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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