Is the Italian community ready/interested/coordinated?
LOFAR, MWA (now) ASKAP, MeerKAT (1 year Cmescale) SKA1-‐LOW, SKA1-‐MID
Individual INAF researchers take part in Science Working Groups (LOFAR, SKA…). INAF=> Italian SKA Science Coordina3on Board to coordinate the Italian research in view of the definiCon of the SKA Key Science Projects. What acCons so far? How this board interact with the scienCfic community?