‘Blocked at every level’: criminal justice system professionals’ experiences of including people with intellectual disabilities within a targeted magistrates’ court

This is an accepted manuscript of an article published by Emerald in Journal of Intellectual Disabilities and Offending Behaviour on 28/03/2020, available online: https://doi.org/10.1108/JIDOB-07-2019-0014 The accepted version of the publication may differ from the final published version.Purpose: Mental health courts (MHCs) may enable better support for people with intellectual disabilities (ID) within the criminal justice system (CJS) but little evaluative empirical evidence is available regarding their operation. This study explores professional perceptions of the challenges of including people with ID in a Targeted Services Court (TSC) designed for people with mental health issues and ID. Methodology: Information was gathered, via interviews and focus groups, from 46 professionals working with people with mental health issues and ID within the TSC. Data were analysed using thematic network analysis. Findings: Findings highlight the neglect and lack of inclusion of people with ID within the TSC processes, with challenges in identifying people with ID, stakeholder awareness, inconsistent adapting of practices for people with ID and information transfer underpinned by the involvement of numerous organisations with differing agendas. Implications: Although valued, development of a TSC including people with ID was a challenging endeavour and may reflect societal and institutional neglect of people with ID, recommendations are provided. Originality: This study adds to the few investigations have considered the process of including people with ID in a TSC from the perspective of those working in the criminal justice system

Police officers’ perceptions of their role in a mental health Magistrates’ court pathway

Although common in the USA, Mental Health Courts are relatively new to the UK and their effectiveness here is not yet fully understood. Referral to these courts is largely reliant upon early identification of mental health problems, a task commonly undertaken by police in the custody suite. Little is known about police perceptions of their role in working with offenders with mental health system in the UK. This exploratory study therefore investigates police views of a pilot Mental Health Courts and their role within the pathway to these. Semi-structured interviews were conducted with six members of a large police force involved in a pilot Mental Health Court. Data-led thematic analysis was used to identify the recurrent themes emerging. Three main themes were identified: ‘Benefits of a Mental Health Court’, ‘Police as Gatekeepers’ and ‘Barriers to Identification’. The introduction of Mental Health Courts in the UK was viewed as being reflective of changes in approaches to criminal justice. Whilst feeling responsibility for referrals to the Mental Health Court, time, training and multiagency working were seen as hindering this. The findings suggest the success of Mental Health Courts is dependent upon ‘getting it right’ from the start of the pathway; recommendations are provided

Internet Access by People with Intellectual Disabilities: Inequalities and Opportunities

This review gives an overview of the societal inequalities faced by people with intellectual disabilities, before focusing specifically on challenges people face accessing the Internet. Current access will be outlined along with the societal, support and attitudinal factors that can hinder access. Discussion of carer views of Internet use by people with intellectual disabilities will be covered incorporating consideration of the tension between protection, self-determination and lifestyle issues and gaining Internet access. We will address how impairment related factors may impede access and subsequently discuss how supports may be used to obfuscate impairments and facilitate access. We will move on from this to critically describe some of the potential benefits the Internet could provide to people with intellectual disabilities, including the potential for self-expression, advocacy and developing friendships. Finally, strategies to better include people with intellectual disabilities online will be given along with future research suggestions

Gender differences in videoed accounts of victim blaming for revenge porn for self-taken and stealth-taken sexually explicit images and videos

© 2021 The Authors. Published by Masaryk University, Faculty of Social Studies. This is an open access article available under a Creative Commons licence. The published version can be accessed at the following link on the publisher’s website: https://doi.org/10.5817/CP2021-4-3Using video recounts from revenge porn victims, this study explores whether levels of victim blaming differs for the sharing of self- and stealth-taken sexually explicit images and videos. Building on previous work which has demonstrated victim blame for both self- and stealth generated images in occurrences of revenge porn (Zvi & Schechory-Bitton, 2020), the reported study presents an original and ecologically valid methodological approach whereby 342 (76 male, 266 female) participants (Mage = 39.27, SD = 11.70) from the UK watched videoed accounts of real experiences of falling victim to revenge porn, rather than using text based, often fictional, vignettes to attribute blame which dominate studies in this area. All data was collected in 2019. The results demonstrated that significantly more blame was assigned to victims when participants were indirectly rather than directly asked who was to blame for the occurrence of revenge porn, supporting the notion of an unconscious processing bias in attributing blame. More blame was also assigned to those victims who themselves generated the material compared to when it had been acquired without their awareness by a perpetrator, suggesting the cognitive bias to be in line with a just world hypothesis. Male participants were more likely to blame a victim than were female participants, although sex of victim and mode of shared sexually-explicit material (video or image) did not appear to affect levels of victim-blame. Findings are considered in terms of extant research and the need for future work in the area of victim blame and revenge pornography.Published onlin

If the Mask Fits: Psychological Correlates with Online Self-Presentation Experimentation in Adults

