{"id":1671,"date":"2019-02-01T16:05:54","date_gmt":"2019-02-01T15:05:54","guid":{"rendered":"https:\/\/www.ict.inaf.it\/computing\/?page_id=1671"},"modified":"2020-12-02T20:38:12","modified_gmt":"2020-12-02T19:38:12","slug":"projects-reports","status":"publish","type":"page","link":"https:\/\/www.ict.inaf.it\/computing\/projects-reports\/","title":{"rendered":"Projects Reports"},"content":{"rendered":"

[et_pb_section admin_label=”Sezione” fullwidth=”off” specialty=”on”][et_pb_column type=”1_4″][et_pb_sidebar admin_label=”Barra Laterale” orientation=”left” area=”et_pb_widget_area_1″ background_layout=”light” remove_border=”off”]<\/p>\n

 <\/p>\n

[\/et_pb_sidebar][\/et_pb_column][et_pb_column type=”3_4″ specialty_columns=”3″][et_pb_row_inner admin_label=”Riga”][et_pb_column_inner type=”4_4″ saved_specialty_column_type=”3_4″][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n

Call 1 Project Reports<\/strong><\/h1>\n

[\/et_pb_text][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n\n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Simulating galaxy clusters at high resolution<\/td>Veronica Biffi<\/td>A00<\/td>PDF<\/a><\/td>\n<\/tr>\n
Deceleration of relativistic jets<\/td>Gianluigi Bodo<\/td>A01<\/td>PDF<\/a><\/td>\n<\/tr>\n
Formation of star clusters: how common is infant rotation?<\/td>Michela Mapelli
\n
\n<\/td>		A02<\/td><\/td>\n<\/tr>\n
Mechanical feedback and backflows in early-type galaxies.<\/td>Vincenzo Antonuccio
\n<\/td>		A03<\/td>PDF<\/a><\/td>\n<\/tr>\n
The impact of stellar dynamics on gravitational wave sources<\/td>Mario Spera
\n<\/td>		A04<\/td>PDF<\/a><\/td>\n<\/tr>\n
The inner parsecs of our Galaxy: star formation and its environment<\/td>Alessandro Ballone<\/td>A05<\/td>PDF<\/a><\/td>\n<\/tr>\n
DEMNUni Covariances<\/td>Carmelita Carbone<\/td>A06<\/td>PDF<\/a><\/td>\n<\/tr>\n
Effects of the feedback of stellar winds and supernovae in young globular clusters<\/td>Francesco Calura<\/td>B00<\/td>PDF<\/a><\/td>\n<\/tr>\n
Three-dimensional hydrodynamical
\n simulations of
\n supernova explosions in the smallest Milky Way satellites<\/td>		 Donatella Romano<\/td>B01<\/td>PDF<\/a><\/td>\n<\/tr>\n
Instabilities, magnetic reconnection and particle acceleration in Blazar jets<\/td>Claudia Raitieri<\/td>B02<\/td>PDF<\/a><\/td>\n<\/tr>\n
Effects of intense flaring activity on accretion disk of Classical T Tauri Stars<\/td>Salvatore Colombo<\/td>B03<\/td>PDF<\/a><\/td>\n<\/tr>\n
Vlasov simulations of reconnection events and comparison with MMS<\/td>Francesco Califano<\/td>B04<\/td>PDF<\/a><\/td>\n<\/tr>\n
Simulations of disk galaxies: the effect of AGN feedback<\/td>Stefano Borgani<\/td>B05<\/td>PDF<\/a><\/td>\n<\/tr>\n
DUSTGRAIN Follow Up<\/td>Marco Baldi<\/td>B09<\/td>PDF<\/a><\/td>\n<\/tr>\n
Post processing and visualisation of galaxy clusters<\/td>Giuliano Taffoni<\/td>Test<\/td>Test Class. Report not requested
\n<\/td>\n<\/tr>\n
Post processing and visualisation of galaxy clusters<\/td>Stefano Borgani<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
AnharmoniCaOs test<\/td>Giacomo Mulas<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
Radiative transfer in exoplanetary atmospheres<\/td>Giambattista Aresu<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
Dust in the Universe <\/td>Sergio Cristallo<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n\n

