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pro vyhledávání: '"B. Weferling"'
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Autor:
Antonio Chrysostomou, J. diFrancesco, F. A. Olguin, M. Fich, Glenn J. White, D. Johnstone, Per Friberg, M. Spaans, Melvin Hoare, Mark Thompson, R. O. Redman, D. Polychroni, Cormac Purcell, Harold M. Butner, A. R. Taylor, Christopher M. Brunt, M. J. Currie, Joseph C. Mottram, Jaime E. Pineda, David S. Berry, Harriet Parsons, Rene Plume, Alessio Traficante, Gerald Schieven, B. Weferling, Q. Nguyen Luong, David Eden, Andrew Rigby, Peter G. Martin, C. Natario, S. N. Longmore, L. J. Summers, L. K. Morgan, James Urquhart, Nicolas Peretto, Andy Gibb, John Richer, D. Carretero, Steven J. Gibson, M. Zhu, T. Jenness, Gary A. Fuller, H. M. deVilliers, Jessica T. Dempsey, Pierre Bastien, Christopher J. Davis, Serena Viti, G. Manser, Toby J. T. Moore, A. Evans, C. Salji, M. R. Pestalozzi, R. Shipman, Tracey Hill, Gilles Joncas, Stuart Lumsden, Jane V. Buckle, H. Thomas
Publikováno v:
Monthly Notices of the Royal Astronomical Society, 453(4), 4264-4277
Monthly Notices of the Royal Astronomical Society, 453(4), 4264-4277. Oxford University Press
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 453(4), 4264-4277. Oxford University Press
Monthly Notices of the Royal Astronomical Society
We present early results from the JCMT (James Clerk Maxwell Telescope) Plane Survey (JPS), which has surveyed the northern inner Galactic plane between longitudes ℓ = 7° and ℓ = 63° in the 850-μm continuum with SCUBA-2 (Submm Common-User Bolom
Autor:
Andy Gibb, Antonio Chrysostomou, Stephen Serjeant, Will Nettke, Ming Zhu, Toby J. T. Moore, Tim Jenness, Glenn J. White, Alistair R. Evans, B. Weferling, Douglas Scott, Tracey Hill, Gilles Joncas, Mark Thompson, James Urquhart, Mattia Vaccari
The SCUBA-2 Ambitious Sky Survey (SASSy) is composed of shallow 850-$\umu$m imaging using the Sub-millimetre Common-User Bolometer Array 2 (SCUBA-2) on the James Clerk Maxwell Telescope. Here we describe the extraction of a catalogue of beam-sized so
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::658cbcf0192077f10cfa2b997d8e61c0
http://oro.open.ac.uk/48878/1/1703.01930.pdf
http://oro.open.ac.uk/48878/1/1703.01930.pdf
Autor:
Steven N. Longmore, L. J. Summers, Alessio Traficante, Melvin Hoare, Joseph C. Mottram, David S. Berry, M. J. Currie, H. Thomas, D. Polychroni, Harriet Parsons, Mark Thompson, Rene Plume, R. O. Redman, C. Natario, Glenn J. White, David Eden, D. Johnstone, J. diFrancesco, M. Fich, K. Tahani, Christopher M. Brunt, J. V. Buckle, C. Salji, M. Zhu, T. Jenness, L. K. Morgan, Gary A. Fuller, M. R. Pestalozzi, Harold M. Butner, A. Chrysostomou, Andrew Rigby, James Urquhart, A. Evans, Andy Gibb, G. Manser, J. S. Richer, G. Joncas, B. Weferling, Toby J. T. Moore, Jessica Dempsey, F. A. Olguin, Nicolas Peretto, H. M. deVilliers, Peter G. Martin, D. Carretero
We present the first data release of the James Clerk Maxwell Telescope (JCMT) Plane Survey (JPS), the JPS Public Release 1 (JPSPR1). JPS is an 850-um continuum survey of six fields in the northern inner Galactic Plane in a longitude range of l=7-63,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adfb62a98891071f87e4db46495f7293
Autor:
B. Weferling, Henry E. Matthews, A. Evans, Martin Cohen, James M. Jackson, Helen Kirk, William R. F. Dent, Jill Rathborne, Doug Johnstone, Gary A. Fuller, Tim Jenness, R. Simon, G. Davis, John Richer
Publikováno v:
The Astronomical Journal. 138:1380-1402
We present imaging observations of continuum emission from interstellar dust at 850 and 1200 μm of a section of the Galactic Plane covering 2 deg2 centered at ℓ = 44°. Complementary jiggle-mapping and fast-scanning techniques were used, respectiv
Autor:
Per Friberg, Jeremy Yates, Gary A. Fuller, Rene Plume, Andy Gibb, John Richer, Tom J. Millar, Harold M. Butner, Marco Spaans, J. Hatchell, George F. Mitchell, J. G. A. Wouterloot, Frank Helmich, Glenn J. White, Emmanuel Caux, M. Zhu, Toby J. T. Moore, Jane V. Buckle, Serena Viti, J. E. Bowey, E. F. van Dishoeck, F. F. S. van der Tak, Cecilia Ceccarelli, Mark Thompson, Volker Ossenkopf, A. G. G. M. Tielens, M. Roellig, H. Roberts, H. E. Matthews, Michiel R. Hogerheijde, B. Weferling, Peter Schilke, J. M. C. Rawlings
Publikováno v:
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2007, 119, pp.102. ⟨10.1086/511161⟩
Publications of the Astronomical Society of the Pacific, 119(851), 102-111
Publications of the Astronomical Society of the Pacific, Astronomical Society of the Pacific, 2007, 119, pp.102. ⟨10.1086/511161⟩
Publications of the Astronomical Society of the Pacific, 119(851), 102-111
International audience; 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 the m
Autor:
B. Weferling
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 362:263-267
Relations are presented between the optical depth of the atmosphere (τ) in the millimetre and submillimetre windows at 350, 450, 850 and 1250 μm. These relations are derived by an analysis of 849 skydips at 850 μm performed with the submillimetre
Publikováno v:
Astronomy & Astrophysics. 383:1088-1099
Ground-based astronomical continuum observations at (sub)millimeter wavelengths are especially difficult, because the emission of the atmospheric water vapor is usually much stronger than any astronomical signal. We present here the principles of the
Publikováno v:
Astronomy & Astrophysics. 379:735-739
Fastscanning is a new observing technique for millimeter and submillimeter astronomy from ground based telescopes. The atmosphere is eliminated by taking advantage of detector arrays. Instead of wobbling the secondary mirror with a fixed frequency of
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 444:404-407
At the Max-Planck-Institut fur Radioastronomie we built a 19-channel bolometer array for 150 GHz operating at 100 mK. We give an overview of how our new bolometer array is installed at mm/submm telescopes. With results obtained during observing runs