A Template-based UHE Neutrino Search Strategy for the Askaryan Radio Array (ARA)

The Askaryan Radio Array (ARA) is a gigaton-size neutrino radio telescope located near the geographic South Pole. ARA has five independent stations designed to detect Askaryan emission coming from the interactions between ultra-high energy neutrinos (> 10 PeV) and Antarctic ice. Each station includes of 16 antenna deployed in a matrix shape at up to 200 m deep in the ice. A simulated neutrino template, including the detector response model, was implemented in a new search technique for reducing background noise and improving the vertex reconstruction resolution. The template is used to scan through the data using the matched filter method, inspired by LIGO, looking for a low SNR neutrino signature and ultimately aiming to lower the detector’s energy threshold at the analysis level. I will present the estimated sensitivity improvements to ARA analyses through the application of the template technique with results from simulation

The Calibration of the Geometry and Antenna delay in Askaryan Radio Array Station 4 and 5

The Askaryan Radio Array (ARA) experiment at the South Pole is designed to detect the radio signals produced by ultra high energy cosmic neutrino interactions in the ice. There are 5 independent ARA stations, one of which (A5) includes a low-threshold phased array trigger string. Each ARA station is designed to work as an autonomous detector. The Data Acquisition System in all ARA stations is equipped with the Ice Ray Sampler second-generation (IRS2) chip, a custom-made, application-specific integrated circuit (ASIC) for high-speed sampling and digitization. In this contribution, we describe the methodology used to calibrate the IRS2 digitizer chip and the station geometry, namely the relative timing between each pair of ARA antennas, deployed at 200 m below the Antarctic ice surface, and their geometrical positions in the ice, for ARA stations 4 and 5. Our calibration allows for proper timing correlations between incoming signals, which is crucial for radio vertex reconstruction and thus detection of ultra high energy neutrinos through the Askaryan effect. We achieve a signal timing precision on a sub-nanosecond level and an antenna position precision within 10 cm

Analyzing Stakeholder Water Source Preference Based upon Social Capital: a Case Study of the Fajr Jam Gas Refinery in Iran

Gas refineries are among the most water-intensive industries in the world. The Fajr Jam gas refinery is one such example, located in the southern Iran. The indiscriminate use of aquifer resources for this highly profitable industry creates tragedy of the commons effects, causing significant environmental controversy and threatening the long-term water security of the region. It behooves decision makers, therefore, to examine a broad range of adaptive water management strategies for this industry. The implementation of such strategies requires understanding the preferences and potential conflicts that may emerge among competing stakeholder interests. This quantitative social scientific study examines stakeholder preferences among water management options through the lens of social capital. Elite stakeholder representatives (including agricultural organizations, governmental organizations, the Water, and Power Authority, Department of Health, Bureau of Water and Wastewater) were canvassed through a survey instrument using paired comparisons. Data were analyzed using Expert Choice software and an analytic hierarchy process technique. The results show that accountability is the main criterion for selecting the best water sources and ranked first with the Eigenvector 0.62. Also, the results show that the least important criterion was social cohesion with the Eigenvalue 0.033. The criteria of partnership and trust ranked as two and three with Eigenvalues 0.215 and 0.133, respectively. The results indicate that the construction of salt water transmission from the sea (A = 0.240) is the preferred option among other alternatives, and this is confirmed by sensitivity analysis

Multi-messenger observations of a binary neutron star merger

On 2017 August 17 a binary neutron star coalescence candidate (later designated GW170817) with merger time 12:41:04 UTC was observed through gravitational waves by the Advanced LIGO and Advanced Virgo detectors. The Fermi Gamma-ray Burst Monitor independently detected a gamma-ray burst (GRB 170817A) with a time delay of ~1.7 s with respect to the merger time. From the gravitational-wave signal, the source was initially localized to a sky region of 31 deg2 at a luminosity distance of 40+8-8 Mpc and with component masses consistent with neutron stars. The component masses were later measured to be in the range 0.86 to 2.26 Mo. An extensive observing campaign was launched across the electromagnetic spectrum leading to the discovery of a bright optical transient (SSS17a, now with the IAU identification of AT 2017gfo) in NGC 4993 (at ~40 Mpc) less than 11 hours after the merger by the One- Meter, Two Hemisphere (1M2H) team using the 1 m Swope Telescope. The optical transient was independently detected by multiple teams within an hour. Subsequent observations targeted the object and its environment. Early ultraviolet observations revealed a blue transient that faded within 48 hours. Optical and infrared observations showed a redward evolution over ~10 days. Following early non-detections, X-ray and radio emission were discovered at the transient’s position ~9 and ~16 days, respectively, after the merger. Both the X-ray and radio emission likely arise from a physical process that is distinct from the one that generates the UV/optical/near-infrared emission. No ultra-high-energy gamma-rays and no neutrino candidates consistent with the source were found in follow-up searches. These observations support the hypothesis that GW170817 was produced by the merger of two neutron stars in NGC4993 followed by a short gamma-ray burst (GRB 170817A) and a kilonova/macronova powered by the radioactive decay of r-process nuclei synthesized in the ejecta

Search for transient optical counterparts to high-energy IceCube neutrinos with Pan-STARRS1

