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QUIET (Q/U Imaging ExperimenT)

The QUIET collaboration during its meeting at Fermilab, June 28-30, 2009. QUIET merges members of previous collaborations that have made successful polarization measurements of the CMB. These are: CAPMAP (Princeton, Chicago, Miami, JPL, MPI-Bonn), CBI (Caltech, Oxford), and QUaD (Stanford, Manchester). A group from Columbia, with lots of experience in CMB measurements, and a group from Oslo, with expertise in CMB data processing and analysis, complete the collaboration. Submitted to ApJ, 2012. Millimeter...

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QUIET (Q/U Imaging ExperimenT) | quiet.uchicago.edu Reviews

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The QUIET collaboration during its meeting at Fermilab, June 28-30, 2009. QUIET merges members of previous collaborations that have made successful polarization measurements of the CMB. These are: CAPMAP (Princeton, Chicago, Miami, JPL, MPI-Bonn), CBI (Caltech, Oxford), and QUaD (Stanford, Manchester). A group from Columbia, with lots of experience in CMB measurements, and a group from Oslo, with expertise in CMB data processing and analysis, complete the collaboration. Submitted to ApJ, 2012. Millimeter...

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7 the quiet experiment

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QUIET (Q/U Imaging ExperimenT) | quiet.uchicago.edu Reviews

https://quiet.uchicago.edu

The QUIET collaboration during its meeting at Fermilab, June 28-30, 2009. QUIET merges members of previous collaborations that have made successful polarization measurements of the CMB. These are: CAPMAP (Princeton, Chicago, Miami, JPL, MPI-Bonn), CBI (Caltech, Oxford), and QUaD (Stanford, Manchester). A group from Columbia, with lots of experience in CMB measurements, and a group from Oslo, with expertise in CMB data processing and analysis, complete the collaboration. Submitted to ApJ, 2012. Millimeter...

INTERNAL PAGES

quiet.uchicago.edu

1

QUIET: Observing Strategy and Analysis

http://quiet.uchicago.edu/observing/index.html

Observing Strategy and Analysis. Data acquisition, storage and distribution. Simulations of the Science Reach for QUIET. We use a periodical scan in azimuth ( 1 degree/second) at high elevations (minimizing ground and atmospheric contributions), fixing the elevation and rotation angle about the optical axis. QUIET radiometers measure both Q and U simultaneously. Still, in order to best separate Q and U, it is desirable to re-measure each pixel multiple times where the detector. Difference in RA, covering...

2

QUIET: Team for QUIET Phase II

http://quiet.uchicago.edu/team/index.html

Team for QUIET Phase II. Max Planck Institute for Radio Astronomy in Bonn. California Institute of Technology. Columbia University in the city of New York. Fermi National Accelerator Laboratory. High Energy Accelerator Research Organization. Kavli Institute for Cosmological Physics at the University of Chicago. Kavli Institute for Particle Astrophysics and Cosmology at the Stanford University. Goddard Space Flight Center. Bonn, Max Planck Institute for Radio Astronomy in Bonn. Miami, University of Miami.

3

QUIET: Instrumentation

http://quiet.uchicago.edu/instrumentation/index.html

Degree Angular Scale Interferometer. Wilkinson Microwave Anisotropy Probe. Overview of QUIET Detector Arrays. The QUIET Polarimetry Modules. Feed horns and Orthomode Transducers. The QUIET Array Optimizer. And build on established techniques for controlling polarization systematic errors. We describe our methods for realizing each N-element dual-Stokes. Mounted on the Cosmic Background Imager (CBI) platform in Chajnantor, Chile, at an altitude of 5080 m. Each of the N elements simultaneously. The key to ...

4

QUIET (Q/U Imaging ExperimenT)

http://quiet.uchicago.edu/index.php

The QUIET collaboration during its meeting at Fermilab, June 28-30, 2009. QUIET merges members of previous collaborations that have made successful polarization measurements of the CMB. These are: CAPMAP (Princeton, Chicago, Miami, JPL, MPI-Bonn), CBI (Caltech, Oxford), and QUaD (Stanford, Manchester). A group from Columbia, with lots of experience in CMB measurements, and a group from Oslo, with expertise in CMB data processing and analysis, complete the collaboration. Submitted to ApJ, 2012. Millimeter...

5

QUIET: Science

http://quiet.uchicago.edu/science/index.html

Degree Angular Scale Interferometer. Wilkinson Microwave Anisotropy Probe. Physics in Precision Studies of CMB Polarization. The Status of E-mode Polarization. The Promise of B-Mode Polarization. CMB science with QUIET. Physics in Precision Studies of CMB Polarization. The Status of E-mode Polarization. Experiments have detected the E-mode polarization: the present status on the EE power spectrum is displayed in Figure 1. In addition, the TE correlation has been detected by WMAP. The Promise of B-Mode Po...

