Bibcode
MacKenzie, Todd; Braglia, Filiberto G.; Gibb, Andy G.; Scott, Douglas; Jenness, Tim; Serjeant, Stephen; Thompson, Mark; Berry, David; Brunt, Christopher M.; Chapin, Edward; Chrysostomou, Antonio; Clements, Dave; Coppin, Kristen; Economou, Frossie; Evans, A.; Friberg, Per; Greaves, Jane; Hill, T.; Holland, Wayne; Ivison, R. J.; Knapen, J. H.; Jackson, Neal; Joncas, Gilles; Morgan, Larry; Mortier, Angela; Pearson, Chris; Pestalozzi, Michele; Pope, Alexandra; Richer, John; Urquhart, J. S.; Vaccari, Mattia; Weferling, Bernd; White, Glenn; Zhu, Ming
Bibliographical reference
Monthly Notices of the Royal Astronomical Society, Volume 415, Issue 2, pp. 1950-1960.
Advertised on:
8
2011
Citations
9
Refereed citations
7
Description
We have carried out a pilot study for the Submillimetre Common-User
Bolometer Array 2 (SCUBA-2) ‘All-Sky’ Survey (SASSy), a wide
and shallow mapping project at 850 μm, 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 × 0?5 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
deg2 around the W5-E H II region. As well as diffuse
structure in the map, a filtering approach was able to extract 27
compact sources with signal-to-noise ratio 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.
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Our small group is well known and respected internationally for our innovative and important work on various aspects of the structure and evolution of nearby spiral galaxies. We primarily use observations at various wavelengths, exploiting synergies that allow us to answer the most pertinent questions relating to what the main properties of
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