| 1. |
- Burgess, J. Michael, et al.
(författare)
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AN OBSERVED CORRELATION BETWEEN THERMAL AND NON-THERMAL EMISSION IN GAMMA-RAY BURSTS
- 2014
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Ingår i: Astrophysical Journal Letters. - 2041-8205 .- 2041-8213. ; 784:2
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Tidskriftsartikel (refereegranskat)abstract
- Recent observations by the Fermi Gamma-ray Space Telescope have confirmed the existence of thermal and non-thermal components in the prompt photon spectra of some gamma-ray bursts (GRBs). Through an analysis of six bright Fermi GRBs, we have discovered a correlation between the observed photospheric and non-thermal gamma-ray emission components of several GRBs using a physical model that has previously been shown to be a good fit to the Fermi data. From the spectral parameters of these fits we find that the characteristic energies, E-p and kT, of these two components are correlated via the relation E-p proportional to T-alpha which varies from GRB to GRB. We present an interpretation in which the value of the index alpha indicates whether the jet is dominated by kinetic or magnetic energy. To date, this jet composition parameter has been assumed in the modeling of GRB outflows rather than derived from the data.
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| 2. |
- Burgess, J Michael, et al.
(författare)
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Constraints on the Synchrotron Shock Model for the Fermi GRB 090820A Observed by Gamma-Ray Burst Monitor
- 2011
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Ingår i: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 741:1
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Tidskriftsartikel (refereegranskat)abstract
- Discerning the radiative dissipation mechanism for prompt emission in gamma-ray bursts (GRBs) requires detailed spectroscopic modeling that straddles the vF(v) peak in the 100 keV-1 MeV range. Historically, empirical fits such as the popular Band function have been employed with considerable success in interpreting the observations. While extrapolations of the Band parameters can provide some physical insight into the emission mechanisms responsible for GRBs, these inferences do not provide a unique way of discerning between models. By fitting physical models directly, this degeneracy can be broken, eliminating the need for empirical functions; our analysis here offers a first step in this direction. One of the oldest, and leading, theoretical ideas for the production of the prompt signal is the synchrotron shock model. Here we explore the applicability of this model to a bright Fermi gamma-ray burst monitor (GBM) burst with a simple temporal structure, GRB 090820A. Our investigation implements, for the first time, thermal and non-thermal synchrotron emissivities in the RMFIT forward-folding spectral analysis software often used in GBM burst studies. We find that these synchrotron emissivities, together with a blackbody shape, provide at least as good a match to the data as the Band GRB spectral fitting function. This success is achieved in both time-integrated and time-resolved spectral fits.
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| 3. |
- Casey, Jillian P, et al.
(författare)
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A novel approach of homozygous haplotype sharing identifies candidate genes in autism spectrum disorder.
- 2012
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Ingår i: Human Genetics. - : Springer Science and Business Media LLC. - 0340-6717 .- 1432-1203. ; 131:4, s. 565-579
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Tidskriftsartikel (refereegranskat)abstract
- Autism spectrum disorder (ASD) is a highly heritable disorder of complex and heterogeneous aetiology. It is primarily characterized by altered cognitive ability including impaired language and communication skills and fundamental deficits in social reciprocity. Despite some notable successes in neuropsychiatric genetics, overall, the high heritability of ASD (~90%) remains poorly explained by common genetic risk variants. However, recent studies suggest that rare genomic variation, in particular copy number variation, may account for a significant proportion of the genetic basis of ASD. We present a large scale analysis to identify candidate genes which may contain low-frequency recessive variation contributing to ASD while taking into account the potential contribution of population differences to the genetic heterogeneity of ASD. Our strategy, homozygous haplotype (HH) mapping, aims to detect homozygous segments of identical haplotype structure that are shared at a higher frequency amongst ASD patients compared to parental controls. The analysis was performed on 1,402 Autism Genome Project trios genotyped for 1 million single nucleotide polymorphisms (SNPs). We identified 25 known and 1,218 novel ASD candidate genes in the discovery analysis including CADM2, ABHD14A, CHRFAM7A, GRIK2, GRM3, EPHA3, FGF10, KCND2, PDZK1, IMMP2L and FOXP2. Furthermore, 10 of the previously reported ASD genes and 300 of the novel candidates identified in the discovery analysis were replicated in an independent sample of 1,182 trios. Our results demonstrate that regions of HH are significantly enriched for previously reported ASD candidate genes and the observed association is independent of gene size (odds ratio 2.10). Our findings highlight the applicability of HH mapping in complex disorders such as ASD and offer an alternative approach to the analysis of genome-wide association data.
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| 4. |
- Fox, Siobhan, et al.
