PATT-Linked Grant for Travel and Subsistence 2012-2014

Lead Research Organisation: Liverpool John Moores University
Department Name: Astrophysics Research Institute

Abstract

This is an application for a PATT-linked continuation grant to cover the travel and subsistence costs of observing runs carried out by staff at the Astrophysics Research Institute (ARI). The observing time is won in internationally competitive, peer-reviewed applications procedures. ARI staff carry out observational research programmes in a diverse range of astrophysics: star formation, the structure and content of galaxies and clusters of galaxies, active galactic nuclei, galaxy evolution, gamma-ray bursts, novae and supernovae. We currently have 22 active researchers, of whom 6 are regular users of STFC telescopes or other PATT-supported ground-based telescopes. We have followed current STFC guidlines and give full details of travel and subsistence for PATT observing runs over the last two years. Projected expenditure in the next two years will be dominated by two JCMT legacy surveys using SCUBA-2, one of which is LJMU-led, that have now begun and will run at least until September 2014.

Publications

10 25 50

publication icon
Bours M (2016) Long-term eclipse timing of white dwarf binaries: an observational hint of a magnetic mechanism at work in Monthly Notices of the Royal Astronomical Society

publication icon
Coppin K (2015) The SCUBA-2 Cosmology Legacy Survey: the submillimetre properties of Lyman-break galaxies at z = 3-5 in Monthly Notices of the Royal Astronomical Society

publication icon
Eden D (2017) The JCMT Plane Survey: first complete data release - emission maps and compact source catalogue in Monthly Notices of the Royal Astronomical Society

publication icon
Font J (2019) Spiral structure in barred galaxies. Observational constraints to spiral arm formation mechanisms in Monthly Notices of the Royal Astronomical Society

publication icon
Geach J (2017) The SCUBA-2 Cosmology Legacy Survey: 850 µm maps, catalogues and number counts in Monthly Notices of the Royal Astronomical Society

publication icon
Habergham S (2014) Environments of interacting transients: impostors and Type IIn supernovae in Monthly Notices of the Royal Astronomical Society

publication icon
James P (2015) Discovery of kpc-scale line emission in barred galaxies, not linked to AGN or star formation. in Monthly Notices of the Royal Astronomical Society

publication icon
James P (2016) Stellar population constraints on the ages of galactic bars in Monthly Notices of the Royal Astronomical Society

publication icon
Littlefair S (2014) A parameter study of the eclipsing CV in the Kepler field, KIS J192748.53+444724.5 in Monthly Notices of the Royal Astronomical Society

publication icon
Lyman J (2013) Environment-derived constraints on the progenitors of low-luminosity Type I supernovae? in Monthly Notices of the Royal Astronomical Society

publication icon
McAllister M (2015) PHL 1445: an eclipsing cataclysmic variable with a substellar donor near the period minimum in Monthly Notices of the Royal Astronomical Society

publication icon
Moore T (2015) The JCMT Plane Survey: early results from the l = 30° field in Monthly Notices of the Royal Astronomical Society

publication icon
Rigby A (2015) CHIMPS: the 13 CO/C 18 O ( J  = 3 ? 2) Heterodyne Inner Milky Way Plane Survey in Monthly Notices of the Royal Astronomical Society

publication icon
Wilkinson A (2017) The SCUBA-2 Cosmology Legacy Survey: the clustering of submillimetre galaxies in the UKIDSS UDS field in Monthly Notices of the Royal Astronomical Society

 
Description This grant provides departmental funds for travel to astronomical observing facilities. Resulting discoveries are various and are detailed in the associated research publications.
Exploitation Route Resulting research published research papers form part of the body of knowledge upon which further research is based.
Sectors Education,Other

 
Description Resulting research published research papers form part of the body of knowledge upon which further research is based.
Sector Other
Impact Types Cultural