Calendar
| Mon | Tue | Wed | Thu | Fri | Sat | Sun | 
|---|---|---|---|---|---|---|
| 
											
												Visita Istituto Giotto-Cipolla di Palermo maestre A.Passarello e S.Ferro
											
																							
													11:30
												
																					 
											
												Seminario: Ripetizione Tesi Vincenzo Cusimano
											
																							
													15:30
												
																					 
																				
											Seminario: Ripetizione Tesi Vincenzo Cusimano
																					
										
										 
											Mar 5 @ 15:30 – 18:00
										 Speaker: Vincenzo Cusimano Titolo: Abstract: | ||||||
| 
											
												Seminario: Ripetizione tesi Roberto Alfano (UniPa)
											
																							
													15:00
												
																					 
																				
											Seminario: Ripetizione tesi Roberto Alfano (UniPa)
																					
										
										 
											Mar 10 @ 15:00 – 17:00
										 Titolo: Modeling the interaction of a Supernova Remnant with the Circumstellar Medium – The case of the gamma-ray bright galactic supernova remnant RX J1713.7-3946   Abstract: SNRs are strongly characterized by their interaction with the circumstellar medium (CSM), often shaped by the mass loss history of the progenitor star, and with the ambient interstellar medium (ISM). The aim of the | ||||||
| 
											
												Seminario: Alex Thompson (UCL)
											
																							
													15:00
												
																					 
																				
											Seminario: Alex Thompson (UCL)
																					
										
										 
											Mar 27 @ 15:00 – 17:00
										 Speaker: Alex Thompson (UCL) Title: Probing Impacts of Stellar Variability within HST WFC3/STIS and Ariel Tier 2 and Tier 3 Observations with Activity Metrics Abstract: Stellar activity produces two main diagnostics within low-resolution exoplanet transmission spectra. Its highly chromatic nature imparts trends in the underlying spectrum that become most noticeable at shorter wavelengths due to the increased contrast between the | ||||||
	
		
		
												Subscribe to filtered calendar
										
		
	
			
		