List of contributions
Talks & Posters
(updated on June. 25th, 2K1)



 
Name Istitution Contribution Title Abstract
Ali Shafinaz University of Wales
Cardiff - UNITED KINGDOM
MBI: Millimeter Wave Bolometric Interferometer
available
Aretxaga Itziar INAOE, Instituto Nacional de Astrofisica, Optica y Electronica
Tonantzintla - MEXICO
Constraints on the accuracy of millimetre - FIR photometric redshifts
available
Battistelli Elia S. Università di Milano - Bicocca
Milan - ITALY
MASTER: millimetre and sub-millimetre three heterodyne receivers
available
Benoit Alain Centre de Recherches sur les Tres Basses Temperatures - CNRS
Grenoble - FRANCE
The Archeops balloon experiment for measuring the CMB anisotropies
available
Bock James Jet Propulsion Laboratory - Caltech
Pasadena, CA - USA
Spider-web bolometers
available
Bujakas Victor Astro Space Center of LPI RAN
Moscow - RUSSIA
The infrared telescope for Submillimetron Mission
available
Carretti Ettore TESRE - CNR
Bologna - ITALY
The BaR-SPOrt Experiment
available
Cartwright John California Institute of Technology
Pasadena, CA - USA
Polarization Observations with the Cosmic Background Imager
available
Chapin Edward INAOE, Instituto Nacional de Astrofisica, Optica y Electronica
Tonantzintla - MEXICO
Telescope simulations of wide-area millimetre and submillimetre surveys
available
Colafrancesco Sergio Osservatorio Astronomico di Roma
Monteporzio - ITALY
Non-thermal vs. Thermal SZ effect in galaxy clusters: theoretical and observational constraints
available
Cortiglioni Stefano TESRE - CNR
Bologna - ITALY
The SPOrt Program
available
de Bernardis Paolo Università "La Sapienza"
Rome - ITALY
l-space spectroscopy of the cosmic microwave background
available
Desert F. Xavier Laboratoire d'Astrophysique, Observatoire de Grenoble
Grenoble - FRANCE
Diabolo and the future of ground based bolometric devices
available
Devlin Mark University of Pennsylvania
Philadelphia, PA - USA
Millimeter and Submillimeter Observations from the Atacama Plateau and High Altitude Balloons
available
Dupac Xavier CESR
Toulouse - FRANCE
Optimal map-making methods for large CMB timelines
available
Encrenaz Pierre DEMIRM, Observatoire de Paris
Paris - FRANCE
Herschel Space Observatory and Odin preliminary results
not yet available
Encrenaz Therese DESPA, Observatoire de Paris
Meudon - FRANCE
Calibrations on planets at millimeter and submillimeter wavelengths
available
Gaztanaga Enrique INAOE, Instituto Nacional de Astrofisica, Optica y Electronica
Tonantzintla - MEXICO
Clustering in deep millimetre surveys
available
Gear Walter University of Wales
Cardiff - UNITED KINGDOM
QUEST: Measuring the Polarization of the CMB
not yet available
Giard Martin CESR
Toulouse - FRANCE
Clusters of Galaxies in SZ surveys and dust contamination
not yet available
Gleeson Emily National University of Ireland Maynooth
Maynooth - IRELAND
Electromagnetic Modelling of Few-Moded Winston Cones in the Far-Infrared.