Online self-presentation refers to the ways in which individuals share aspects of the self to portray a particular image. Being online presents opportunities for individuals to experiment with different versions of the self as part of identity development but also to manage how others perceive them. Research has shown that personality can influence online self-presentation behaviors, but these studies have mainly focused on internal characteristics, and more research is needed exploring the relational facets of personality. This study aims to investigate the extent to which an individual's self-concept clarity, self-monitoring tendency, self-esteem, and social anxiety predict different presentations of the online self. A cross-sectional online survey was conducted with 405 adult participants from Australia, the United Kingdom, and the United States. Results show that individuals with higher self-concept clarity and self-monitoring are more likely to present a single consistent online and offline self. Younger adults and those with greater social anxiety are more likely to present idealized self-images online, and participants with higher social anxiety and lower self-esteem are more likely to prefer online, rather than offline, communication. Findings are broadly consistent with the literature, and suggest the need for more systematic investigation into a variety of personality variables that take into account the relational nature of identity formation and impression management. This research emphasizes the multifaceted nature of online self-presentation behaviors, and the ways in which they are differentially influenced by personality variables

Perceptions of unwanted sexual behaviour on public transport

This study focuses on bystander perceptions and expected responses to unwanted sexual behaviours on public transport. Level of blame, incident seriousness, likelihood of reporting and intervening were evaluated using a series of 6 vignettes that manipulated passenger density and severity of the behaviour. Half of the participants also viewed a video to raise their awareness of unwanted sexual behaviours. The results indicated that blame was attributed to the perpetrator and not the victim, with perpetrator blame, incident seriousness, and likelihood of reporting all being influenced by a passenger density and behaviour severity interaction. Increasing awareness of unwanted sexual behaviours had no effect with the exception of likelihood of intervention. Findings are discussed in relation to women’s safety during peak and off peak travel and the role of the bystander here. The implications of this for women’s safety are considered

The wide-field, multiplexed, spectroscopic facility WEAVE : survey design, overview, and simulated implementation

Funding for the WEAVE facility has been provided by UKRI STFC, the University of Oxford, NOVA, NWO, Instituto de Astrofísica de Canarias (IAC), the Isaac Newton Group partners (STFC, NWO, and Spain, led by the IAC), INAF, CNRS-INSU, the Observatoire de Paris, Région Île-de-France, CONCYT through INAOE, Konkoly Observatory (CSFK), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Lund University, the Leibniz Institute for Astrophysics Potsdam (AIP), the Swedish Research Council, the European Commission, and the University of Pennsylvania.WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366-959 nm at R ∼ 5000, or two shorter ranges at R ∼ 20,000. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for ∼ 3 million stars and detailed abundances for ∼ 1.5 million brighter field and open-cluster stars; (ii) survey ∼ 0.4 million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey  ∼ 400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in z 1 million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at z > 2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.PostprintPeer reviewe

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366$-$959\,nm at $R\sim5000$, or two shorter ranges at $R\sim20\,000$. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for $\sim$3 million stars and detailed abundances for $\sim1.5$ million brighter field and open-cluster stars; (ii) survey $\sim0.4$ million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey $\sim400$ neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in $z<0.5$ cluster galaxies; (vi) survey stellar populations and kinematics in $\sim25\,000$ field galaxies at $0.3\lesssim z \lesssim 0.7$; (vii) study the cosmic evolution of accretion and star formation using $>1$ million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at $z>2$. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator.Comment: 41 pages, 27 figures, accepted for publication by MNRA

The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation

WEAVE, the new wide-field, massively multiplexed spectroscopic survey facility for the William Herschel Telescope, will see first light in late 2022. WEAVE comprises a new 2-degree field-of-view prime-focus corrector system, a nearly 1000-multiplex fibre positioner, 20 individually deployable 'mini' integral field units (IFUs), and a single large IFU. These fibre systems feed a dual-beam spectrograph covering the wavelength range 366−959\,nm at R∼5000, or two shorter ranges at R∼20000. After summarising the design and implementation of WEAVE and its data systems, we present the organisation, science drivers and design of a five- to seven-year programme of eight individual surveys to: (i) study our Galaxy's origins by completing Gaia's phase-space information, providing metallicities to its limiting magnitude for ∼3 million stars and detailed abundances for ∼1.5 million brighter field and open-cluster stars; (ii) survey ∼0.4 million Galactic-plane OBA stars, young stellar objects and nearby gas to understand the evolution of young stars and their environments; (iii) perform an extensive spectral survey of white dwarfs; (iv) survey ∼400 neutral-hydrogen-selected galaxies with the IFUs; (v) study properties and kinematics of stellar populations and ionised gas in z1 million spectra of LOFAR-selected radio sources; (viii) trace structures using intergalactic/circumgalactic gas at z>2. Finally, we describe the WEAVE Operational Rehearsals using the WEAVE Simulator