In order to identify the sources of the observed diffuse high-energy neutrino flux, it is crucial to discover their electromagnetic counterparts. To increase the sensitivity of detecting counterparts of transient or variable sources by telescopes with a limited field of view, IceCube began releasing alerts for single high-energy (E-v > 60 TeV) neutrino detections with sky localisation regions of order 1 degrees radius in 2016. We used Pan-STARRS1 to follow-up five of these alerts during 2016-2017 to search for any optical transients that may be related to the neutrinos. Typically 10-20 faint m(ip1) less than or similar to 22.5 mag) extragalactic transients are found within the Pan-STARRS1 footprints and are generally consistent with being unrelated field supernovae (SNe) and AGN. We looked for unusual properties of the detected transients, such as temporal coincidence of explosion epoch with the IceCube timestamp, or other peculiar light curve and physical properties. We found only one transient that had properties worthy of a specific follow-up. In the Pan-STARRS1 imaging for IceCube-160427A (probability to be of astrophysical origin of similar to 50%), we found a SN PS16cgx, located at 10.0' from the nominal IceCube direction. Spectroscopic observations of PS16cgx showed that it was an H-poor SN at redshift z = 0.2895 +/- 0.0001. The spectra and light curve resemble some high-energy Type Ic SNe, raising the possibility of a jet driven SN with an explosion epoch temporally coincident with the neutrino detection. However, distinguishing Type Ia and Type Ic SNe at this redshift is notoriously difficult. Based on all available data we conclude that the transient is more likely to be a Type Ia with relatively weak Sin absorption and a fairly normal rest-frame r-band light curve. If, as predicted, there is no high-energy neutrino emission from Type Ia SNe, then PS16cgx must be a random coincidence, and unrelated to the IceCube-160427A. We find no other plausible optical transient for any of the five IceCube events observed down to a 5 sigma limiting magnitude of mip1 approximate to 22 mag, between 1 day and 25 days after detection

Communication about environmental health risks: a systematic review.

BACKGROUND: Using the most effective methods and techniques for communicating risk to the public is critical. Understanding the impact that different types of risk communication have played in real and perceived public health risks can provide information about how messages, policies and programs can and should be communicated in order to be most effective. The purpose of this systematic review is to identify the effectiveness of communication strategies and factors that impact communication uptake related to environmental health risks. METHODS: A systematic review of English articles using multiple databases with appropriate search terms. Data sources also included grey literature. Key organization websites and key journals were hand searched for relevant articles. Consultation with experts took place to locate any additional references.Articles had to meet relevance criteria for study design [randomized controlled trials, clinical controlled trials, cohort analytic, cohort, any pre-post, interrupted time series, mixed methods or any qualitative studies), participants (those in community-living, non-clinical populations), interventions (including, but not limited to, any community-based methods or tools such as Internet, telephone, media-based interventions or any combination thereof), and outcomes (reported measurable outcomes such as awareness, knowledge or attitudinal or behavioural change). Articles were assessed for quality and data was extracted using standardized tools by two independent reviewers. Articles were given an overall assessment of strong, moderate or weak quality. RESULTS: There were no strong or moderate studies. Meta-analysis was not appropriate to the data. Data for 24 articles were analyzed and reported in a narrative format. The findings suggest that a multi-media approach is more effective than any single media approach. Similarly, printed material that offers a combination of information types (i.e., text and diagrams) is a more effective than just a single type, such as all text. Findings also suggest that factors influencing response to risk communications are impacted by personal risk perception, previous personal experience with risk, sources of information and trust in those sources. CONCLUSIONS: No single method of message delivery is best. Risk communication strategies that incorporate the needs of the target audience(s) with a multi-faceted delivery method are most effective at reaching the audience

Mechanisms leading to increased vasodilator responses to calcitonin-gene-related peptide in mesenteric resistance arteries of early pregnant rats.

Contains fulltext : 69189.pdf (publisher's version ) (Closed access)The objective of this study was to explore the mechanism responsible for the higher relaxing responses of mesenteric arteries to calcitonin-gene-related peptide (CGRP) in pregnancy. We performed myograph and ligand binding studies to determine the role of matrix metalloproteinase-2 (MMP-2) and CGRP receptor density. MMP activity was manipulated in isolated arteries by exposing them to the blocking effects of doxycycline. Vascular activity of MMP-2 was studied by gelatin zymography, and CGRP receptor density was determined by ligand binding analysis. Compared to nonpregnant rats, CGRP elicited stronger arterial relaxation in pregnant rats. The latter effect was neither accompanied by a change in relaxing responses to direct activation of adenylyl cyclase by forskolin nor by a change in the response to stimulation of G-protein-coupled adrenergic receptors by isoproterenol. Doxycycline did not affect the stronger arterial relaxation in pregnancy in spite of the observed more than threefold higher arterial MMP-2 activity. Density of binding sites for [(125)I]CGRP in arteries from pregnant rats (64 +/- 14 fmol/mg protein) and from virgin rats (54 +/- 5 fmol/mg protein) were comparable. The results of this study provide evidence for increased coupling of CGRP receptors to adenylyl cyclase in early pregnancy

Comparison of bedtime rest classification from accelerometer placed on waist or wrist in the development and validation groups with classification obtained using whole- room indirect calorimeter.

a<p>– Area under the ROC curve calculated as sensitivity multiplied by specificity before data was rounded;</p>b<p>- defined as the probability of correctly classifying bedtime rest period;</p>c<p>- defined as a probability of correctly classifying activity period;</p>d<p>- Wilcoxon signed rank test;</p>e<p>- automated computer algorithm;</p>f<p>- cut points were 20 counts/min (bedtime) and 500 counts/min (activity);</p>g<p>- cut points were 250 counts/min (bedtime) and 3000 counts/min (activity).</p

Electroweak parameters of the z0 resonance and the standard model

Contains fulltext : 124399.pdf (publisher's version ) (Open Access