4 results
Peer mentoring in psychiatry: a trainee-led initiative
- Zoe Moore, Linda Irwin, Stuart Brown, Julie Anderson, Stephen Moore
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- Journal:
- BJPsych Open / Volume 7 / Issue S1 / June 2021
- Published online by Cambridge University Press:
- 18 June 2021, p. S149
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- Article
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Aims
Our aim was to establish a Peer Mentoring Network within Psychiatry Training in Northern Ireland.
Recognising that starting a new job can be a stressful time in any junior doctor's career, we wanted to ensure that new Core Trainees (CT1s) joining our Specialty Programme were well supported through this transition.
Although Clinical and Educational Supervision is well established in providing a support structure for trainees, we believed that a peer mentoring relationship, (with allocation of a Higher Psychiatry Trainee as mentor), would be of additional benefit.
It was hoped that the scheme would prove mutually beneficial to both mentee and mentor.
MethodWe delivered a presentation at CT1 induction and sent out follow-up emails to encourage participation. Higher trainees were also sent information via email and asked to complete a basic application form if interested in becoming a mentor. Prospective mentors then attended a one-day training session.
Two lead mentors, (also higher trainees), were allocated to oversee the scheme, with additional supervision from two lead Consultants. Mentor-Mentee matches were made based on information such as location, sub-specialty affiliations and outside interests.
Matched pairs were advised about the intended frequency and nature of contacts. Check-in emails were sent halfway through the year and feedback evaluations completed at the end.
Result95% of trainees who completed the evaluations said they would recommend the scheme to colleagues.
Mentees reported benefits in terms of personal and professional development, whilst mentors reported improved listening, coaching, and supervisory skills.
A small number of trainees highlighted that 6 monthly rotations impacted on ability to maintain face to face contacts.
Recruitment and engagement have improved annually. We are currently running the third year of the scheme and have achieved 100% uptake amongst CT1s and are over-subscribed with mentors, (19 mentors to 13 mentees).
ConclusionThe majority of feedback received has been positive and interest in the scheme continues to grow.
Potential issues relating to location of postings has been overcome, at least in part, by recent changes to ways of working and the use of alternative forms of contact, such as video calling.
Having exceeded demand in terms of mentor recruitment, we hope to extend the scheme to include trainees of other grades, and particularly those who are new to Northern Ireland.
We are excited to see where the next stage of our journey takes us and hope that others will be inspired to embark on similar schemes within their areas of work.
The science of EChO
- Giovanna Tinetti, James Y-K. Cho, Caitlin A. Griffith, Olivier Grasset, Lee Grenfell, Tristan Guillot, Tommi T. Koskinen, Julianne I. Moses, David Pinfield, Jonathan Tennyson, Marcell Tessenyi, Robin Wordsworth, Alan Aylward, Roy van Boekel, Angioletta Coradini, Therese Encrenaz, Ignas Snellen, Maria R. Zapatero-Osorio, Jeroen Bouwman, Vincent Coudé du Foresto, Mercedes Lopez-Morales, Ingo Mueller-Wodarg, Enric Pallé, Franck Selsis, Alessandro Sozzetti, Jean-Philippe Beaulieu, Thomas Henning, Michael Meyer, Giuseppina Micela, Ignasi Ribas, Daphne Stam, Mark Swain, Oliver Krause, Marc Ollivier, Emanuele Pace, Bruce Swinyard, Peter A.R. Ade, Nick Achilleos, Alberto Adriani, Craig B. Agnor, Cristina Afonso, Carlos Allende Prieto, Gaspar Bakos, Robert J. Barber, Michael Barlow, Peter Bernath, Bruno Bézard, Pascal Bordé, Linda R. Brown, Arnaud Cassan, Céline Cavarroc, Angela Ciaravella, Charles Cockell, Athéna Coustenis, Camilla Danielski, Leen Decin, Remco De Kok, Olivier Demangeon, Pieter Deroo, Peter Doel, Pierre Drossart, Leigh N. Fletcher, Matteo Focardi, Francois Forget, Steve Fossey, Pascal Fouqué, James Frith, Marina Galand, Patrick Gaulme, Jonay I. González Hernández, Davide Grassi, Matt J. Griffin, Ulrich Grözinger, Manuel Guedel, Pactrick Guio, Olivier Hainaut, Robert Hargreaves, Peter H. Hauschildt, Kevin Heng, David Heyrovsky, Ricardo Hueso, Pat Irwin, Lisa Kaltenegger, Patrick Kervella, David Kipping, Geza Kovacs, Antonino La Barbera, Helmut Lammer, Emmanuel Lellouch, Giuseppe Leto, Mercedes Lopez Morales, Miguel A. Lopez Valverde, Manuel Lopez-Puertas, Christophe Lovi, Antonio Maggio, Jean-Pierre Maillard, Jesus Maldonado Prado, Jean-Baptiste Marquette, Francisco J. Martin-Torres, Pierre Maxted, Steve Miller, Sergio Molinari, David Montes, Amaya Moro-Martin, Olivier Mousis, Napoléon Nguyen Tuong, Richard Nelson, Glenn S. Orton, Eric Pantin, Enzo Pascale, Stefano Pezzuto, Ennio Poretti, Raman Prinja, Loredana Prisinzano, Jean-Michel Réess, Ansgar Reiners, Benjamin Samuel, Jorge Sanz Forcada, Dimitar Sasselov, Giorgio Savini, Bruno Sicardy, Alan Smith, Lars Stixrude, Giovanni Strazzulla, Gautam Vasisht, Sandrine Vinatier, Serena Viti, Ingo Waldmann, Glenn J. White, Thomas Widemann, Roger Yelle, Yuk Yung, Sergey Yurchenko
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- Journal:
- Proceedings of the International Astronomical Union / Volume 6 / Issue S276 / October 2010
- Published online by Cambridge University Press:
- 10 November 2011, pp. 359-370
- Print publication:
- October 2010
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The science of extra-solar planets is one of the most rapidly changing areas of astrophysics and since 1995 the number of planets known has increased by almost two orders of magnitude. A combination of ground-based surveys and dedicated space missions has resulted in 560-plus planets being detected, and over 1200 that await confirmation. NASA's Kepler mission has opened up the possibility of discovering Earth-like planets in the habitable zone around some of the 100,000 stars it is surveying during its 3 to 4-year lifetime. The new ESA's Gaia mission is expected to discover thousands of new planets around stars within 200 parsecs of the Sun. The key challenge now is moving on from discovery, important though that remains, to characterisation: what are these planets actually like, and why are they as they are?