available
Gromov Vladimir Astro Space Center of LPI RAN
Moscow - RUSSIA
Submillimeter and millimeter wave sky mapping in space project Submillimetron
available
Holler Christian Astrophysics Group, Cavendish Laboratory,  Cambridge University Cambridge - UNITED KINGDOM Broadband Correlator for AMI
available
Hristov Viktor California Institute of Technology
Pasadena, CA - USA 
Signal Processing of NTD-GE Cryogenic Bolometric Sensors
available
Hughes David INAOE, Instituto Nacional de Astrofisica, Optica y Electronica
Tonantzintla - MEXICO
Guiding cosmological experiments with simulated millimetre wavelength surveys
available
Jones Michael Astrophysics Group, Cavendish Laboratory,  Cambridge University
Cambridge - UNITED KINGDOM
Spurious signals in VSA data
available
Keating Brian Caltech Observational Cosmology
Pasadena, CA - USA
Polarization of the CMB: Large Angular Scales Results From POLAR
available
Kreysa Ernst Max-Planck-Institut fuer Radioastronomie
Bonn - GERMANY
Bolometer arrays for Astronomy
available
Lamagna Luca Università "La Sapienza"
Rome - ITALY
The MAD-4-MITO experiment: multi-pixel, multi-band ground-based observations of SZ effect
 available
Lamarre Jean Michel Institut d'Astrophysique Spatiale, Universite Paris-Sud
Orsay - FRANCE
Planck-HFI: performance requirements and instrument
design
available
Leitch Erik University of Chicago
Chicago, IL - USA
First Season Results from the Degree Angular Scale Interferometer
available
Lubin Phil University of California at Santa Barbara 
Santa Barbara, CA USA
Future Balloon Borne and Ground Based CMB Measurement
available
Macculi Claudio TESRE - CNR
Bologna - ITALY
BaR SPOrt: Balloon Radiometer for Sky Polarisation Observations
available
Mandolesi Reno TESRE - CNR
Bologna - ITALY
Planck Low Frequency Instrument
not yet available
Masi Silvia Università "La Sapienza"
Rome - ITALY
Diffuse emission from Interstellar Dust at mm wavelengths: a problem for high sensitivity CMB experiments?
available
Masi Silvia Università "La Sapienza"
Rome - ITALY
B2K
available
Mauskopf Phil University of Wales
Cardiff - UNITED KINGDOM
BOLOCAM: A 144 Element Bolometer Array
available
Melchiorri Francesco Università "La Sapienza"
Rome - ITALY
Measurements of CMB polarization
available
Mennella Aniello IFC-CNR
Milan - ITALY
Analysis of thermally-induced effects in Planck Low Frequency Instrument
available
Morgante Gianluca TESRE - CNR
Bologna - ITALY
Two Hydrogen Sorption Cryocoolers for the Planck Mission
available
Murphy J.Anthony National University of Ireland Maynooth
Maynooth - IRELAND
Corrugated Horn Design for PLANCK
available
Natale Enzo Osservatorio Astrofisico di Arcetri 
Florence - ITALY
HERSCHEL/FIRST: The Far Infrared and Sub-millimeter Space Telescope
available
Nati Federico Università "La Sapienza"
Rome - ITALY
A fast star sensor for balloon borne payloads
available
O'Sullivan Creidhe National University of Ireland Maynooth
Maynooth - IRELAND
MM-Wave Optics Design & Verification
available
Palladino Emilia Università "La Sapienza"
Rome - ITALY
Spatial features of non-thermal SZ effect in galaxy clusters
available
Pascale Enzo IROE - CNR
Florence - ITALY
Attitude Control System for balloon borne experiments
available
Piacentini Francesco Università "La Sapienza"
Rome - ITALY
The Boomerang experiment
available
Piccirillo Lucio University of Wales
Cardiff - UNITED KINGDOM
COMPASS: a 2.6m telescope for CMBR polarization studies
available
Phillips Thomas G.  California Institute of Technology
Pasadena, CA USA
CSO and it's contribution to Experimental Cosmology
not yet available
Puy Denis Institute of Theoretical Physics, University of Zurich
Zurich - SWITZERLAND
Molecules at millimeter wavelengths 
available