[\/et_pb_text][\/et_pb_column_inner][\/et_pb_row_inner][et_pb_row_inner admin_label=”Riga”][et_pb_column_inner type=”4_4″ saved_specialty_column_type=”3_4″][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n

Call 2 Project Reports<\/strong><\/h1>\n

[\/et_pb_text][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n\n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Jet\/ambient interaction in low power radiosources
\n<\/td>		Silvano Massaglia<\/td>A07<\/td>PDF<\/a><\/td>\n<\/tr>\n
GESBAYES<\/td>Alessandro Lanzafame<\/td>A09<\/td>PDF<\/a><\/td>\n<\/tr>\n
GRMHD simulation of the binary neutron star
\n<\/td>		Riccardo Ciolfi
\n
\n<\/td>		A11<\/td>PDF<\/a><\/td>\n<\/tr>\n
3D MHD simulation of bow shock nebula
\n<\/td>		Barbara Olmi<\/td>A14<\/td>PDF<\/a><\/td>\n<\/tr>\n
Magnetic reconnection Vlasov simulation<\/td>Francesco Califano<\/td>A16<\/td>PDF<\/a><\/td>\n<\/tr>\n
Global dynamo simulations of stars<\/td>Alfio Bonanno<\/td>BA13<\/td>PDF<\/a><\/td>\n<\/tr>\n
Stability studies of super earth atmospheres
\n<\/td>		Eleonora Alei<\/td>BB0<\/td>PDF<\/a><\/td>\n<\/tr>\n
MACSE<\/td>Roberto Orosei<\/td>B10<\/td>PDF<\/a><\/td>\n<\/tr>\n
On the energy transfer
\nfrom low power jet to IGM
\n<\/td>		Alessandro Capetti<\/td>B11<\/td>PDF<\/a><\/td>\n<\/tr>\n
Anharmonic spectroscopy
\nof astronomical PAHs
\n<\/td>		Giacomo Mulas<\/td>B13<\/td>PDF<\/a><\/td>\n<\/tr>\n
Tests of PINOCCHIO code<\/td>Pierluigi Monaco<\/td>BT6<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
Turbulence Spectral anisotropy and energy flow at ion scales<\/td>Simone Landi<\/td>A22<\/td><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n\n

[\/et_pb_text][\/et_pb_column_inner][\/et_pb_row_inner][et_pb_row_inner admin_label=”Riga”][et_pb_column_inner type=”4_4″ saved_specialty_column_type=”3_4″][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n

Call 3 Project Reports<\/strong><\/h1>\n

[\/et_pb_text][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n\n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Turbulence Spectral anisotropy and energy flow at ion scales<\/td>Simone Landi<\/td>A22<\/td>PDF<\/a><\/td>\n<\/tr>\n
Short GRB jet formation in binary neutron star mergers<\/td>Riccardo Ciolfi<\/td>A23<\/td>PDF<\/a><\/td>\n<\/tr>\n
Simulating Feedback From Powerful Jets<\/td>Gianluigi Bodo<\/td>A24<\/td>PDF<\/a><\/td>\n<\/tr>\n
A numerical study of a new class of astrophysical objects: the isolated star-forming gas cloud<\/td>Francesco Calura<\/td>A25<\/td>PDF<\/a><\/td>\n<\/tr>\n
Atmospheric Modeling of Super Earths orbiting M stars<\/td>Eleonora Alei<\/td>B15<\/td>PDF<\/a><\/td>\n<\/tr>\n
Simulating galaxy outflows in ultrafaint dwarf galaxies<\/td>Donatella Romano<\/td>B16<\/td>PDF<\/a><\/td>\n<\/tr>\n
Modelling anharmonic spectra of PAHs at high temperatures<\/td>Giacomo Mulas<\/td>B18<\/td><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n\n

[\/et_pb_text][\/et_pb_column_inner][\/et_pb_row_inner][et_pb_row_inner admin_label=”Riga”][et_pb_column_inner type=”4_4″ saved_specialty_column_type=”3_4″][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n

