A hierarchical method for vetoing noise transients in gravitational-wave detectors

Non-Gaussian noise transients in interferometric gravitational-wave detectors increase the background in searches for short-duration and un-modelled signals. We describe a method for vetoing noise transients by ranking the statistical relationship between triggers in auxiliary channels that have negligible sensitivity to gravitational waves and putative gravitational-wave triggers in the detector output. The novelty of the algorithm lies in its hierarchical approach, which leads to a minimal set of veto conditions with high performance and low deadtime. After a given channel has been selected it is used to veto triggers from the detector output, then the algorithm selects a new channel that performs well on the remaining triggers and the process is repeated. This method has been demonstrated to reduce the background in searches for transient gravitational waves by the LIGO and Virgo collaborations.Comment: 13 page

Evaluation of Bilayer Silk Fibroin Grafts for Tubular Esophagoplasty in a Porcine Defect Model.

Surgical reconstruction of tubular esophageal defects with autologous gastrointestinal segments is the gold standard treatment to replace damaged or diseased esophageal tissues. Unfortunately, this approach is associated with adverse complications, including dysphagia, donor-site morbidity, and in some cases patient death. Bilayer silk fibroin (BLSF) scaffolds were investigated as alternative, acellular grafts for tubular esophagoplasty in a porcine defect model for 3 months of implantation. Adult Yucatan mini-swine (n = 5) were subjected to esophageal reconstruction with tubular BLSF grafts (2 cm in length) in combination with transient esophageal stenting for 2 months followed by a 1-month period, where the graft site was unstented. All animals receiving BLSF grafts survived and were capable of solid food consumption, however strictures were noted at graft regions in 60% of the experimental cohort between 2 and 3 months postop and required balloon dilation. In addition, fluoroscopic analysis showed peristaltic function in only 1/5 neotissues. Following swine harvest at 3 months, ex vivo tissue bath evaluations revealed that neoconduits exhibited contractile responses to carbachol, electric field stimulation, and KCl, whereas sodium nitroprusside and isoproterenol induced relaxation effects. Histological (Masson's Trichrome) and immunohistochemical analyses of regenerated tissue conduits showed a stratified, squamous epithelium expressing pan-cytokeratins buttressed by a vascularized lamina propria containing a smooth muscle-rich muscularis mucosa surrounded by a muscularis externa. Neuronal density, characterized by the presence of synaptophysin-positive boutons, was significantly lower in neotissues in comparison to nonsurgical controls. BLSF scaffolds represent a promising platform for the repair of tubular esophageal defects, however improvements in scaffold design are needed to reduce the rate of complications and improve the extent of constructive tissue remodeling. Impact statement The search for a superior "off-the-shelf" scaffold capable of repairing tubularesophageal defects as well as overcoming limitations associated with conventional autologous gastrointestinal segments remains elusive. The purpose of this study was to investigate the performance of an acellular, bilayer silk fibroin graft (BLSF) for tubular esophagoplasty in a porcine model. Our results demonstrated that BLSF scaffolds supported the formation of tubular neotissues with innervated, vascularized epithelial and muscular components capable of contractile and relaxation responses. BLSF scaffolds represent a promising platform for esophageal tissue engineering

Identifying correlations between LIGO's astronomical range and auxiliary sensors using lasso regression

The range to which the Laser Interferometer Gravitational-Wave Observatory (LIGO) can observe astrophysical systems varies over time, limited by noise in the instruments and their environments. Identifying and removing the sources of noise that limit LIGO's range enables higher signal-to-noise observations and increases the number of observations. The LIGO observatories are continuously monitored by hundreds of thousands of auxiliary channels that may contain information about these noise sources. This paper describes an algorithm that uses linear regression, namely lasso (least absolute shrinkage and selection operator) regression, to analyze all of these channels and identify a small subset of them that can be used to reconstruct variations in LIGO's astrophysical range. Exemplary results of the application of this method to three different periods of LIGO Livingston data are presented, along with computational performance and current limitations

The PyCBC search for gravitational waves from compact binary coalescence

We describe the PyCBC search for gravitational waves from compact-object binary coalescences in advanced gravitational-wave detector data. The search was used in the first Advanced LIGO observing run and unambiguously identified two black hole binary mergers, GW150914 and GW151226. At its core, the PyCBC search performs a matched-filter search for binary merger signals using a bank of gravitational-wave template waveforms. We provide a complete description of the search pipeline including the steps used to mitigate the effects of noise transients in the data, identify candidate events and measure their statistical significance. The analysis is able to measure false-alarm rates as low as one per million years, required for confident detection of signals. Using data from initial LIGO's sixth science run, we show that the new analysis reduces the background noise in the search, giving a 30% increase in sensitive volume for binary neutron star systems over previous searches.Comment: 29 pages, 7 figures, accepted by Classical and Quantum Gravit