(författare)
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"Give me the knowledge, and I can do what I want with it, it's my right and my choice" : Triangulated perspectives on the disclosure of young onset dementia
- 2023
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Ingår i: Dementia. - : Sage Publications. - 1471-3012 .- 1741-2684. ; 22:8, s. 1757-1775
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Tidskriftsartikel (refereegranskat)abstract
- IntroductionReceiving a diagnosis of young onset dementia is particularly distressing; the person under 65 years is often in employment, with financial commitments, young children, and an active social life. Some of the stress experienced by younger people experiencing cognitive changes can be reduced by an early and accurate diagnosis, but this is contingent on the timing of disclosure and a process which is sensitive and appropriate to the person. The study aim was to explore experiences of giving and receiving a diagnosis of young onset dementia, by triangulating the perspectives of the key parties involved.MethodsA qualitative design was employed, using semi-structured interviews. Participants (N = 47) included people with young onset dementia (n = 10), family members (n = 12), and health and social care professionals (n = 25). Thematic analysis and triangulation enabled identification of overall themes across different participant groups.ResultsAll participant groups agreed on key aspects of good disclosure practice, with two overarching themes: The optimal conditions for disclosure, and how best to disclose a diagnosis. Positive experiences of disclosure were prefaced on having the appropriate space and time; having a support person present; clearly labelling the diagnosis; providing appropriate information at the right pace. Other findings include recommendations for longer appointment times, offering additional support for young families, and for carers of people with atypical presentations (e.g. frontotemporal dementia).ConclusionMany people with young onset dementia had unsatisfactory disclosure experiences. Health and social care professionals should provide a 'pre-disclosure' appointment, elicit the amount of information the person may want at the point of disclosure of the diagnosis, balance truth and hope, provide contact details for follow-up, and overall be mindful of the individual in front of them. While young onset dementia may be a life-altering diagnosis, a disclosure meeting which is sensitively undertaken can increase the person's agency, coping ability, and ultimately empower them to live well with their diagnosis.
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| 5. |
- Goldstein, Adam, et al.
(författare)
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The Fermi GBM Gamma-Ray Burst Spectral Catalog : The First Two Years
- 2012
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Ingår i: Astrophysical Journal Supplement Series. - : American Astronomical Society. - 0067-0049 .- 1538-4365. ; 199:1
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Tidskriftsartikel (refereegranskat)abstract
- We present systematic spectral analyses of gamma-ray bursts (GRBs) detected by the Fermi Gamma-Ray Burst Monitor (GBM) during its first two years of operation. This catalog contains two types of spectra extracted from 487 GRBs, and by fitting four different spectral models, this results in a compendium of over 3800 spectra. The models were selected based on their empirical importance to the spectral shape of many GRBs, and the analysis performed was devised to be as thorough and objective as possible. We describe in detail our procedure and criteria for the analyses, and present the bulk results in the form of parameter distributions. This catalog should be considered an official product from the Fermi GBM Science Team, and the data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center.
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| 6. |
- Guiriec, Sylvain, et al.
(författare)
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Detection of a thermal spectral component in the prompt emission of GRB 100724B
- 2011
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Ingår i: ASTROPHYSICAL JOURNAL LETTERS. - 2041-8205. ; 727:2, s. L33-
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Tidskriftsartikel (refereegranskat)abstract
- Observations of GRB 100724B with the Fermi Gamma-Ray Burst Monitor find that the spectrum is dominated by the typical Band functional form, which is usually taken to represent a non-thermal emission component, but also includes a statistically highly significant thermal spectral contribution. The simultaneous observation of the thermal and non-thermal components allows us to confidently identify the two emission components. The fact that these seem to vary independently favors the idea that the thermal component is of photospheric origin while the dominant non-thermal emission occurs at larger radii. Our results imply either a very high efficiency for the non-thermal process or a very small size of the region at the base of the flow, both quite challenging for the standard fireball model. These problems are resolved if the jet is initially highly magnetized and has a substantial Poynting flux.
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| 7. |
- Guiriec, Sylvain, et al.
(författare)
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Time-resolved Spectroscopy of the Three Brightest and Hardest Short Gamma-ray Bursts Observed with the Fermi Gamma-ray Burst Monitor
- 2010
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Ingår i: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 725:1, s. 225-241
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Tidskriftsartikel (refereegranskat)abstract
- From 2008 July to 2009 October, the Gamma-ray Burst Monitor (GBM) on board the Fermi Gamma-ray Space Telescope has detected 320 gamma-ray bursts (GRBs). About 20% of these events are classified as short based on their T90 duration below 2 s. We present here for the first time time-resolved spectroscopy at timescales as short as 2 ms for the three brightest short GRBs observed with GBM. The time-integrated spectra of the events deviate from the Band function, indicating the existence of an additional spectral component, which can be fit by a power law with index ∼-1.5. The time-integrated Epeak values exceed 2 MeV for two of the bursts and are well above the values observed in the brightest long GRBs. Their Epeak values and their low-energy power-law indices (a) confirm that short GRBs are harder than long ones. We find that short GRBs are very similar to long ones, but with light curves contracted in time and with harder spectra stretched toward higher energies. In our time-resolved spectroscopy analysis, we find that the Epeak values range from a few tens of keV up to more than 6MeV. In general, the hardness evolutions during the bursts follow their flux/intensity variations, similar to long bursts. However, we do not always see the Epeak leading the light-curve rises and confirm the zero/short average light-curve spectral lag below 1 MeV, already established for short GRBs. We also find that the time-resolved low-energy power-law indices of the Band function mostly violate the limits imposed by the synchrotron models for both slow and fast electron cooling and may require additional emission processes to explain the data. Finally, we interpreted these observations in the context of the current existing models and emission mechanisms for the prompt emission of GRBs.