Call 4 Project Reports<\/strong><\/h1>\n

[\/et_pb_text][et_pb_text admin_label=”Testo” background_layout=”light” text_orientation=”left” use_border_color=”off” border_color=”#ffffff” border_style=”solid”]<\/p>\n\n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Plasma Turbulence and magnetic reconnection in the low electron beta regime<\/td>Luca Franci<\/td>A26<\/td><\/td>\n<\/tr>\n
Chemodynamics of Ultrafaint Dwarf Galaxies under Ram Pressure and Tidal Forces<\/td>Donatella Romano<\/td>A27<\/td><\/td>\n<\/tr>\n
MatiLeo Simulation<\/td>Franco Vazza<\/td>A28<\/td>PDF<\/a><\/td>\n<\/tr>\n
Global dynamo simulations of massive stars<\/td>Alfio Bonanno<\/td>B19<\/td><\/td>\n<\/tr>\n
Kelvin-Helmholtz instability at the hermean magnetopause: impact of the magnetic field and density gradients<\/td>Francesco Califano<\/td>A30<\/td><\/td>\n<\/tr>\n
Escape of particles from bow shock pulsar wind nebulae<\/td>Barbara Olmi<\/td>A31<\/td>PDF<\/a><\/td>\n<\/tr>\n
Linking core-collapse supernova explosions to supernova remnants through 3D MHD modeling<\/td>Salvatore Orlando<\/td>A32<\/td>PDF<\/a><\/td>\n<\/tr>\n
Realistic simulations of relativistic jet Feedback<\/td>Dipanjan Mukherjee<\/td>A34<\/td>PDF<\/a><\/td>\n<\/tr>\n
Seeing the UNSeEN with Marconi SC<\/td>Guillermo Rodriguez<\/td>B20<\/td>PDF<\/a><\/td>\n<\/tr>\n
AGILE Particle Background Simulation<\/td>Alessio Trois<\/td>B21<\/td><\/td>\n<\/tr>\n
TurboDyn<\/td>Luca Del Zanna<\/td>B22<\/td>PDF<\/a><\/td>\n<\/tr>\n
Numerical simulation of restarting radio galaxies<\/td>Salvatore Massaglia<\/td>B23<\/td>PDF<\/a><\/td>\n<\/tr>\n
HD simulations of Pulsar Wind Nebulae for a morphology-matching analysis<\/td>Barbara Olmi<\/td>B24<\/td>PDF<\/a><\/td>\n<\/tr>\n
MAGRATHEA Cross Section Database<\/td>Antonello Petralia<\/td>B25<\/td>PDF<\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n\n

[\/et_pb_text][\/et_pb_column_inner][\/et_pb_row_inner][\/et_pb_column][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"

