124 research outputs found
A Bayesian approach to high fidelity interferometric calibration II: demonstration with simulated data
In a companion paper, we presented BayesCal, a mathematical formalism for
mitigating sky-model incompleteness in interferometric calibration. In this
paper, we demonstrate the use of BayesCal to calibrate the degenerate gain
parameters of full-Stokes simulated observations with a HERA-like hexagonal
close-packed redundant array, for three assumed levels of completeness of the a
priori known component of the calibration sky model. We compare the BayesCal
calibration solutions to those recovered by calibrating the degenerate gain
parameters with only the a priori known component of the calibration sky model
both with and without imposing physically motivated priors on the gain
amplitude solutions and for two choices of baseline length range over which to
calibrate. We find that BayesCal provides calibration solutions with up to four
orders of magnitude lower power in spurious gain amplitude fluctuations than
the calibration solutions derived for the same data set with the alternate
approaches, and between and times smaller than in the
mean degenerate gain amplitude on the full range of spectral scales accessible
in the data. Additionally, we find that in the scenarios modelled only BayesCal
has sufficiently high fidelity calibration solutions for unbiased recovery of
the 21 cm power spectrum on large spectral scales (). In all other cases, in the completeness regimes
studied, those scales are contaminated
Evaluating Diet Composition of Pronghorn in Wind Cave National Park, South Dakota
The pronghorn (Antilocapra americana) was reintroduced into Wind Cave National Park (WCNP), South Dakota, in 1914, and thus, has inhabited the Park for nearly a century. During the 1990\u27s, a decline in the population raised concern for the continued existence of pronghorn inside WCNP; an investigation into the observed decline was initiated. Primary objectives of our study were to evaluate diet composition and forage selection by pronghorn in WCNP. Microhistological analysis was conducted on 58 fecal samples collected opportunistically from pronghorn during 2002. Blue grama (Bouteloua gracilis), common juniper (Juniperus communis), and northern bedstraw (Galium boreale) were identified as major seasonal food items, representing 14.6, l 0.6, and 6.5 % of the annual diet, respectively. Annual diets of pronghorn in WCNP included 41.5% grasses, 31.1% shrubs, and 27.4% forbs. Total forage production in WCNP was 2% grass, 4% shrubs, and 23% forbs. Results indicated strong dietary selection by pronghorn for shrubs
Determining the Hubble constant from gravitational wave observations of merging compact binaries
Recent observations have accumulated compelling evidence that some short gamma-ray bursts (SGRBs) are associated with the mergers of neutron star (NS) binaries. This would indicate that the SGRB event is associated with a gravitational-wave (GW) signal corresponding to the final inspiral of the compact binary. In addition, the radioactive decay of elements produced in NS binary mergers may result in transients visible in the optical and infrared with peak luminosities on hours-days timescales. Simultaneous observations of the inspiral GWs and signatures in the electromagnetic band may allow us to directly and independently determine both the luminosity distance and redshift to a binary. These standard sirens (the GW analog of standard candles) have the potential to provide an accurate measurement of the low-redshift Hubble flow. In addition, these systems are absolutely calibrated by general relativity, and therefore do not experience the same set of astrophysical systematics found in traditional standard candles, nor do the measurements rely on a distance ladder. We show that 15 observable GW and EM events should allow the Hubble constant to be measured with 5% precision using a network of detectors that includes advanced LIGO and Virgo. Measuring 30 beamed GW-SGRB events could constrain H_0 to better than 1%. When comparing to standard Gaussian likelihood analysis, we find that each event's non-Gaussian posterior in H_0 helps reduce the overall measurement errors in H_0 for an ensemble of NS binary mergers
Exploring short gamma-ray bursts as gravitational-wave standard sirens
Recent observations support the hypothesis that a large fraction of
"short-hard" gamma-ray bursts (SHBs) are associated with compact binary
inspiral. Since gravitational-wave (GW) measurements of well-localized
