71 research outputs found
The QUIET Instrument
The Q/U Imaging ExperimenT (QUIET) is designed to measure polarization in the
Cosmic Microwave Background, targeting the imprint of inflationary
gravitational waves at large angular scales (~ 1 degree). Between 2008 October
and 2010 December, two independent receiver arrays were deployed sequentially
on a 1.4 m side-fed Dragonian telescope. The polarimeters which form the focal
planes use a highly compact design based on High Electron Mobility Transistors
(HEMTs) that provides simultaneous measurements of the Stokes parameters Q, U,
and I in a single module. The 17-element Q-band polarimeter array, with a
central frequency of 43.1 GHz, has the best sensitivity (69 uK sqrt(s)) and the
lowest instrumental systematic errors ever achieved in this band, contributing
to the tensor-to-scalar ratio at r < 0.1. The 84-element W-band polarimeter
array has a sensitivity of 87 uK sqrt(s) at a central frequency of 94.5 GHz. It
has the lowest systematic errors to date, contributing at r < 0.01. The two
arrays together cover multipoles in the range l= 25-975. These are the largest
HEMT-based arrays deployed to date. This article describes the design,
calibration, performance of, and sources of systematic error for the
instrument
First Season QUIET Observations: Measurements of CMB Polarization Power Spectra at 43 GHz in the Multipole Range 25 <= ell <= 475
The Q/U Imaging ExperimenT (QUIET) employs coherent receivers at 43GHz and
95GHz, operating on the Chajnantor plateau in the Atacama Desert in Chile, to
measure the anisotropy in the polarization of the CMB. QUIET primarily targets
the B modes from primordial gravitational waves. The combination of these
frequencies gives sensitivity to foreground contributions from diffuse Galactic
synchrotron radiation. Between 2008 October and 2010 December, >10,000hours of
data were collected, first with the 19-element 43GHz array (3458hours) and then
with the 90-element 95GHz array. Each array observes the same four fields,
selected for low foregrounds, together covering ~1000deg^2. This paper reports
initial results from the 43GHz receiver which has an array sensitivity to CMB
fluctuations of 69uK sqrt(s). The data were extensively studied with a large
suite of null tests before the power spectra, determined with two independent
pipelines, were examined. Analysis choices, including data selection, were
modified until the null tests passed. Cross correlating maps with different
telescope pointings is used to eliminate a bias. This paper reports the EE, BB
and EB power spectra in the multipole range ell=25-475. With the exception of
the lowest multipole bin for one of the fields, where a polarized foreground,
consistent with Galactic synchrotron radiation, is detected with 3sigma
significance, the E-mode spectrum is consistent with the LCDM model, confirming
the only previous detection of the first acoustic peak. The B-mode spectrum is
consistent with zero, leading to a measurement of the tensor-to-scalar ratio of
r=0.35+1.06-0.87. The combination of a new time-stream double-demodulation
technique, Mizuguchi-Dragone optics, natural sky rotation, and frequent
boresight rotation leads to the lowest level of systematic contamination in the
B-mode power so far reported, below the level of r=0.1Comment: 19 pages, 14 figures, higher quality figures are available at
http://quiet.uchicago.edu/results/index.html; Fixed a typo and corrected
statistical error values used as a reference in Figure 14, showing our
systematic uncertainties (unchanged) vs. multipole; Revision to ApJ accepted
version, this paper should be cited as "QUIET Collaboration et al. (2011)
The Q/U Imaging Experiment: Polarization Measurements of Radio Sources at 43 and 95 GHz
We present polarization measurements of extragalactic radio sources observed
during the Cosmic Microwave Background polarization survey of the Q/U Imaging
Experiment (QUIET), operating at 43 GHz (Q-band) and 95 GHz (W-band). We
examine sources selected at 20 GHz from the public, 40 mJy catalog of the
Australia Telescope (AT20G) survey. There are 480 such sources within
QUIET's four low-foreground survey patches, including the nearby radio galaxies
Centaurus A and Pictor A. The median error on our polarized flux density
measurements is 30--40 mJy per Stokes parameter. At S/N significance, we
detect linear polarization for seven sources in Q-band and six in W-band; only
detections per frequency band are expected by chance. For sources
without a detection of polarized emission, we find that half of the sources
have polarization amplitudes below 90 mJy (Q-band) and 106 mJy (W-band), at 95%
confidence. Finally, we compare our polarization measurements to intensity and
polarization measurements of the same sources from the literature. For the four
sources with WMAP and Planck intensity measurements Jy, the polarization
fraction are above 1% in both QUIET bands. At high significance, we compute
polarization fractions as much as 10--20% for some sources, but the effects of
source variability may cut that level in half for contemporaneous comparisons.