  Call 1 Project Reports \n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Simulating galaxy clusters at high resolution<\/td>Veronica Biffi<\/td>A00<\/td>PDF<\/a><\/td>\n<\/tr>\n
Deceleration of relativistic jets<\/td>Gianluigi Bodo<\/td>A01<\/td>PDF<\/a><\/td>\n<\/tr>\n
Formation of star clusters: how common is infant rotation?<\/td>Michela Mapelli
\n
\n<\/td>		A02<\/td><\/td>\n<\/tr>\n
Mechanical feedback and backflows in early-type galaxies.<\/td>Vincenzo Antonuccio
\n<\/td>		A03<\/td>PDF<\/a><\/td>\n<\/tr>\n
The impact of stellar dynamics on gravitational wave sources<\/td>Mario Spera
\n<\/td>		A04<\/td>PDF<\/a><\/td>\n<\/tr>\n
The inner parsecs of our Galaxy: star formation and its environment<\/td>Alessandro Ballone<\/td>A05<\/td>PDF<\/a><\/td>\n<\/tr>\n
DEMNUni Covariances<\/td>Carmelita Carbone<\/td>A06<\/td>PDF<\/a><\/td>\n<\/tr>\n
Effects of the feedback of stellar winds and supernovae in young globular clusters<\/td>Francesco Calura<\/td>B00<\/td>PDF<\/a><\/td>\n<\/tr>\n
Three-dimensional hydrodynamical
\n simulations of
\n supernova explosions in the smallest Milky Way satellites<\/td>		 Donatella Romano<\/td>B01<\/td>PDF<\/a><\/td>\n<\/tr>\n
Instabilities, magnetic reconnection and particle acceleration in Blazar jets<\/td>Claudia Raitieri<\/td>B02<\/td>PDF<\/a><\/td>\n<\/tr>\n
Effects of intense flaring activity on accretion disk of Classical T Tauri Stars<\/td>Salvatore Colombo<\/td>B03<\/td>PDF<\/a><\/td>\n<\/tr>\n
Vlasov simulations of reconnection events and comparison with MMS<\/td>Francesco Califano<\/td>B04<\/td>PDF<\/a><\/td>\n<\/tr>\n
Simulations of disk galaxies: the effect of AGN feedback<\/td>Stefano Borgani<\/td>B05<\/td>PDF<\/a><\/td>\n<\/tr>\n
DUSTGRAIN Follow Up<\/td>Marco Baldi<\/td>B09<\/td>PDF<\/a><\/td>\n<\/tr>\n
Post processing and visualisation of galaxy clusters<\/td>Giuliano Taffoni<\/td>Test<\/td>Test Class. Report not requested
\n<\/td>\n<\/tr>\n
Post processing and visualisation of galaxy clusters<\/td>Stefano Borgani<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
AnharmoniCaOs test<\/td>Giacomo Mulas<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
Radiative transfer in exoplanetary atmospheres<\/td>Giambattista Aresu<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
Dust in the Universe <\/td>Sergio Cristallo<\/td>Test<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n Call 2 Project Reports \n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Jet\/ambient interaction in low power radiosources
\n<\/td>		Silvano Massaglia<\/td>A07<\/td>PDF<\/a><\/td>\n<\/tr>\n
GESBAYES<\/td>Alessandro Lanzafame<\/td>A09<\/td>PDF<\/a><\/td>\n<\/tr>\n
GRMHD simulation of the binary neutron star
\n<\/td>		Riccardo Ciolfi
\n
\n<\/td>		A11<\/td>PDF<\/a><\/td>\n<\/tr>\n
3D MHD simulation of bow shock nebula
\n<\/td>		Barbara Olmi<\/td>A14<\/td>PDF<\/a><\/td>\n<\/tr>\n
Magnetic reconnection Vlasov simulation<\/td>Francesco Califano<\/td>A16<\/td>PDF<\/a><\/td>\n<\/tr>\n
Global dynamo simulations of stars<\/td>Alfio Bonanno<\/td>BA13<\/td>PDF<\/a><\/td>\n<\/tr>\n
Stability studies of super earth atmospheres
\n<\/td>		Eleonora Alei<\/td>BB0<\/td>PDF<\/a><\/td>\n<\/tr>\n
MACSE<\/td>Roberto Orosei<\/td>B10<\/td>PDF<\/a><\/td>\n<\/tr>\n
On the energy transfer
\nfrom low power jet to IGM
\n<\/td>		Alessandro Capetti<\/td>B11<\/td>PDF<\/a><\/td>\n<\/tr>\n
Anharmonic spectroscopy
\nof astronomical PAHs
\n<\/td>		Giacomo Mulas<\/td>B13<\/td>PDF<\/a><\/td>\n<\/tr>\n
Tests of PINOCCHIO code<\/td>Pierluigi Monaco<\/td>BT6<\/td>Test Class. Report not requested<\/td>\n<\/tr>\n