inspiraling binaries can measure absolute source distances, simultaneous
observation of a binary's GWs and SHB would allow us to independently determine
both its luminosity distance and redshift. Such a "standard siren" (the GW
analog of a standard candle) would provide an excellent probe of the relatively
nearby universe's expansion, complementing other standard candles. In this
paper, we examine binary measurement using a Markov Chain Monte Carlo technique
to build the probability distributions describing measured parameters. We
assume that each SHB observation gives both sky position and the time of
coalescence, and we take both binary neutron stars and black hole-neutron star
coalescences as plausible SHB progenitors. We examine how well parameters
particularly distance) can be measured from GW observations of SHBs by a range
of ground-based detector networks. We find that earlier estimates overstate how
well distances can be measured, even at fairly large signal-to-noise ratio. The
fundamental limitation to determining distance proves to be a degeneracy
between distance and source inclination. Overcoming this limitation requires
that we either break this degeneracy, or measure enough sources to broadly
sample the inclination distribution. (Abridged)Comment: 19 pages, 10 figures. Accepted for publication in ApJ; this version
incorporates referee's comments and criticism
972-107 L-Arginine Decreases Infarct Size in Rats Exposed to Environmental Tobacco Smoke
We previously showed that environmental tobacco smoke (ETS) increased myocardial infarct size in a rat model of ischemia and reperfusion. If reduced reperfusion was caused by endothelial cell damage and increased vascular tone, we postulated that L-arginine (ARG) would increase nitric oxide and better protect the heart. 60 rats were randomly divided into 4 groups: ETS or Control (C) with and without ARG (2.25% ARG in drinking water). The ETS groups were exposed (4 Marlboro cigarettes per 15 minutes. 6 hours a day) for 6 weeks. During ETS-exposure, average air nicotine, carbon monoxide and total particulate concentrations were 1304 μg/m3, 78 ppm and 31 mg/m3, respectively. After 6 weeks, all rats were subjected to 35 min LAD occlusion (0) and 120 min reperfusion, with hemodynamic monitoring via the carotid artery. Aortic rings were harvested to evaluate vascular reactivity. Infarct size (infarct mass/risk area x 100%) decreased significantly in the ETS with ARG group compared to the ETS without ARG group. There were no significant differences among groups in heart rate (HR), systolic pressure (SP), and rate pressure product. Tlere were positive correlations between infarct size and heart rates from baseline to reperfusion 120 min (r = 0.4-0.6. p = 0.01-0.001). There was no relationship between vascular reactivity and infarct size.GroupNo. of RatsInf/LV (%)Inf/RA (%)0-35’HR (beats/m)0-35'SP (mmHg)Max Relax (%)C1125±351±6408±11120±784±11C+ ARG1025±252±3415±10103±11112±15ETS1034±464±6427±16108±8128±16ETS + ARG1122±3*42±6*410±17106±10127±18Values are Means±SEM*p<0.05, p values from two-way ANOVAConclusionL-arginine decreases myocardial infarct size after ischemia and reperfusion in ETS-exposed rats. This effect does not appear to be secondary to alterations in hemodynamics
Precision Epoch of Reionization studies with next-generation CMB experiments
Future arcminute resolution polarization data from ground-based Cosmic
Microwave Background (CMB) observations can be used to estimate the
contribution to the temperature power spectrum from the primary anisotropies
and to uncover the signature of reionization near in the small
angular-scale temperature measurements. Our projections are based on combining
expected small-scale E-mode polarization measurements from Advanced ACTPol in
the range with simulated temperature data from the full Planck
mission in the low and intermediate region, . We show that
the six basic cosmological parameters determined from this combination of data
will predict the underlying primordial temperature spectrum at high multipoles
to better than accuracy. Assuming an efficient cleaning from
multi-frequency channels of most foregrounds in the temperature data, we
investigate the sensitivity to the only residual secondary component, the
kinematic Sunyaev-Zel'dovich (kSZ) term. The CMB polarization is used to break
degeneracies between primordial and secondary terms present in temperature and,
in effect, to remove from the temperature data all but the residual kSZ term.
