493 research outputs found
Recovery of Large Angular Scale CMB Polarization for Instruments Employing Variable-delay Polarization Modulators
Variable-delay Polarization Modulators (VPMs) are currently being implemented
in experiments designed to measure the polarization of the cosmic microwave
background on large angular scales because of their capability for providing
rapid, front-end polarization modulation and control over systematic errors.
Despite the advantages provided by the VPM, it is important to identify and
mitigate any time-varying effects that leak into the synchronously modulated
component of the signal. In this paper, the effect of emission from a K
VPM on the system performance is considered and addressed. Though instrument
design can greatly reduce the influence of modulated VPM emission, some
residual modulated signal is expected. VPM emission is treated in the presence
of rotational misalignments and temperature variation. Simulations of
time-ordered data are used to evaluate the effect of these residual errors on
the power spectrum. The analysis and modeling in this paper guides
experimentalists on the critical aspects of observations using VPMs as
front-end modulators. By implementing the characterizations and controls as
described, front-end VPM modulation can be very powerful for mitigating
noise in large angular scale polarimetric surveys. None of the systematic
errors studied fundamentally limit the detection and characterization of
B-modes on large scales for a tensor-to-scalar ratio of . Indeed,
is achievable with commensurately improved characterizations and
controls.Comment: 13 pages, 13 figures, 1 table, matches published versio
CORSIA: The first internationally adopted approach to calculate life-cycle GHG emissions for aviation fuels
The aviation sector has grown at a significant pace in recent years, and despite improvements in aircraft efficiency, the sector's impact on climate change is a growing concern. To address this concern, the International Civil Aviation Organization (ICAO) established the Carbon Offsetting and Reduction Scheme for International Aviation (CORSIA) to help reduce aviation greenhouse gas (GHG) emissions. This paper presents a methodology agreed by the 193 ICAO member states to evaluate the life-cycle GHG emissions of sustainable aviation fuels (SAFs), in the CORSIA system. The core life-cycle assessment and induced land use change values of SAFs are presented to determine the GHG savings of certified pathways. The paper aims to present that a number of SAFs can yield significant life-cycle emission reductions compared to petroleum-derived jet fuel. This implies the potentially major role of SAFs in reducing aviation's carbon footprint
Supreme Court Clerks\u27 Recollections of October Term 1951, Including the Steel Seizure Cases
A roundtable panel discussion at the Chautauqua Institution. The panel brought together five lawyers who fifty-five years ago served as law clerks to Justices of the Supreme Court of the United States. The panelists discussed the Justices and some of the cases of that Supreme Court Term, including the Steel Seizure Cases,1 which came to the Supreme Court in the spring of 1952. The honored guests and panelists are five lawyers who have led high-achieving, diverse and public-spirited lives: Charles C. Hileman, Abner J. Mikva , James C.N. Paul , Neal Person Rutledge, Marshall L. Small
Supreme Court Law Clerks\u27 Recollections of October Term 1951, Including the Steel Seizure Cases
Supreme Court Law Clerks\u27 Recollections of October Term 1951, Including the Steel Seizure Cases
The Atacama Cosmology Telescope: A Measurement of the 600< ell <8000 Cosmic Microwave Background Power Spectrum at 148 GHz
We present a measurement of the angular power spectrum of the cosmic
microwave background (CMB) radiation observed at 148 GHz. The measurement uses
maps with 1.4' angular resolution made with data from the Atacama Cosmology
Telescope (ACT). The observations cover 228 square degrees of the southern sky,
in a 4.2-degree-wide strip centered on declination 53 degrees South. The CMB at
arcminute angular scales is particularly sensitive to the Silk damping scale,
to the Sunyaev-Zel'dovich (SZ) effect from galaxy clusters, and to emission by
radio sources and dusty galaxies. After masking the 108 brightest point sources
in our maps, we estimate the power spectrum between 600 < \ell < 8000 using the
adaptive multi-taper method to minimize spectral leakage and maximize use of
the full data set. Our absolute calibration is based on observations of Uranus.