Turbulence Spectral anisotropy and energy flow at ion scales<\/td>Simone Landi<\/td>A22<\/td><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n Call 3 Project Reports \n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Turbulence Spectral anisotropy and energy flow at ion scales<\/td>Simone Landi<\/td>A22<\/td>PDF<\/a><\/td>\n<\/tr>\n
Short GRB jet formation in binary neutron star mergers<\/td>Riccardo Ciolfi<\/td>A23<\/td>PDF<\/a><\/td>\n<\/tr>\n
Simulating Feedback From Powerful Jets<\/td>Gianluigi Bodo<\/td>A24<\/td>PDF<\/a><\/td>\n<\/tr>\n
A numerical study of a new class of astrophysical objects: the isolated star-forming gas cloud<\/td>Francesco Calura<\/td>A25<\/td>PDF<\/a><\/td>\n<\/tr>\n
Atmospheric Modeling of Super Earths orbiting M stars<\/td>Eleonora Alei<\/td>B15<\/td>PDF<\/a><\/td>\n<\/tr>\n
Simulating galaxy outflows in ultrafaint dwarf galaxies<\/td>Donatella Romano<\/td>B16<\/td>PDF<\/a><\/td>\n<\/tr>\n
Modelling anharmonic spectra of PAHs at high temperatures<\/td>Giacomo Mulas<\/td>B18<\/td><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n Call 4 Project Reports \n\n\n\n\t\n\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t\n\t
Project<\/th>Principal Investigator<\/th>Account<\/th>Report PDF<\/th>\n<\/tr>\n<\/thead>\n
Plasma Turbulence and magnetic reconnection in the low electron beta regime<\/td>Luca Franci<\/td>A26<\/td><\/td>\n<\/tr>\n
Chemodynamics of Ultrafaint Dwarf Galaxies under Ram Pressure and Tidal Forces<\/td>Donatella Romano<\/td>A27<\/td><\/td>\n<\/tr>\n
MatiLeo Simulation<\/td>Franco Vazza<\/td>A28<\/td>PDF<\/a><\/td>\n<\/tr>\n
Global dynamo simulations of massive stars<\/td>Alfio Bonanno<\/td>B19<\/td><\/td>\n<\/tr>\n
Kelvin-Helmholtz instability at the hermean magnetopause: impact of the magnetic field and density gradients<\/td>Francesco Califano<\/td>A30<\/td><\/td>\n<\/tr>\n
Escape of particles from bow shock pulsar wind nebulae<\/td>Barbara Olmi<\/td>A31<\/td>PDF<\/a><\/td>\n<\/tr>\n
Linking core-collapse supernova explosions to supernova remnants through 3D MHD modeling<\/td>Salvatore Orlando<\/td>A32<\/td>PDF<\/a><\/td>\n<\/tr>\n
Realistic simulations of relativistic jet Feedback<\/td>Dipanjan Mukherjee<\/td>A34<\/td>PDF<\/a><\/td>\n<\/tr>\n
Seeing the UNSeEN with Marconi SC<\/td>Guillermo Rodriguez<\/td>B20<\/td>PDF<\/a><\/td>\n<\/tr>\n
AGILE Particle Background Simulation<\/td>Alessio Trois<\/td>B21<\/td><\/td>\n<\/tr>\n
TurboDyn<\/td>Luca Del Zanna<\/td>B22<\/td>PDF<\/a><\/td>\n<\/tr>\n
Numerical simulation of restarting radio galaxies<\/td>Salvatore Massaglia<\/td>B23<\/td>PDF<\/a><\/td>\n<\/tr>\n
HD simulations of Pulsar Wind Nebulae for a morphology-matching analysis<\/td>Barbara Olmi<\/td>B24<\/td>PDF<\/a><\/td>\n<\/tr>\n
MAGRATHEA Cross Section Database<\/td>Antonello Petralia<\/td>B25<\/td>PDF<\/a><\/td>\n<\/tr>\n<\/tbody>\n<\/table>\n<\/p>\n","protected":false},"author":185,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":""},"_links":{"self":[{"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/pages\/1671"}],"collection":[{"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/users\/185"}],"replies":[{"embeddable":true,"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/comments?post=1671"}],"version-history":[{"count":6,"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/pages\/1671\/revisions"}],"predecessor-version":[{"id":2896,"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/pages\/1671\/revisions\/2896"}],"wp:attachment":[{"href":"https:\/\/www.ict.inaf.it\/computing\/wp-json\/wp\/v2\/media?parent=1671"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}