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The Taipan Galaxy Survey: Scientific Goals and Observing Strategy
- Elisabete da Cunha, Andrew M. Hopkins, Matthew Colless, Edward N. Taylor, Chris Blake, Cullan Howlett, Christina Magoulas, John R. Lucey, Claudia Lagos, Kyler Kuehn, Yjan Gordon, Dilyar Barat, Fuyan Bian, Christian Wolf, Michael J. Cowley, Marc White, Ixandra Achitouv, Maciej Bilicki, Joss Bland-Hawthorn, Krzysztof Bolejko, Michael J. I. Brown, Rebecca Brown, Julia Bryant, Scott Croom, Tamara M. Davis, Simon P. Driver, Miroslav D. Filipovic, Samuel R. Hinton, Melanie Johnston-Hollitt, D. Heath Jones, Bärbel Koribalski, Dane Kleiner, Jon Lawrence, Nuria Lorente, Jeremy Mould, Matt S. Owers, Kevin Pimbblet, C. G. Tinney, Nicholas F. H. Tothill, Fred Watson
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- Journal:
- Publications of the Astronomical Society of Australia / Volume 34 / 2017
- Published online by Cambridge University Press:
- 24 October 2017, e047
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The Taipan galaxy survey (hereafter simply ‘Taipan’) is a multi-object spectroscopic survey starting in 2017 that will cover 2π steradians over the southern sky (δ ≲ 10°, |b| ≳ 10°), and obtain optical spectra for about two million galaxies out to z < 0.4. Taipan will use the newly refurbished 1.2-m UK Schmidt Telescope at Siding Spring Observatory with the new TAIPAN instrument, which includes an innovative ‘Starbugs’ positioning system capable of rapidly and simultaneously deploying up to 150 spectroscopic fibres (and up to 300 with a proposed upgrade) over the 6° diameter focal plane, and a purpose-built spectrograph operating in the range from 370 to 870 nm with resolving power R ≳ 2000. The main scientific goals of Taipan are (i) to measure the distance scale of the Universe (primarily governed by the local expansion rate, H0) to 1% precision, and the growth rate of structure to 5%; (ii) to make the most extensive map yet constructed of the total mass distribution and motions in the local Universe, using peculiar velocities based on improved Fundamental Plane distances, which will enable sensitive tests of gravitational physics; and (iii) to deliver a legacy sample of low-redshift galaxies as a unique laboratory for studying galaxy evolution as a function of dark matter halo and stellar mass and environment. The final survey, which will be completed within 5 yrs, will consist of a complete magnitude-limited sample (i ⩽ 17) of about 1.2 × 106 galaxies supplemented by an extension to higher redshifts and fainter magnitudes (i ⩽ 18.1) of a luminous red galaxy sample of about 0.8 × 106 galaxies. Observations and data processing will be carried out remotely and in a fully automated way, using a purpose-built automated ‘virtual observer’ software and an automated data reduction pipeline. The Taipan survey is deliberately designed to maximise its legacy value by complementing and enhancing current and planned surveys of the southern sky at wavelengths from the optical to the radio; it will become the primary redshift and optical spectroscopic reference catalogue for the local extragalactic Universe in the southern sky for the coming decade.
Concepts of mental illness and medical pluralism in Harare
- V. Patel, T. Musara, T. Butau, P. Maramba, S. Fuyane
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- Journal:
- Psychological Medicine / Volume 25 / Issue 3 / May 1995
- Published online by Cambridge University Press:
- 09 July 2009, pp. 485-493
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The Focus Group Discussions (FGD) described in this paper are the first step of a study aiming to develop an ‘emic’ case-finding instrument. In keeping with the realities of primary care in Zimbabwe, nine FGD were held with 76 care providers including 30 village community workers, 22 traditional and faith healers (collectively referred to as traditional healers in this paper), 15 relatives of patients and 9 community psychiatric nurses. In addition to the general facets of concepts of mental illness, three ‘etic’ case vignettes were also presented.
A change in behaviour or ability to care for oneself emerged as the central definition of mental illness. Both the head and the heart were regarded as playing an important role in the mediation of emotions. The types of mental illness described were intimately related to beliefs about spiritual causation. Angered ancestral spirits, evil spirits and witchcraft were seen as potent causes of mental illness. Families not only bore the burden of caring for the patient and all financial expenses involved, but were also ostracized and isolated. Both biomedical and traditional healers could help mentally ill persons by resolving different issues relating to the same illness episode. All case vignettes were recognized by the care providers in their communities though many felt that the descriptions did not reflect ‘illnesses’ but social problems and that accordingly, the treatment for these was social, rather than medical.
The data enabled us to develop screening criteria for mental illness to be used by traditional healers and primary care nurses in the next stage of the study in which patients selected by these care providers on the grounds of suspicion of suffering from mental illness will be interviewed to elicit their explanatory models of illness and phenomenology.