To verify the calibration and test the fidelity of our map at large angular
scales, we cross-correlate the ACT map to the WMAP map and recover the WMAP
power spectrum from 250 < ell < 1150. The power beyond the Silk damping tail of
the CMB is consistent with models of the emission from point sources. We
quantify the contribution of SZ clusters to the power spectrum by fitting to a
model normalized at sigma8 = 0.8. We constrain the model's amplitude ASZ < 1.63
(95% CL). If interpreted as a measurement of sigma8, this implies sigma8^SZ <
0.86 (95% CL) given our SZ model. A fit of ACT and WMAP five-year data jointly
to a 6-parameter LCDM model plus terms for point sources and the SZ effect is
consistent with these results.Comment: 15 pages, 8 figures. Accepted for publication in Ap
Evidence for dark energy from the cosmic microwave background alone using the Atacama Cosmology Telescope lensing measurements
For the first time, measurements of the cosmic microwave background radiation
(CMB) alone favor cosmologies with dark energy over models without dark
energy at a 3.2-sigma level. We demonstrate this by combining the CMB lensing
deflection power spectrum from the Atacama Cosmology Telescope with temperature
and polarization power spectra from the Wilkinson Microwave Anisotropy Probe.
The lensing data break the geometric degeneracy of different cosmological
models with similar CMB temperature power spectra. Our CMB-only measurement of
the dark energy density confirms other measurements from
supernovae, galaxy clusters and baryon acoustic oscillations, and demonstrates
the power of CMB lensing as a new cosmological tool.Comment: 4 pages, 3 figures; replaced with version accepted by Physical Review
Letters, added sentence on models with non-standard primordial power spectr
Preliminary seismological and geological studies of the San Fernando, California, earthquake of February 9 1971
The San Fernando earthquake was the largest earthquake to occur in the metropolitan Los
Angeles area in more than 50 years. It has tentatively been assigned a magnitude, M_L of 6.6, a focal
depth of 13.0 km, and an epicentral location about 12 km east of Newhall, California, at 34°24.0'N,
118°23.7'W (Figure 1), but these figures undoubtedly will be modified as further data become available.
Although the focal depth is not as well defined as the epicenter, it is consistent with other
observations suggesting thrusting on a fault plane dipping north about 45 ° and breaking the surface
in the Sylmar-San Fernando area (Figure 1). It should be emphasized that the hypocenter of
the main shock represents only the point of initial rupture. Breaking, presumably, then propagated
southward and upward from this point, so that the main geological and engineering effects
were observed farther south where the fault was shallower and the displacement greater. The location
of the main shock is based on readings from permanent stations of the Caltech network, as
well as the U. S. Geological Survey station at Point Mugu (SBLG) and the California Department
of Water Resources stations at Pyramid (PYR) and Cedar Springs (CSP). Portable Caltech seismographs
were installed in the epicentral area as early as 3 hr following the main shock, and,
within a few days, there were at least 30 portable units in the region operated by various groups
and agencies
The Atacama Cosmology Telescope (ACT): Beam Profiles and First SZ Cluster Maps
The Atacama Cosmology Telescope (ACT) is currently observing the cosmic
microwave background with arcminute resolution at 148 GHz, 218 GHz, and 277
GHz. In this paper, we present ACT's first results. Data have been analyzed
using a maximum-likelihood map-making method which uses B-splines to model and
remove the atmospheric signal. It has been used to make high-precision beam
maps from which we determine the experiment's window functions. This beam
information directly impacts all subsequent analyses of the data. We also used
the method to map a sample of galaxy clusters via the Sunyaev-Zel'dovich (SZ)
effect, and show five clusters previously detected with X-ray or SZ
observations. We provide integrated Compton-y measurements for each cluster. Of
particular interest is our detection of the z = 0.44 component of A3128 and our
current non-detection of the low-redshift part, providing strong evidence that
the further cluster is more massive as suggested by X-ray measurements. This is
a compelling example of the redshift-independent mass selection of the SZ
effect.Comment: 16 pages, 10 figures. Accepted for publication in ApJS. See Marriage
et al. (arXiv:1010.1065) and Menanteau et al. (arXiv:1006.5126) for
additional cluster result
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