Raccanelli Andrea Max-Planck-Institut fuer Radioastronomie
Bonn - GERMANY
Excess Noise in Cryogenic detectors due to Vibrating 1 K Pots
available
Raljevich Mirko Instituto de Investigaciones Fisicas - UMSA
La Paz - BOLIVIA
Chacaltaya Mountain: An option for astrophysical observations
available
Reichertz Lothar Max-Planck-Institut fuer Radioastronomie
Bonn - GERMANY
Fast Scanning: a new observing technique with detector arrays
available
Rephaeli Yoel Tel Aviv University
Tel Aviv - ISRAEL
The Sunyaev-Zeldovich Effect: Recent Progress and Future Prospects
available
Reveret Vincent CEA/Saclay, Service d'Astrophysique
Sacley - FRANCE
A fully sampled bolometer camera for ground submillimeter observations
available
Richards Paul University of California at Berkeley
Berkeley, CA USA
The MAXIMA and MAXIPOLE Experiments
available
Richards Paul University of California at Berkeley
Berkeley, CA USA
New Technologies for the Detection of Millimeter and Submillimeter Waves
available
Romeo Giovanni INGV
Rome - ITALY
Wide-Sky High-Precision Sun Angle Detector
available
Sandri Maura TESRE - CNR
Bologna - ITALY
Optical interface of the Planck Low Frequency Instrument
available
Signore Monique DEMIRM, Observatoire de Paris
Paris - FRANCE
CMBA and primordial nucleosynthesis
available
Silverberg Robert NASA/Goddard Space Flight Center
Greenbelt,MD - USA
Arrays of Bolometric Detectors 
available
Siringo Giorgio Max-Planck-Institut fuer Radioastronomie
Bonn - GERMANY
PolKa: a tunable polarimeter for mm/submm wavelenghts
available
Soglasnova Vera Space Research Institute of Russian Academy of Science
Moscow - RUSSIA
The spectral filters for the astronomical observations through the atmospheric windows
available
Spergel Martin York College of the City University of New York
New York - USA
A Center for Cosmic Structure
available
Stark Anthony Smithsonian Astrophysical Observatory
Cambridge, MA - USA
Millimeter and Submillimeter Observations from the South Pole
available
Subrahmanyan Ravi Australia Telescope National Facility (CSIRO)
Narrabri - AUSTRALIA
Cross-talk in close-packed interferometer arrays
available
Tascone Riccardo IRITI-CNR  c/o Politecnico di Torino 
Torino - ITALY
Millimeter wave passive devices for measurements of the polarized sky emission
available
Taylor Angela Cavendish Astrophysics, University of Cambridge
Cambridge - UNITED KINGDOM
The Very Small Array
available
Terenzi Luca TESRE - CNR
Bologna - ITALY
Planck-LFI: Sources quick identification
available
Thorpe Jim R. Department of Electronic and Electrical Engineering, University of Leeds
Leeds - UNITED KINGDOM
Design and Fabrication of Broad-Band Quasi-Optical Heterodyne Detectors for MASTER
available
Tofani Gianni CAISMI-CNR/Osservatorio Astrofisico di Arcetri
Florence - ITALY
The ALMA Project
available
Valenziano Luca TESRE - CNR
Bologna - ITALY
The 4K Reference Load for the Planck Low Frequency Instrument
available
Villa Fabrizio TESRE - CNR
Bologna - ITALY
Planck Telescope Performances
available
Wilson Grant University of Massachusetts - Dept. of Astronomy
Amherst, MA - USA
An Update on The TopHat Experiment
available
Withington Stafford Astrophysics Group, Cavendish Laboratory,  Cambridge University
Cambridge - UNITED KINGDOM
Partially-Coherent Long-Wavelength Optical Simulation Techniques  for Microwave Background Astronomy
available
Yurchenko Vladimir National University of Ireland Maynooth
Maynooth - IRELAND
Measuring CMB Polarization with ESA PLANCK SubMM-Wave
Telescope
available
Zannoni Mario Università di Milano - Bicocca
Milan - ITALY
The Milano polarimeter: an instrument to search for large scale polarization of the Cosmic Microwave Background
available

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