2006 SQ372: A Likely Long-Period Comet from the Inner Oort Cloud

We report the discovery of a minor planet (2006 SQ372) on an orbit with a perihelion of 24 AU and a semimajor axis of 796 AU. Dynamical simulations show that this is a transient orbit and is unstable on a timescale of 200 Myrs. Falling near the upper semimajor axis range of the scattered disk and the lower semimajor axis range of the Oort Cloud, previous membership in either class is possible. By modeling the production of similar orbits from the Oort Cloud as well as from the scattered disk, we find that the Oort Cloud produces 16 times as many objects on SQ372-like orbits as the scattered disk. Given this result, we believe this to be the most distant long-period comet ever discovered. Furthermore, our simulation results also indicate that 2000 OO67 has had a similar dynamical history. Unaffected by the "Jupiter-Saturn Barrier," these two objects are most likely long-period comets from the inner Oort Cloud

Northern SPIRIT Consortium - Canadian Collaboration through Student-Led CubeSat Constellation

The Northern Space Program for Innovative Research and Integrated Training (Northern SPIRIT) is a unique collaboration of three Canadian post-secondary institutions that will design, build, and operate a constellation of three CubeSats. The consortium, beginning in 2017, comprises Yukon University, Aurora College, and the University of Alberta (U of A). The partnership will develop three CubeSats: YukonSat (2U), AuroraSat (2U) and Ex-Alta 2 (3U) which will be launched into Low Earth Orbit in 2022. Northern SPIRIT strives to use space technology development to inspire motivated youth across Canada to engage in student-led collaboration and hands-on education, research, training, and to amplify Northern Canadian voices. Supported by the Canadian Space Agency (CSA) through the Canadian CubeSat Project (CCP), Northern SPIRIT will help further the CSAs goal of making space more accessible throughout Canada. The constellation mission will support a range of educational payloads dedicated to the expansion of STEM, arts, and language outreach opportunities. They also introduce passionate k-12 students to hands-on experiences with space mission concepts such as operations, coding, and data analytics. AuroraSat’s mission objective is educational outreach directed at sharing Northern art, languages, and history. Northern Images Mission will host a screen and an imager which will capture artwork created by Northern Artists backdropped by the Earth’s horizon. Northern Voices Mission will broadcast Northern Canadian stories of the space and sky, read by students, on amateur radio bands from all three satellites. Finally, the Northern Games Mission will transmit partial messages (focusing on Northern history) from the three satellites in select geographic zones, requiring global cooperation between amateur radio operators to decode a whole message. YukonSat will provide the novel opportunity to expand the capacity of highly qualified space science personnel in the Yukon, while furthering space science engagement and education of the public. The satellite’s payload will host a robotic arm, an OLED screen, camera, and a sensor array for attitude determination. The robotic arm allows freedom to point remote sensing equipment without using the spacecraft attitude determination and control system. The OLED screen and camera will display and photograph student-made Northern art with the Earth and space in the background. Ex-Alta 2 will host a multispectral imaging payload with the mission objective to study wildfires. A secondary science objective on all three satellites is space weather monitoring using a Digital Fluxgate Magnetometer that was designed and built at the U of A. In addition to this inter-institutional coordination, the U of A-designed 3U bus has been adapted into a 2U version to be used on the other two satellites in the constellation. The partnership amongst the three institutions supports collaboration in remote communities across Provincial & Territorial borders, advancing Canada’s contribution to the space industry and showcasing the exciting possibilities for interdisciplinary, national partnership. Extending across Canada, the consortium strives to inspire and enable passionate students to celebrate the Canadian voice and pursue opportunities in the space industry. In partnership with the CSA, Northern SPIRIT is a frontrunner in the exciting upward trend of the democratization of space

hCALCRL mutation causes autosomal recessive nonimmune hydrops fetalis with lymphatic dysplasia

We report the first case of nonimmune hydrops fetalis (NIHF) associated with a recessive, in-frame deletion of V205 in the G protein–coupled receptor, Calcitonin Receptor-Like Receptor (hCALCRL). Homozygosity results in fetal demise from hydrops fetalis, while heterozygosity in females is associated with spontaneous miscarriage and subfertility. Using molecular dynamic modeling and in vitro biochemical assays, we show that the hCLR(V205del) mutant results in misfolding of the first extracellular loop, reducing association with its requisite receptor chaperone, receptor activity modifying protein (RAMP), translocation to the plasma membrane and signaling. Using three independent genetic mouse models we establish that the adrenomedullin–CLR–RAMP2 axis is both necessary and sufficient for driving lymphatic vascular proliferation. Genetic ablation of either lymphatic endothelial Calcrl or nonendothelial Ramp2 leads to severe NIHF with embryonic demise and placental pathologies, similar to that observed in humans. Our results highlight a novel candidate gene for human congenital NIHF and provide structure–function insights of this signaling axis for human physiology