We estimate a detection of the diffuse homogeneous kSZ signal from
expected AdvACT temperature data at , leading to a measurement of
the amplitude of matter density fluctuations, , at precision.
Alternatively, by exploring the reionization signal encoded in the patchy kSZ
measurements, we bound the time and duration of the reionization with
and . We find that
these constraints degrade rapidly with large beam sizes, which highlights the
importance of arcminute-scale resolution for future CMB surveys.Comment: 10 pages, 10 figure
MeerKLASS: MeerKAT Large Area Synoptic Survey
We discuss the ground-breaking science that will be possible with a wide area
survey, using the MeerKAT telescope, known as MeerKLASS (MeerKAT Large Area
Synoptic Survey). The current specifications of MeerKAT make it a great fit for
science applications that require large survey speeds but not necessarily high
angular resolutions. In particular, for cosmology, a large survey over for hours will potentially provide the first
ever measurements of the baryon acoustic oscillations using the 21cm intensity
mapping technique, with enough accuracy to impose constraints on the nature of
dark energy. The combination with multi-wavelength data will give unique
additional information, such as exquisite constraints on primordial
non-Gaussianity using the multi-tracer technique, as well as a better handle on
foregrounds and systematics. Such a wide survey with MeerKAT is also a great
match for HI galaxy studies, providing unrivalled statistics in the pre-SKA era
for galaxies resolved in the HI emission line beyond local structures at z >
0.01. It will also produce a large continuum galaxy sample down to a depth of
about 5\,Jy in L-band, which is quite unique over such large areas and
will allow studies of the large-scale structure of the Universe out to high
redshifts, complementing the galaxy HI survey to form a transformational
multi-wavelength approach to study galaxy dynamics and evolution. Finally, the
same survey will supply unique information for a range of other science
applications, including a large statistical investigation of galaxy clusters as
well as produce a rotation measure map across a huge swathe of the sky. The
MeerKLASS survey will be a crucial step on the road to using SKA1-MID for
cosmological applications and other commensal surveys, as described in the top
priority SKA key science projects (abridged).Comment: Larger version of the paper submitted to the Proceedings of Science,
"MeerKAT Science: On the Pathway to the SKA", Stellenbosch, 25-27 May 201
Simulating the detection of the global 21 cm signal with MIST for different models of the soil and beam directivity
The Mapper of the IGM Spin Temperature (MIST) is a new ground-based,
single-antenna, radio experiment attempting to detect the global 21 cm signal
from the Dark Ages and Cosmic Dawn. A significant challenge in this measurement
is the frequency-dependence, or chromaticity, of the antenna beam directivity.
MIST observes with the antenna above the soil and without a metal ground plane,
and the beam directivity is sensitive to the electrical characteristics of the
soil. In this paper, we use simulated observations with MIST to study how the
detection of the global 21 cm signal from Cosmic Dawn is affected by the soil
and the MIST beam directivity. We simulate observations using electromagnetic
models of the directivity computed for single- and two-layer models of the
soil. We test the recovery of the Cosmic Dawn signal with and without beam
chromaticity correction applied to the simulated data. We find that our
single-layer soil models enable a straightforward recovery of the signal even
without chromaticity correction. Two-layer models increase the beam
chromaticity and make the recovery more challenging. However, for the model in
which the bottom soil layer has a lower electrical conductivity than the top
layer, the signal can be recovered even without chromaticity correction. For
the other two-layer models, chromaticity correction is necessary for the
recovery of the signal and the accuracy requirements for the soil parameters
vary between models. These results will be used as a guideline to select
observation sites that are favorable for the detection of the Cosmic Dawn
signal.Comment: Accepted for publication in the Astrophysical Journa
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