- Baccigalupi, Carlo. : ICA Based Component Separation and CMB Polarization.
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- Bartlett, James : Analysis of Need to go to Space.
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- Battye, Richard : Topological Defects.
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- Beck, Rainer : SKADS: Polarization Simulations.
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- Bernard, J.-Philippe . : Dust Polairzation at Long Wavelengths.
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- de Bernardis, , Paolo : The Italian View of BPol.
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- Bock, Jamie : Experimental Probe of Inflationary Cosmology (EPIC).
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- Burigana, Carlo : Foreground Working Group General Talk
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- Carretti, E. : Surveys of the Polarized Synchrotron Emission at @ 2.3 GHz.
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- Colombo, L.P.L. : Added Science from Improved Measurements of T and E.
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- Désert, Francois-Xavier : BPol and the SAMPAN Design Study.
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- Finelli, Fabio : Distinguishing Primordial B Modes from Lensing.
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- Land, Kate : Science Case Working Group : Inflation Section.
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- Leahy, Patrick : CBASS (C-Band All Sky Survey).
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- Macias-Perez, Juan : Blind Component Separation for Polarized Observations of the CMB
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- Macias-Perez, Juan : Using Archeops and WMAP to simulate polarized diffuse backgrounds
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- Martinez-Gonzalez, Enrique : Foreground limits on the detectability of the B-mode by BPol.
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- Massardi M. :
Polarization Properties of Extragalactic Point Sources (EPS) at High Frequencies.
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- Matarrese, Sabino : Non-Gaussianity and BPol.
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- Orlando, Angiola : CARDIFF Astronomy Instrumentation group.
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- Perotto, Laurence : Exploitation of the Gravitational Lensing Signal:
Probing the large scale structures with the CMB
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- Piccirillo, Lucio : UK Contribution to B-Pol .
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- Rebolo, Raphael. : B-pol : Views in Spain.
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- Rubino Martin, J.A. : Latest results on Anomalous Galactic Microwave Emission from the Cosmosomas Experiment.
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- Siringo, G. : PolKa : A tunable polarimeter for (sub)mm bolometer arrays.
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- Stompor, Radek : B-pol data analysis: Preliminaries.
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- Tucker, Gregory : The Einstein Polarization Interferometer for Cosmology (EPIC).
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- Report From CNES Study : SAMPAN (Satellite for Analyzing Microwave Polarization Anisotropies).
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- Science Requirements for SAMPAN.
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- NASA Definition of Technology Readiness Levels.
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