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destinopolosur.blogspot.com

DestinoPoloSur: diciembre 2012

http://destinopolosur.blogspot.com/2012_12_01_archive.html

Sigue mi experiencia de vivir un año en el Polo Sur como winterover del observatorio de neutrinos más grande del mundo! Lunes, 24 de diciembre de 2012. DESDE LA BASE AMUNDSEN-SCOTT LES ENVIAMOS UN GRAN SALUDO DE NAVIDAD A TODOS EN EL MUNDO. También hemos recibido saludos de navidad desde otras bases antárticas. Vean abajo las tarjetas de saludos y el link a wikipedia en el nombre de cada base para mayores detalles. Saludo de navidad de la base Amundsen-Scott, Polo Sur. No hay comentarios.:. Realizando me...

astro.caltech.edu

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http://www.astro.caltech.edu/~acr

Robinson Professor of Astronomy. Director, Owens Valley Radio Observatory. 222 Cahill, Caltech. Cosmology and the Formation of Structure in the Universe. Active Galaxies and Fermi-GST. High Resolution Imaging Techniques. The Cosmic Background Imager* (CBI). The QU Imaging ExperimenT* (QUIET). The C-Band All Sky Survey (CBASS). At the Chajnantor Test Facility. Sievers, J. L., et al. 2005, preprint. Implications of the Cosmic Background Imager polarization data. Middot; PDF Reprint. Middot; PDF Reprint.

chajnantor.caltech.edu

Chajnantor Observatory: SAINT

http://chajnantor.caltech.edu/saint/index.html

Strategic Alliance for the Implementation of New Technologies (SAINT). Description and Statement of Purpose. The Strategic Alliance for the Implementation of New Technologies (SAINT) is a consortium consisting of groups from the following twelve institutions:. The California Institute of Technology and the Jet Propulsion Laboratory,. The University of Chicago,. The Max Planck Institute for Radio Astronomy (Bonn),. The University of Manchester,. The University of Miami,. The University of Oslo, and. In pu...

astro.caltech.edu

Chajnantor Observatory

http://www.astro.caltech.edu/chajnantor

A facility operated by the California Institute of Technology (Caltech) in collaboration with the University of Chile and the University of Concepción, is located at an elevation of 5080 meters (16700 feet) in the Andes mountains in northern Chile. The high, dry Chajnantor plateau is one of the best sites in the world for millimeter and submillimeter astronomy. The observatory is partially supported by the Strategic Alliance for the Implementation of New Technologies. The Q/U Imaging ExperimenT. Another ...

destinopolosur.blogspot.com

DestinoPoloSur: Por qué y cómo he llegado a este lugar?

http://destinopolosur.blogspot.com/2012/12/porque-y-como-he-llegado-este-lugar.html

Sigue mi experiencia de vivir un año en el Polo Sur como winterover del observatorio de neutrinos más grande del mundo! Jueves, 20 de diciembre de 2012. Por qué y cómo he llegado a este lugar? He comenzado escribiendo este blog desde el momento en que pisaba Antártica, sin embargo no he hablado sobre qué y por qué estoy realmente aquí. Observatorio geodésico TIGO en Concepción, Chile. Radiotelescopio QUIET en el Llano de Chajnantor, Desierto de Atacama, Chile. Mi interés por los observatorios y mi deseo ...

chajnantor.caltech.edu

Chajnantor Observatory

http://chajnantor.caltech.edu/safety

blankonthemap.blogspot.com

Blank On The Map: BICEP2: reasons to be sceptical, part 1

http://blankonthemap.blogspot.com/2014/03/bicep2-reasons-to-be-sceptical-part-1.html

Blank On The Map. Explorations of physics and whimsy. Friday, March 21, 2014. BICEP2: reasons to be sceptical, part 1. As the dust begins to settle following the amazing announcement of the discovery of gravitational waves by the BICEP2 experiment, physicists around the world are taking stock and scrutinizing the results. However, as all physicists have been saying, with results of this magnitude it is important to be very careful indeed. Speculating who should get the Nobel Prize (or Prize s. What I wan...

edg.uchicago.edu

Electronics Design Group Projects

http://edg.uchicago.edu/projects

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lwlab.dunlap.utoronto.ca

Long Wavelength Lab - University of Toronto, Dunlap Institute for Astronomy & Astrophysics

http://lwlab.dunlap.utoronto.ca/members.html

Prof Vanderlinde is a microwave cosmologist by training, interested in the Large Scale Structure of the Universe. His work focuses on development of innovative instruments and observational probes of stucture ranging from the. To Baryone Acoustic Oscillations. And he has recently joined early efforts to develop the field of pulsar scintillometry. Dr Klages comes from a background of holographic imaging, a technique strikingly similar to the beam-forming correlation proposed for CHIME. Colin Merkel joined...

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QUIET (Q/U Imaging ExperimenT)

The QUIET collaboration during its meeting at Fermilab, June 28-30, 2009. QUIET merges members of previous collaborations that have made successful polarization measurements of the CMB. These are: CAPMAP (Princeton, Chicago, Miami, JPL, MPI-Bonn), CBI (Caltech, Oxford), and QUaD (Stanford, Manchester). A group from Columbia, with lots of experience in CMB measurements, and a group from Oslo, with expertise in CMB data processing and analysis, complete the collaboration. Submitted to ApJ, 2012. Millimeter...

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