A5079641435- Galaxies: Formation, Evolution, Phenomena
- Bacillus and Francisella bacterial research
- Technology Assessment and Management
- Cardiac, Anesthesia and Surgical Outcomes
- Disaster Response and Management
- Impact of Light on Environment and Health
- Chemical Safety and Risk Management
- Defense, Military, and Policy Studies
- Astrophysical Phenomena and Observations
- Ultrasound in Clinical Applications
- Advanced Chemical Sensor Technologies
- Adaptive optics and wavefront sensing
- Neurology and Historical Studies
- Stroke Rehabilitation and Recovery
- Cosmology and Gravitation Theories
- Infection Control in Healthcare
- Chemotherapy-related skin toxicity
- Opportunistic and Delay-Tolerant Networks
- 3D Printing in Biomedical Research
- Milk Quality and Mastitis in Dairy Cows
- Information and Cyber Security
- Laser-Ablation Synthesis of Nanoparticles
- Forensic Toxicology and Drug Analysis
- Food Chemistry and Fat Analysis
- Space Science and Extraterrestrial Life
Pennsylvania State University
2022-2024
Colorado State University
2022
Centre for Life
2020
York Teaching Hospital NHS Foundation Trust
2018-2020
Raigmore Hospital
2014
NHS Education for Scotland
2014
Glasgow Royal Infirmary
2013
University of Glasgow
2013
Minnesota Veterans Medical Research and Education Foundation
1998
Changing-look quasars exhibit dramatic variability in broad emission-line fluxes on short timescales. This behavior is challenging to many models of the quasar line region, due large part transition times between high and low states. In order constrain cause variability, we obtained contemporaneous Hubble Space Telescope UV Hobby Eberly optical spectra three changing-look caught their state. We use these spectra, along with archival taken during both states, investigate potential scenarios...
Abstract Changing-look quasars (CLQs) exhibit dramatic variability in broad emission-line fluxes on short timescales. This behavior is challenging to many models of the quasar broad-line region, due large part transition times between high and low states. In order constrain cause variability, we obtained contemporaneous Hubble Space Telescope ultraviolet Hobby Eberly optical spectra three CLQs caught their state. We use these spectra, along with archival taken during both states, investigate...
Stars provide an enormous gain for interstellar communications at their gravitational focus, perhaps as part of network. If the Sun is such a network, there should be probes foci nearby stars. are within solar system connected to we might detect them by intercepting transmissions from relays these foci. Here, demonstrate search across wide bandwidth communication beyond Sun's innermost focus 550 AU using Green Bank Telescope (GBT) and Breakthrough Listen (BL) backend. As first target,...
Abstract This article sets out a summary of standards for departmental accreditation set by the British Society Echocardiography (BSE) Departmental Accreditation Committee. Full are available at www.bsecho.org . The BSE were first national organisation to establish quality framework departments that support practice individual echocardiographers. is an updated version which recognises that, not only should all echocardiographers be individually accredited as competent practice, but also need...
ABSTRACT The effect of dust attenuation on a galaxy’s light depends number physical properties, such as geometry and composition, both which can vary across the faces galaxies. To investigate this variation, we continue analysis star-forming regions in 29 galaxies studied previously. We analyse these using Swift/UV Optical Telescope Wide-field Infrared Survey Explorer images, well Sloan Digital Sky Survey/Mapping Nearby Galaxies at Apache Point Observatory emission line maps to constrain...
The next space race has begun. Plans are well underway to establish architectures in cislunar space. This paper provides a summary of research conducted on architectures, including primary missions, and supporting functions. Planned missions can be broadly categorized as science, commercial, defense missions. Supporting functions transportation, communication, navigation, domain awareness, service, energy, shelter, control. Potential solutions identified gaps for each mission function is...
Abstract Background : Quality assurance (QA) of echocardiographic studies is vital to ensure that clinicians can act on findings high quality deliver excellent patient care. To date, there a paucity published guidance how perform this QA. The British Society Echocardiography (BSE) has previously produced an Framework (EQF) assist departments with their QA processes. This article expands the EQF structured yet versatile approach analyse high-quality standards are met. In addition, process...
Ronald MacVicar and colleagues describe an initiative that is including trainees in the drive to improve recruitment medical posts Scotland
Those who attended the Inaugural Integrative Medicine Research Forum hosted by Osher Center for at Harvard Medical School (HMS) and Brigham Women's Hospital, Boston, Masssachusetts, had unique experience of viewing an interactive research network, 670 individuals representing 19 different institutions, seeing poster presentations from 38 investigators, hearing that described impressive clinical educational programs are underway in Boston area. Throughout proceedings, two themes emerged:...
The effect of dust attenuation on a galaxy's light depends number physical properties, such as geometry and composition, both which can vary across the faces galaxies. To investigate this variation, we continue analysis star-forming regions in 29 galaxies studied previously. We analyse these using Swift/UVOT WISE images, well SDSS/MaNGA emission line maps to constrain relationship between infrared excess (IRX) UV spectral index (beta) for each star forming region. This be used law is...
Abstract We present the new Swift/UVOT+MaNGA (SwiM) catalog (SwiM_v4.1). SwiM_v4.1 is designed to study star formation and dust attenuation within nearby galaxies given unique overlap of Swift/UVOT near-ultraviolet (NUV) imaging MaNGA integral field optical spectroscopy. comprises 559 objects, ∼4 times more than original SwiM (SwiM_v3.1), spans redshift range z ≈ 0.0002–0.1482, provides a diverse rich sample. Approximately 5% final sample included in SwiM_v4.1, 42% are cross-listed with...