A pilot study for the SCUBA-2 'All-Sky' Survey

Autor: Mackenzie, T, Braglia, FG, Gibb, AG, Scott, D, Jenness, T, Serjeant, S, Thompson, M, Berry, D, Brunt, CM, Chapin, E, Chrysostomou, A, Clements, D, Coppin, K, Economou, F, Evans, A, Friberg, P, Greaves, J, Hill, T, Holland, W, Ivison, RJ, Knapen, JH, Jackson, N, Joncas, G, Morgan, L, Mortier, A, Pearson, C, Pestalozzi, M, Pope, A, Richer, J, Urquhart, JS, Vaccari, M, Weferling, B, White, G, Zhu, M
Přispěvatelé: Astrophysique Interprétation Modélisation (AIM (UMR7158 / UMR_E_9005 / UM_112)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Science and Technology Facilities Council (STFC)
Jazyk: angličtina
Rok vydání: 2011
Předmět:
Zdroj: Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2011, 415, pp.1950-1960. ⟨10.1111/j.1365-2966.2011.18840.x⟩
ISSN: 0035-8711
1365-2966
Popis: We have carried out a pilot study for the SCUBA-2 'All-Sky' Survey, SASSy, a wide and shallow mapping project at 850 microns, designed to find rare objects, both Galactic and extragalactic. Two distinct sets of exploratory observations were undertaken, and used to test the SASSy approach and data reduction pipeline. The first was a 0.5 by 0.5 degrees map around the nearby galaxy NGC 2559. The galaxy was easily detected at 156 mJy, but no other convincing sources are present in the map. Comparison with other galaxies with similar wavelength coverage indicates that NGC 2559 has relatively warm dust. The second observations cover 1 square degree around the W5-E HII region. As well as diffuse structure in the map, a filtering approach was able to extract 27 compact sources with signal-to-noise greater than 6. By matching with data at other wavelengths we can see that the SCUBA-2 data can be used to discriminate the colder cores. Together these observations show that the SASSy project will be able to meet its original goals of detecting new bright sources which will be ideal for follow-up observations with other facilities.
12 pages, including 14 figures
Databáze: OpenAIRE
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