In the past ten years, we have learned how to obtain the first spectra of exoplanets using transit transmission and emission spectroscopy. With the high stability of Spitzer, Hubble, and large ground-based telescopes the spectra of bright close-in massive planets can be obtained and species like water vapour, methane, carbon monoxide and dioxide have been detected. With transit science came the first tangible remote sensing of these planetary bodies and so one can start to extrapolate from what has been learnt from Solar System probes to what one might plan to learn about their faraway siblings. As we learn more about the atmospheres, surfaces and near-surfaces of these remote bodies, we will begin to build up a clearer picture of their construction, history and suitability for life.
The Exoplanet Characterisation Observatory, EChO, will be the first dedicated mission to investigate the physics and chemistry of Exoplanetary Atmospheres. By characterising spectroscopically more bodies in different environments we will take detailed planetology out of the Solar System and into the Galaxy as a whole.
EChO has now been selected by the European Space Agency to be assessed as one of four M3 mission candidates.
Contributors
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- By Robert S. Agnew, Lara M. Belliston, Daniel M. Blonigen, Michel Boivin, Jeanne Brooks‐Gunn, Andrew Canastar, Noel A. Card, Emil F. Coccaro, Nicki R. Crick, Linda L. Dahlberg, Garth Davies, Scott H. Decker, Kenneth A. Dodge, Dorothy L. Espelage, Jeffrey Fagan, Albert D. Farrell, David P. Farrington, Daniel J. Flannery, Mark S. Fleisher, Vangie A. Foshee, Holly Foster, Richard J. Gelles, Denise C. Gottfredson, Gary D. Gottfredson, Michael R. Gottfredson, Richard E. Heyman, James C. (Buddy) Howell, Megan Q. Howell, Li Huang, L. Rowell Huesmann, Cynthia Irvin, Gary F. Jensen, Yoshito Kawabata, Lucyna Kirwil, Jeff M. Kretschmar, Robert F. Krueger, Markus J. P. Kruesi, Benjamin B. Lahey, Royce Lee, Scott O. Lilienfeld, Todd D. Little, Anne Martin, Rebecca A. Matthew, Stephen C. Maxson, Jacquelyn Mize, Terrie E. Moffitt, Daniel S. Nagin, Jamie M. Ostrov, Christopher J. Patrick, Bowen Paulle, Gregory S. Pettit, Adrian Raine, Soo Hyun Rhee, Angela Scarpa, Jean R. Séguin, Michelle R. Sherrill, Mark I. Singer, Amy M. Smith Slep, Kevin J. Strom, Patrick Sylvers, Patrick H. Tolan, Elizabeth Trejos‐Castillo, Richard E. Tremblay, Manfred van Dulmen, Johan van Wilsem, Alexander T. Vazsonyi, Edelyn Verona, Frank Vitaro, Monique Vulin‐Reynolds, Irwin D. Waldman, Mark Warr, Stanley Wasserman, Deanna L. Wilkinson
- Edited by Daniel J. Flannery, Kent State University, Ohio, Alexander T. Vazsonyi, Auburn University, Alabama, Irwin D. Waldman, Emory University, Atlanta
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- Book:
- The Cambridge Handbook of Violent Behavior and Aggression
- Published online:
- 05 June 2012
- Print publication:
- 03 September 2007, pp xi-xviii
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Modeling and characterization of the amino propeptide of collagenα1(XI), a regulatory domain in collagen fibrillar architecture.
- Lisa R. Warner, Arzhang Fallahi, Becky Kroll, Katey M. Irwin, Sorcha Yingst, Linda M. Mercer, Susan E. Shadle, Julia Thom Oxford
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- Journal:
- MRS Online Proceedings Library Archive / Volume 874 / 2005
- Published online by Cambridge University Press:
- 01 February 2011, L4.9
- Print publication:
- 2005
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Connective tissues such as cartilage, tendon, skin, bone, and arteries are composite bio-materials that contain predominantly water, collagen, proteoglycans and hyaluronic acid. Like any composite material, the components themselves and their interactions dictate the properties of the material. Fibrillar collagens are the principal structural molecules of the connective tissues and require regulated assembly and growth. Previous work from our lab indicates that the amino propeptide (Npp) domain of collagen type XI α1 chain regulates fibril diameter growth. Npp is a globular domain that is thought to sterically hinder the dense packing assembly of collagen molecules in fibrils. This mechanism of regulating collagen fibril assembly may be more complex than steric hindrance. We hypothesize that the Npp domain has a more dynamic role in establishing the structure/function relationship of collagen fibrils in connective tissues. In this study, the molecular structure of Npp was predicted by modeling. The model predicted putative binding sites for heparan sulfate and divalent cations. These predicted binding sites were evaluated empirically by fluorescence spectroscopy and surface plasmon resonance.