Program

Courses are given daily from Monday to Friday in sessions of 45 minutes (#) from 8:30 am to 5:30 pm, followed by 45 minutes of discussion and three 15-minute presentations given by participants. Interruptions of 30 and 90 minutes (coffee breaks and lunches) will allow for exchanges and provide opportunities for speakers to develop their topics informally.

The additions or exceptions to this schedule are as follows:

Sunday 12 November 2017: Arrival of participants

• 7:15 pm at the airport of Ajaccio, departure of the shuttle for the IESC
• 8:00 pm - 8:30 pm: Installation of the participants

• 8:20 am - 8:30 am: Presentation of the IESC
• 7:30 pm - 8:30 pm: Welcome party
  

• 1:30 pm - 5:30 pm : Hike to the Genoese tower of Punta d'Omigna

• 12:30 am : Group photo
• 7:30 pm - 9:30 pm: Banquet

• 09 am at IESC, departure of the shuttle for the Ajaccio airport

Title	Lecturer	#	Id	Abs.	Slides
Introduction to the Cargese school  "The CMB from A to Z"	F. R. Bouchet	3	FRB		pdf : 1
The magnetized interstellar medium	F. Boulanger	1	FB		pdf : 1
Statistical description and modeling of polarized foregrounds	F. Boulanger	1	FB		pdf : 1
Extracting the Cosmic Microwave Background from multi-frequency observations	J.-F. Cardoso	3	JFC		pdf : 1
Cosmology Beyond Thermal Equilibrium: Future Steps with CMB Spectral Distortions	J. Chluba	3	JC		pdf : 1
Extragalactic surveys with CMB experiments	G. De Zotti	1	GDZ		pdf : 1
CMB Experimental Landscape	K. Ganga	1	KG		pdf : 1
Galactic dust as a nuisance for cosmological studies	V. Guillet	1	VG		pdf : 1
CMB, angular power spectra and their likelihoods: in Theory and in Practice	E. Hivon	2	EH		pdf : 1, 2
Physics of CMB Anisotropies	E. Komatsu	5	EK		pdf :1, 2, 3, 4, 5
CMB lensing	A. Lewis	2	AL		pdf : 1
Primordial non-Gaussianity	S. Matarrese	2	SM		pdf : 1
SZ clusters as cosmological probes	J.-B. Melin	2	JBM		pdf : 1
From TOI to maps & E2E simulations	P. Natoli	1	PN		pptx : 1
CMB Instruments	M. Piat	3	MP		pdf : 1, 2, 3
Galactic foregrounds and scattering transform	E. Allys	⅓	S4		pdf : 1
Dark Energy from the Thermal Sunyaev Zeldovich Power Spectrum	B. Bolliet	⅓	S1		pdf : 1
Which Galactic dust map should I use ? Insights from extragalactic tomography	Y-K Chiang	⅓	S3		pdf : 1
CosmoML: A Machine Learning method to measure the cosmological parameters	M. de los Rios	⅓	S2		pdf : 1
Probing secret interactions in the neutrino sector  through CMB observations	F. Forastieri	⅓	S4		pdf : 1
Optimization of the next generation of CMB missions	D.T. Hoang	⅓	S4		pdf : 1
Model-based component separation exploring sparsity	M. Irfan	⅓	S2		pdf : 1
The cosmic infrared background and ISW effect: can we constrain the cosmology?	A. Maniyar	⅓	S3		pdf : 1
Cosmological constraints on scalar-tensor gravity and the variation of G	J. Ooba	⅓	S3		pdf : 1
Investigating Cluster Astrophysics and Cosmology with Cross-Correlation of tSZ and WL	K. Osato	⅓	S2		pdf : 1
Measuring the mass of galaxy clusters with CMB lensing	S. Patil	⅓	S4		pdf : 1
Primordial non-Gaussianity and y-distortions: dealing with secondary sources	A. Ravenni	⅓	S1		pptx : 1
A GW yielding small field model	I. Wolfson	⅓	S1		pptx : 1

Schedule