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| 8. |
- Kilty, Caroline, et al.
(författare)
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Young onset dementia : implications for employment and finances
- 2023
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Ingår i: Dementia. - : Sage Publications. - 1471-3012 .- 1741-2684. ; 22:1, s. 68-84
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Tidskriftsartikel (refereegranskat)abstract
- Background: People with young onset dementia face unique challenges. Notably, at time of symptom presentation, many people affected by young onset dementia are still employed with significant financial obligations. The aim of this study was to explore the specific impact that young onset dementia has on continued employment and finances and to identify ways to optimise post-diagnostic approaches in this regard.Methods: Purposive sampling, with a maximum variation technique, was used to recruit a small but diverse range of people with young onset dementia in Ireland. In-depth semi-structured interviews were conducted, and data were analysed using Reflexive Thematic Analysis. In total, 22 interviews were conducted with 10 people with young onset dementia and 12 spouses and children. Two themes were constructed: impact of young onset dementia on (I) employment and (II) finances.Findings: Participants' lived accounts showed the devastating effect of a diagnosis of young onset dementia on working life, and the resultant financial, social, and psychological consequences. Participants reported having to leave paid employment early, reported losing contracts and retiring on medical grounds. There were financial implications caused by loss of income, and many additional expenses owing to dementia were incurred. In some families, spouses had to take up employment at the same time as a caring role to mitigate the loss of income, and young children were anxious at the resultant occupational and financial tensions.Conclusion: People diagnosed with young onset dementia encounter significant challenges associated with employment, and individual and family finances. There is a need for more specific information and guidance from healthcare professionals around employment rights, income support and welfare benefits and the pension status for this group of people. Additionally, healthcare professionals should be cognisant of the additional financial burden people face in young onset dementia when advising on services which incur out-of-pocket costs.
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| 9. |
- Paciesas, William S, et al.
(författare)
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The Fermi GBM Gamma-Ray Burst Catalog : The First Two Years
- 2012
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Ingår i: Astrophysical Journal Supplement Series. - : American Astronomical Society. - 0067-0049 .- 1538-4365. ; 199:1
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Tidskriftsartikel (refereegranskat)abstract
- The Fermi Gamma-ray Burst Monitor (GBM) is designed to enhance the scientific return from Fermi in studying gamma-ray bursts (GRBs). In its first two years of operation GBM triggered on 491 GRBs. We summarize the criteria used for triggering and quantify the general characteristics of the triggered GRBs, including their locations, durations, peak flux, and fluence. This catalog is an official product of the Fermi GBM science team, and the data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center.
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| 10. |
- von Kienlin, Andreas, et al.
(författare)
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The Second Fermi GBM Gamma-Ray Burst Catalog : The First Four Years
- 2014
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Ingår i: Astrophysical Journal Supplement Series. - : Institute of Physics Publishing (IOPP). - 0067-0049 .- 1538-4365. ; 211:1
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Tidskriftsartikel (refereegranskat)abstract
- This is the second of a series of catalogs of gamma-ray bursts (GRBs) observed with the Fermi Gamma-ray Burst Monitor (GBM). It extends the first two-year catalog by two more years, resulting in an overall list of 953 GBM triggered GRBs. The intention of the GBM GRB catalog is to provide information to the community on the most important observables of the GBM detected GRBs. For each GRB the location and main characteristics of the prompt emission, the duration, peak flux and fluence are derived. The latter two quantities are calculated for the 50-300 keV energy band, where the maximum energy release of GRBs in the instrument reference system is observed and also for a broader energy band from 10-1000 keV, exploiting the full energy range of GBMs low-energy detectors. Furthermore, information is given on the settings and modifications of the triggering criteria and exceptional operational conditions during years three and four in the mission. This second catalog is an official product of the Fermi GBM science team, and the data files containing the complete results are available from the High-Energy Astrophysics Science Archive Research Center.
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| 11. |
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- 2019
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Tidskriftsartikel (refereegranskat)
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