24 research outputs found

    The TESS-Keck Survey. II. An Ultra-Short-Period Rocky Planet And Its Siblings Transiting The Galactic Thick-Disk Star TOI-561

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    We report the discovery of TOI-561, a multiplanet system in the galactic thick disk that contains a rocky, ultra-short-period planet. This bright (V = 10.2) star hosts three small transiting planets identified in photometry from the NASA TESS mission: TOI-561 b (TOI-561.02, P = 0.44 days, Rp = 1.45 ± 0.11 R⊕), c (TOI-561.01, P = 10.8 days, Rp = 2.90 ± 0.13 R⊕), and d (TOI-561.03, P = 16.3 days, Rp = 2.32 ± 0.16 R⊕). The star is chemically ([Fe/H] = −0.41 ± 0.05, [α/Fe] = +0.23 ± 0.05) and kinematically consistent with the galactic thick-disk population, making TOI-561 one of the oldest (10 ± 3 Gyr) and most metal-poor planetary systems discovered yet. We dynamically confirm planets b and c with radial velocities from the W. M. Keck Observatory High Resolution Echelle Spectrometer. Planet b has a mass and density of 3.2 ± 0.8 M⊕ and 5.5−1.6+2.0{5.5}_{-1.6}^{+2.0}g cm−3, consistent with a rocky composition. Its lower-than-average density is consistent with an iron-poor composition, although an Earth-like iron-to-silicates ratio is not ruled out. Planet c is 7.0 ± 2.3 M⊕ and 1.6 ± 0.6 g cm−3, consistent with an interior rocky core overlaid with a low-mass volatile envelope. Several attributes of the photometry for planet d (which we did not detect dynamically) complicate the analysis, but we vet the planet with high-contrast imaging, ground-based photometric follow-up, and radial velocities. TOI-561 b is the first rocky world around a galactic thick-disk star confirmed with radial velocities and one of the best rocky planets for thermal emission studies

    The TESS-Keck survey. II. An ultra-short-period rocky planet and its siblings transiting the galactic thick-disk star TOI-561

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    We report the discovery of TOI-561, a multiplanet system in the galactic thick disk that contains a rocky, ultrashort- period planet. This bright (V = 10.2) star hosts three small transiting planets identified in photometry from the NASA TESS mission: TOI-561 b (TOI-561.02, P = 0.44 days, Rp = 1.45 ± 0.11 R⊕), c (TOI-561.01, P = 10.8 days, Rp = 2.90 ± 0.13 R⊕), and d (TOI-561.03, P = 16.3 days, Rp = 2.32 ± 0.16 R⊕). The star is chemically ([Fe/ H] = -0.41 ± 0.05, [a/Fe]=+0.23 ± 0.05) and kinematically consistent with the galactic thick-disk population, making TOI-561 one of the oldest (10 ± 3 Gyr) and most metal-poor planetary systems discovered yet. We dynamically confirm planets b and c with radial velocities from the W. M. Keck Observatory High Resolution Echelle Spectrometer. Planet b has a mass and density of 3.2 ± 0.8M⊕ and 5.5+2.0-1.6g cm-3, consistent with a rocky composition. Its lower-than-average density is consistent with an iron-poor composition, although an Earth-like iron-to-silicates ratio is not ruled out. Planet c is 7.0 ± 2.3M⊕ and 1.6 ± 0.6 g cm-3, consistent with an interior rocky core overlaid with a low-mass volatile envelope. Several attributes of the photometry for planet d (which we did not detect dynamically) complicate the analysis, but we vet the planet with high-contrast imaging, groundbased photometric follow-up, and radial velocities. TOI-561 b is the first rocky world around a galactic thick-disk star confirmed with radial velocities and one of the best rocky planets for thermal emission studies

    Reactions to Mindfulness Intervention in an Early Psychosis Program

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    Objective: The Mindfulness Ambassador Program (MAP) is a standardized facilitated group mindfulness-based intervention designed for youth that intersects core foundations of mindfulness with social emotional learning. The curriculum introduces participants to mindfulness practices and related activities in order to achieve the following: increased self-awareness; emotional regulation; responsive listening; communication skills; social awareness; and perspective taking. These pillars of the MAP curriculum align with psychosocial rehabilitation outcomes among those experiencing early psychosis. The objective of this study was to understand the client experience and assess the acceptability of MAP within the clinical setting of an early psychosis intervention program. Research Design and Methods: Two semi-structured focus groups explored experiences of clients (n=9) of an early psychosis intervention program who participated in a pilot trial of MAP in a clinical setting. Focus group discussions were analyzed using a thematic analysis framework. Results: Five overarching themes emerged with nuanced subthemes: (i) program engagement (overall impressions, participant involvement); (ii) learning (core mindfulness skills, personal learning and growth); (iii) direct benefits to participants’ well-being; (iv) aspects of the program (facilitation, group structure, group dynamic); and (v) challenges and opportunities for improvement. Conclusions: All participants reported benefits from and/or challenges with participating in MAP. Evaluative comments about MAP content, facilitation, and structure were expressed. This research supports MAP as a promising intervention for young people recovering from early psychosis

    Understanding the role of the family physician in early psychosis intervention

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    Background The family physician is key to facilitating access to psychiatric treatment for young people with first-episode psychosis, and this involvement can reduce aversive events in pathways to care. Those who seek help from primary care tend to have longer intervals to psychiatric care, and some people receive ongoing psychiatric treatment from the family physician. Aims Our objective is to understand the role of the family physician in help-seeking, recognition and ongoing management of first-episode psychosis. Method We will use a mixed-methods approach, incorporating health administrative data, electronic medical records (EMRs) and qualitative methodologies to study the role of the family physician at three points on the pathway to care. First, help-seeking: we will use health administrative data to examine access to a family physician and patterns of primary care use preceding the first diagnosis of psychosis; second, recognition: we will identify first-onset cases of psychosis in health administrative data, and look back at linked EMRs from primary care to define a risk profile for undetected cases; and third, management: we will examine service provision to identified patients through EMR data, including patterns of contacts, prescriptions and referrals to specialised care. We will then conduct qualitative interviews and focus groups with key stakeholders to better understand the trends observed in the quantitative data. Discussion These findings will provide an in-depth description of first-episode psychosis in primary care, informing strategies to build linkages between family physicians and psychiatric services to improve transitions of care during the crucial early stages of psychosis

    Developing efficient upconverter silicon solar cell devices

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    Advanced systems for harvesting sub-bandgap photons via upconversion were investigated, comprising improved upconverter materials, adapted silicon solar cells, nanocrystalline quantum dots and spectrally selective photonic crystals. Upconversion increased JSC by 13.3±3.0 mA/cm2 at 207±86 suns
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