MPI-Bonn is providing the RF hardware which enables 10% of the detectors in both Q and W bands to measure TT correlations.

Faculty/Senior Scientist

Dorothea Samtleben

Caltech is responsible for the beam pattern measurements of the large scale telescopes and integrating them on the CBI mount. Caltech is also responsible for supervising the Chilean staff, and for developing and maintaining software for both data acquisition, telescope control, and initial calibrations.

Faculty/Senior Scientist	PostDoctoral/Fellow	Graduate Student	Undergraduate Student
Tim Pearson Tony Readhead Martin Shepherd	Kieran Cleary Clive Dickinson	Joey Richards	Priya Kollipara

Columbia will be providing all of the cryostats for QUIET. They have major responsibilities for the Q-band arrays, including their integration, optimization, and deployment.

QUIET @ Columbia

Faculty/Senior Scientist	PostDoctoral/Fellow	Graduate Student	Undergraduate Student
Michele Limon Amber Miller	Ross Williamson	Robert DuMoulin Laura Newburgh	Seth Hilbrand Morgan Rhodes

JPL is responsible for production and initial testing of the modules, the most critical component in QUIET. Caltech/JPL will host one of the two analysis centers (Chicago/Caltech), making use of their experience with simulations for Planck. JPL scientists are designing and producing many of the in-dewar electronics boards; and they are slated to lead a field test of a small (7-element) array.

Faculty/Senior Scientist	Engineer
Mark Dragovan Todd Gaier Krzystof Gorski Charles Lawrence Erik Leitch Michael Seiffert	April Campbell Douglas Dawson William Imbriale Pekka Kangaslahti Steve Smith Mary Wells

Members of the Japanese High Energy Physics Laboratory KEK have recently joined QUIET. This constitutes the first initiative into studies of the CMB in Japan. The group is currently building a setup for testing HEMT detectors and is bringing their extensive experience in data acquisition hardware and software to bear in QUIET.

Faculty/Senior Scientist

Masashi Hazumi Takeo Higuchi Osamu Tajima

KICP is responsible for the integration and optimization/characterization of the W-band arrays. It is also responsible for the design of the in-dewar electronics systems and for producing many of the boards as well as the ADC system. Chicago will be co-designing the data acquisition system with Caltech.

The Project Manager will reside in Chicago, the managing institution in QUIET. Chicago will host one of the two analysis centers (Caltech/Chicago) making use of the experience from the analysis of CAPMAP data. In addition to the existing group Wayne Hu and center fellow Xiaomin Wang will help us in getting ready for analysis.

Faculty/Senior Scientist	PostDoctoral/Fellow	Engineer	Graduate Student	Undergraduate Student
Bruce Winstein	Dan Kapner Akito Kusaka	Mircea Bogdan Bill Nagle Dale Sanford	Colin Bischoff Alison Brizius Immanuel Buder Kendrick Smith (now a PPARC Fellow in Cambridge) Keith Vanderlinde (now with SPT)	Kathryn Huff

Stanford is responsible for the design and production of the large scale telescopes and the modification of the CBI platform to accommodate them. They will also be doing a joint analysis of data from QUaD and QUIET.

Faculty/Senior Scientist

Sarah Church Keith Thompson

Manchester is contributing to telescope production.

Faculty/Senior Scientist

Lucio Piccirrilo Peter Wilkinson

Miami is responsible for the design and construction of the platelet arrays for all receivers. These provide the optical benefits of corrugated horns at a reasonable cost. Miami is also leading "KUPID" which will gather important information of galactic foregrounds and which may also take data on the CBI mount.

Faculty/Senior Scientist	Undergraduate Student
Josh Gundersen	David Leibovitch

Oslo is leading an analysis effort and providing a processor farm for the collaboration.

Faculty/Senior Scientist	Graduate Student
Hans Kristian Eriksen	Jostein R. Kristiansen

Oxford University has recently joined and is now designing and slated to produce the ground screen for the large scale telescopes. They will be working on preparations for analysis/simulations as well.

Faculty/Senior Scientist	PostDoctoral/Fellow
Pedro G. Ferreira Mike Jones Joe Silk Ghassan Yassin	Angela Taylor

Princeton is responsible for the design and construction of the OMTs for all receivers, as well as for the Flexible Printed Circuits used to bring signals and biases voltages from the 20K to the warm environment. They will also oversee the refurbishment and move of the 7m telescope to Chile, including the design and construction of its new secondary.

Faculty/Senior Scientist	Graduate Student	Undergraduate Student
Suzanne Staggs	Joshua Green Glen Nixon	Vaclav Cvicek Clinton Hansen Madhuri Kaul Kevin Kung Will Serber Joe Wolf Sajid Zaidi

Martin White will work with a graduate student on QUIET data analysis and interpretations.

Faculty/Senior Scientist

Martin White

Edward Wollack brings his broad perspective to QUIET; he has provided the base design for the L/R OMTs.

Faculty/Senior Scientist

Edward Wollack

Without Robert Wilson, we wouldn't have much to look at!

Faculty/Senior Scientist

Robert Wilson