Abstract
The JCMT Gould Belt survey has now collected 25 % of its SCUBA-2 data. We report on the quality of these data, and demonstrate how we can map all of the star-formation in the Gould Belt down to our original sensitivity in our allocated time. We describe how the SCUBA-2 and Herschel datasets are highly complementary, and how the SCUBA-2 data add value to the Herschel data, giving a more reliable measure of the column density at higher angular resolution.
This is a preview of subscription content, log in via an institution to check access.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
References
Buckle J. V., et al., 2010, MNRAS, 401, 204
Buckle J. V., et al., 2012, MNRAS, 422, 521
Christie H., et al., 2012, MNRAS, 422, 968
Davis C. J., et al., 2010, MNRAS, 405, 759
Graves S. F., et al., 2010, MNRAS, 409, 1412
Kirk J., et al., 2012, This Publication
Nutter D., Ward-Thompson D., 2007, MNRAS, 374, 1413
Ward-Thompson D., et al., 2007, PASP, 119, 855
Author information
Authors and Affiliations
Corresponding author
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 2014 Springer International Publishing Switzerland
About this paper
Cite this paper
Nutter, D. (2014). Initial Results from SCUBA-2. In: Stamatellos, D., Goodwin, S., Ward-Thompson, D. (eds) The Labyrinth of Star Formation. Astrophysics and Space Science Proceedings, vol 36. Springer, Cham. https://doi.org/10.1007/978-3-319-03041-8_45
Download citation
DOI: https://doi.org/10.1007/978-3-319-03041-8_45
Published:
Publisher Name: Springer, Cham
Print ISBN: 978-3-319-03040-1
Online ISBN: 978-3-319-03041-8
eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)