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  • Tan, B.K.; Leech, J.; Rigopoulou, D.; Warren, B.E.; Wilson, C.D.; Attewell, D.; Azimlu, M.; Bendo, G. J.; Butner, H. M.; Brinks, E.; Chanial, P.; Clements, D. L.; Heesen, V.; Israel, F.; Knapen, J.H.; Matthews, H.E.; Mortier, A.M.J.; Muhle, S.; Sánchez-Gallego, J.R.; Tilanus, R.P.J.; Usero, A.; van der Werf, P.; Zhu, M. (2013-11-21)
  • Plume, R.; Fuller, G.A.; Helmich, F.; van der Tak, F.F.S.; Roberts, H.; Bowey, J.; Buckle, J.; Butner, H.; Caux, E.; Ceccarelli, C.; van Dishoeck, E.F.; Friberg, P.; Gibb, A.G.; Hatchell, J.; Hogerheijde, M.R.; Matthews, H.; Millar, T.J.; Mitchell, G.; Moore, T.J.T.; Ossenkopf, V.; Rawlings, J.M.C.; Richer, J.; Roellig, M.; Schilke, P.; Spaans, M.; Tielens, A.G.G.M.; Thompson, M.A.; Viti, S.; Weferling, B.; White, G.J.; Wouterloot, J.; Yates, J.A.; Zhu, M. (2007)
    Stars form in the densest, coldest, most quiescent regions of molecular clouds. Molecules provide the only probes that can reveal the dynamics, physics, chemistry, and evolution of these regions, but our understanding of ...
  • Bancarzewski, Maciej Albert (2016-04-15)
    This research contributes to an understanding of Japanese Foreign Investment (JFDI) in Poland, by using a Variety of Capitalism approach and drawing on literature from employment relations. It examines firstly, the extent ...
  • Stotz, Henrik; Jikumaru, Y.; Shimada, Y.; Sasaki, E.; Stingl, N.; Mueller, M. J.; Kamiya, Y. (2011)
    The jasmonate receptor COI1 is known to facilitate plant defense responses against necrotrophic pathogens, including the ascomycete Sclerotinia sclerotiorum. However, it is not known to what extent jasmonates contribute ...
  • Goulding, N. T.; Barnes, J. R.; Pinfield, D.J.; Kovacs, G.; Birkby, J.; Hodgkin, S.; Catalan, S.; Sipocz, B.; Jones, H.R.A.; del Burgo, C.; Jeffers, S.V.; Nefs, S.; Galvez-Ortiz, M. -C.; Martin, E. L. (2012-12)
    We present an analysis of the photometric variability of M dwarfs in the Wide Field Camera (WFCAM) Transit Survey. Although periodic light-curve variability in low mass stars is generally dominated by photospheric star ...
  • Rumble, D.; Hatchell, J.; Gutermuth, R. A.; Kirk, H.; Buckle, J.; Beaulieu, S. F.; Berry, D.S.; Broekhoven-Fiene, H.; Currie, M. J.; Fich, M.; Jenness, T.; Johnstone, D.; Mottram, J. C.; Nutter, D.; Pattle, K.; Pineda, J. E.; Quinn, C.; Salji, C.; Tisi, S.; Walker-Smith, S.; Di Francesco, J.; Hogerheijde, M.R.; Ward-Thompson, D.; Allen, L.E.; Cieza, L. A.; Dunham, M. M.; Harvey, P. M.; Stapelfeldt, K. R.; Bastien, P.; Butner, H.; Chen, M.; Chrysostomou, A.; Coude, S.; Davis, C.J.; Drabek-Maunder, E.; Duarte-Cabral, A.; Fiege, J.; Friberg, P.; Friesen, R.; Fuller, G.A.; Graves, S.; Greaves, J.; Gregson, J.; Holland, W.; Joncas, G.; Kirk, J.M.; Knee, L. B. G.; Mairs, S.; Marsh, K.; Matthews, B. C.; Moriarty-Schieven, G.; Rawlings, J.; Richer, J.; Robertson, D.; Rosolowsky, E.; Sadavoy, S.; Thomas, H.; Tothill, N.; Viti, S.; White, G.J.; Wilson, C. D.; Wouterloot, J.; Yates, J.; Zhu, M. (2015-04-01)
    We present SCUBA-2 450 and 850 μm observations of the Serpens MWC 297 region, part of the James Clerk Maxwell Telescope (JCMT) Gould Belt Survey of nearby star-forming regions. Simulations suggest that radiative feedback ...