Our results indicate that simple models---ones that scale a fixed polarization
fraction with frequency---are inadequate to model the behavior of these sources
and their contributions to polarization maps.Comment: 16 pages, 10 figures. Submitted to Ap
Second Season QUIET Observations: Measurements of the CMB Polarization Power Spectrum at 95 GHz
The Q/U Imaging ExperimenT (QUIET) has observed the cosmic microwave
background (CMB) at 43 and 95GHz. The 43-GHz results have been published in
QUIET Collaboration et al. (2011), and here we report the measurement of CMB
polarization power spectra using the 95-GHz data. This data set comprises 5337
hours of observations recorded by an array of 84 polarized coherent receivers
with a total array sensitivity of 87 uK sqrt(s). Four low-foreground fields
were observed, covering a total of ~1000 square degrees with an effective
angular resolution of 12.8', allowing for constraints on primordial
gravitational waves and high-signal-to-noise measurements of the E-modes across
three acoustic peaks. The data reduction was performed using two independent
analysis pipelines, one based on a pseudo-Cl (PCL) cross-correlation approach,
and the other on a maximum-likelihood (ML) approach. All data selection
criteria and filters were modified until a predefined set of null tests had
been satisfied before inspecting any non-null power spectrum. The results
derived by the two pipelines are in good agreement. We characterize the EE, EB
and BB power spectra between l=25 and 975 and find that the EE spectrum is
consistent with LCDM, while the BB power spectrum is consistent with zero.
Based on these measurements, we constrain the tensor-to-scalar ratio to
r=1.1+0.9-0.8 (r<2.8 at 95% C.L.) as derived by the ML pipeline, and
r=1.2+0.9-0.8 (r<2.7 at 95% C.L.) as derived by the PCL pipeline. In one of the
fields, we find a correlation with the dust component of the Planck Sky Model,
though the corresponding excess power is small compared to statistical errors.
Finally, we derive limits on all known systematic errors, and demonstrate that
these correspond to a tensor-to-scalar ratio smaller than r=0.01, the lowest
level yet reported in the literature.Comment: 10 pages, 6 figures, 3 tables, submitted to ApJ, This paper should be
cited as "QUIET Collaboration (2012)." v2: updated to reflect published
versio
Immunogenicity of Fractional Doses of Tetravalent A/C/Y/W135 Meningococcal Polysaccharide Vaccine: Results from a Randomized Non-Inferiority Controlled Trial in Uganda
Meningitis are infections of the lining of the brain and spinal cord and can cause high fever, blood poisoning, and brain damage, as well as result in death in up to 10% of cases. Epidemics of meningitis occur almost every year in parts of sub-Saharan Africa, throughout a high-burden area spanning Senegal to Ethiopia dubbed the “Meningitis Belt.” Most epidemics in Africa are caused by Neisseria meningitidis (mostly serogroup A and W135). Mass vaccination campaigns attempt to control epidemics by administering meningococcal vaccines targeted against these serogroups, among others. However, global shortages of these vaccines are currently seen. We studied the use of fractional (1/5 and 1/10) doses of a licensed vaccine to assess its non-inferiority compared with the normal full dose. In a randomized trial in Uganda, we found that immune response and safety using a 1/5 dose were comparable to full dose for three serogroups (A, Y, W135), though not a fourth (C). In light of current shortages of meningococcal vaccines and their importance in fighting meningitis epidemics around the world, we suggest fractional doses be taken under consideration in mass vaccination campaigns
Sustainable Urban Systems: Co-design and Framing for Transformation
Rapid urbanisation generates risks and opportunities for sustainable development. Urban policy and decision makers are challenged by the complexity of cities as social–ecological–technical systems. Consequently there is an increasing need for collaborative knowledge development that supports a whole-of-system view, and transformational change at multiple scales. Such holistic urban approaches are rare in practice. A co-design process involving researchers, practitioners and other stakeholders, has progressed such an approach in the Australian context, aiming to also contribute to international knowledge development and sharing. This process has generated three outputs: (1) a shared framework to support more systematic knowledge development and use, (2) identification of barriers that create a gap between stated urban goals and actual practice, and (3) identification of strategic focal areas to address this gap. Developing integrated strategies at broader urban scales is seen as the most pressing need. The knowledge framework adopts a systems perspective that incorporates the many urban trade-offs and synergies revealed by a systems view. Broader implications are drawn for policy and decision makers, for researchers and for a shared forward agenda
Modelling human choices: MADeM and decision‑making
Research supported by FAPESP 2015/50122-0 and DFG-GRTK 1740/2. RP and AR are also part of the Research, Innovation and Dissemination Center for Neuromathematics FAPESP grant (2013/07699-0). RP is supported by a FAPESP scholarship (2013/25667-8). ACR is partially supported by a CNPq fellowship (grant 306251/2014-0)
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