  • Buckle, J.; Curtis, E.I.; Roberts, J.F.; White, G.J.; Hatchell, J.; Brunt, C.; Butner, H.; Cavanagh, B.; Chrysostomou, A.; Davis, C.J.; Duarte-Cabral, A.; Etxaluze, M.; Di Francesco, J.; Friberg, P.; Friesen, R.; Fuller, G.A.; Graves, S.; Greaves, J.S.; Hogerheijde, M.R.; Johnstone, D.; Matthews, B.; Matthews, H.; Nutter, D.; Rawlings, J.M.C.; Richer, J.; Sadavoy, S.; Simpson, R.J.; Tothill, N.F.H.; Tsamis, Y.G.; Viti, S.; Ward-Thompson, D.; Wouterloot, J.; Yates, J.A. (2010)
    The Gould Belt Legacy Survey will survey nearby star-forming regions (within 500 pc), using Heterodyne Array Receiver Programme (HARP), Submillimetre Common-User Bolometer Array 2 and Polarimeter 2 on the James Clerk Maxwell ...
  • Graves, S. F.; Richer, J. S.; Buckle, J. V.; Duarte-Cabral, A.; Fuller, G. A.; Hogerheijde, M. R.; Owen, J. E.; Brunt, C.; Butner, H. M.; Cavanagh, B.; Chrysostomou, A.; Curtis, E. I.; Davis, C. J.; Etxaluze, M.; Di Francesco, J.; Friberg, P.; Friesen, R. K.; Greaves, J. S.; Hatchell, J.; Johnstone, D.; Matthews, B.; Matthews, H.; Matzner, C. D.; Nutter, D.; Rawlings, J. M. C.; Roberts, J. F.; Sadavoy, S.; Simpson, R. J.; Tothill, N. F. H.; Tsamis, Y. G.; Viti, S.; Ward-Thompson, D.; White, G. J.; Wouterloot, J. G. A.; Yates, J. (2010-12-21)
    The Gould Belt Legacy Survey on the James Clerk Maxwell Telescope's has observed a region of 260 arcmin2 in 12CO J = 3 -> 2 emission, and a 190 arcmin2 subset of this in 13CO and C18O towards the Serpens molecular cloud. ...
  • Davis, C.J.; Chrysostomou, A.; Hatchell, J.; Wouterloot, J. G. A.; Buckle, J. V.; Nutter, D.; Fich, M.; Brunt, C.; Butner, H.; Cavanagh, B.; Curtis, E.I.; Duarte-Cabral, A.; Di Francesco, J.; Etxaluze, M.; Friberg, P.; Johnstone, D.; Matthews, B.; Matthews, H.; Rawlings, J.M.C.; Richer, J. S.; Roberts, J.; Sadavoy, S.; Simpson, R.J.; Tothill, N.F.H.; Tsamis, Y.G.; Viti, S.; Ward-Thompson, D.; White, G.J.; Yates, J. (2010)
    As part of a James Clerk Maxwell Telescope (JCMT) Legacy Survey of star formation in the Gould Belt, we present early science results for Taurus. CO J= 3 –2 maps have been secured along the north-west ridge and bowl, ...
  • Buckle, J. V.; Davis, C.J.; Di Francesco, J.; Graves, S. F.; Nutter, D.; Richer, J. S.; Roberts, J. F.; Ward-Thompson, D.; White, G.J.; Brunt, C.; Butner, H. M.; Cavanagh, B.; Chrysostomou, A.; Curtis, E.I.; Duarte-Cabral, A.; Etxaluze, M.; Fich, M.; Friberg, P.; Friesen, R.; Fuller, G.A.; Greaves, J.S.; Hatchell, J.; Hogerheijde, M.R.; Johnstone, D.; Matthews, B.; Matthews, H.; Rawlings, J.M.C.; Sadavoy, S.; Simpson, R.J.; Tothill, N.F.H.; Tsamis, Y.G.; Viti, S.; Wouterloot, J. G. A.; Yates, J. (2012-05)
    The Gould Belt Legacy Survey will map star-forming regions within 500 pc, using Heterodyne Array Receiver Programme (HARP), Submillimetre Common-User Bolometer Array 2 (SCUBA-2) and Polarimeter 2 (POL-2) on the James Clerk ...
  • Economou, F.; Jenness, T.; Chrysostomou, A.; Cavanagh, B.; Redman, R.; Berry, D.S. (Astronomical Society of the Pacific, 2008)
    The JCMT Legacy Survey (JLS) is an ambitious programme that will provide the first large-scale survey of the submillimetre sky. From planetary science through to cosmology, the first phase of the campaign will be using the ...
  • Bendo, G.; Wilson, C.D.; Warren, B.E.; Brinks, E.; Butner, H.; Chanial, P.; Clements, D.; Courteau, S.; Irwin, J.; Israel, F.P.; Knapen, J.; Leech, J.; Matthews, H.; Muhle, S.; Petitpas, G.; Serjeant, S.; Tan, B.K.; Tilanus, R.P.J.; Usero, A.; Vaccari, M.; van der Werf, P.; Vlahakis, C.; Wiegert, T.; Zhu, M. (2010)
    We used Spitzer Space Telescope 3.6, 8.0, 70 and 160 μm data, James Clerk Maxwell Telescope HARP-B CO J= (3–2) data, National Radio Astronomy Observatory 12 m telescope CO J= (1–0) data and Very Large Array H i data to ...
  • Wilson, C. D.; Warren, B.E.; Irwin, J.; Knapen, Johan; Israel, F.P.; Sergeant, S.; Attewell, D.; Bendo, G.; Brinks, E.; Butner, H.; Clements, D.; Leech, J.; Mathews, H.E.; Muhle, S.; Mortier, A.M.J.; Parkin, T.J.; Petitpas, G.; Tan, B.K.; Tilanus, R.P.J.; Usero, Antonio; Vaccari, M.; van der Werf, P.; Wiegert, T.; Zhu, M. (2011)
    An analysis of large-area CO J = 3-2 maps from the James Clerk Maxwell Telescope for 12 nearby spiral galaxies reveals low velocity dispersions in the molecular component of the interstellar medium. The three lowest ...
  • Wilson, C.D.; Warren, B.E.; Israel, F.P.; Serjeant, S.; Attewell, D.; Bendo, G. J.; Butner, H. M.; Chanial, P.; Clements, D. L.; Golding, J.; Heesen, V.; Irwin, J.; Leech, J.; Matthews, H.E.; Muhle, S.; Mortier, A.M.J.; Petitpas, G.; Sánchez-Gallego, J.R.; Sinukoff, E.; Shorten, K.; Tan, B.K.; Tilanus, R.P.J.; Usero, A.; Vaccari, M.; Wiegert, T.; Zhu, M.; Alexander, D.M.; Alexander, P.; Azimlu, M.; Barmby, P.; Brar, R.; Bridge, C.; Brinks, E.; Brooks, S.; Coppin, Kristen; Côté, S.; Côté, P.; Courteau, S.; Davies, J.; Eales, S.; Fich, M.; Hudson, M.; Hughes, D.H.; Ivison, R.J.; Knapen, J.H.; Page, M.; Parkin, T.J.; Rigopoulou, D.; Rosolowsky, E.; Seaquist, E.R.; Spekkens, K.; Tanvir, N.; van der Hulst, J.M.; van der Werf, P.; Vlahakis, C.; Webb, T.M.; Weferling, B.; White, G.J. (2012-08-21)
    The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey (NGLS) comprises an Hi-selected sample of 155 galaxies spanning all morphological types with distances less than 25Mpc. We describe the scientific goals of ...
  • Irwin, J.; Wilson, C. D.; Wiegert, T.; Bendo, G.; Warren, B.E.; Wang, Q.D.; Israel, F.P.; Sergeant, S.; Knapen, Johan; Brinks, E.; Tilanus, R.P.J.; van der Werf, P.; Muhle, S. (2011)
    We have made the first map of CO(J = 3-2) emission covering the disc of the edge-on galaxy, NGC 4631, which is known for its spectacular gaseous halo. The strongest emission, which we model with a Gaussian ring, occurs ...
  • Granot, J.; Kumar, P.; Piran, T. (2004)
  • Sandell, G.; Avery, L.W.; Baas, F.; Coulson, I.M.; Dent, W.R.; Friberg, P.; Gear, W.P.K.; Greaves, J.S.; Holland, W.S.; Jenness, T.; Jewell, P.; Lightfoot, J.F.; Matthews, H.; Moriarty-Schieven, G.; Prestage, R.; Robson, E.I.; Stevens, J. A.; Tilanus, R.P.J.; Watt, G.D. (1999)
  • Croston, J.H. (Astronomical Society of the Pacific, 2008)
    The interactions between low-power radio galaxies and their environments are thought to play a crucial role in supplying energy to offset cooling in the centres of groups and clusters. Such interactions are also important ...
  • Croston, J.H.; Hardcastle, M.J.; Birkinshaw, M.; Worrall, D.M. (2004)
    We present the results of new XMM-Newton observations of FRI and FRII radio galaxies that show the importance of jet/environment interactions for both radiosource structure and the properties of the surrounding gas. The ...
  • Kraft, R.P.; Forman, W.R.; Hardcastle, M.J.; Birkinshaw, M.; Croston, J.H.; Jones, C.; Nulsen, P.E.J.; Worrall, D.M.; Murray, S.S. (2009)
    We present results from a 40 ks XMM-Newton observation of the X-ray filament coincident with the southeast edge of the Centaurus A Northern Middle Radio Lobe (NML). We find that the X-ray filament consists of five spatially ...

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