Moore, TJT and Plume, R and Thompson, MA and Parsons, H and Urquhart, JS and Eden, DJ and Dempsey, JT and Morgan, LK and Thomas, HS and Buckle, J and Brunt, CM and Butner, H and Carretero, D and Chrysostomou, A and deVilliers, HM and Fich, M and Hoare, MG and Manser, G and Mottram, JC and Natario, C and Olguin, F and Peretto, N and Polychroni, D and Redman, RO and Rigby, AJ and Salji, C and Summers, LJ and Berry, D and Currie, MJ and Jenness, T and Pestalozzi, M and Traficante, A and Bastien, P and diFrancesco, J and Davis, CJ and Evans, A and Friberg, P and Fuller, GA and Gibb, AG and Gibson, S and Hill, T and Johnstone, D and Joncas, G and Longmore, SN and Lumsden, SL and Martin, PG and Lu'o'ng, QN and Pineda, JE and Purcell, C and Richer, JS and Schieven, GH and Shipman, R and Spaans, M and Taylor, AR and Viti, S and Weferling, B and White, GJ and Zhu, M (2015) The JCMT Plane Survey: early results from the l=30 degrees field. Monthly Notices of the Royal Astronomical Society, 453 (4). 4264 -4277. ISSN 1365-2966

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Abstract

We present early results from the JCMT (James Clerk Maxwell Telescope) Plane Survey (JPS), which has surveyed the northern inner Galactic plane between longitudes = 7◦ and = 63◦ in the 850-µm continuum with SCUBA-2 (Submm Common-User Bolometer Array 2), as part of the JCMT Legacy Survey programme. Data from the = 30◦ survey region, which contains the massive-star-forming regions W43 and G29.96, are analysed after approximately 40 per cent of the observations had been completed. The pixel-to-pixel noise is found to be 19 mJy beam−1 after a smooth over the beam area, and the projected equivalent noise levels in the final survey are expected to be around 10 mJy beam−1. An initial extraction of compact sources was performed using the FELLWALKER method, resulting in the detection of 1029 sources above a 5σ surface-brightness threshold. The completeness limits in these data are estimated to be around 0.2 Jy beam−1 (peak flux density) and 0.8 Jy (integrated flux density) and are therefore probably already dominated by source confusion in this relatively crowded section of the survey. The flux densities of extracted compact sources are consistent with those of matching detections in the shallower APEX (Atacama Pathfinder Experiment) Telescope Large Area Survey of the Galaxy (ATLASGAL) survey. We analyse the virial and evolutionary state of the detected clumps in the W43 star-forming complex and find that they appear younger than the Galactic-plane average.

Item Type: Article
Additional Information: This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2015 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
Uncontrolled Keywords: surveys, stars, formation, ISM, clouds, individual, objexts, W43, submillimetre,
Subjects: Q Science > QB Astronomy
Divisions: Faculty of Natural Sciences > School of Physical and Geographical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 03 Feb 2016 11:53
Last Modified: 19 Sep 2017 10:58
URI: http://eprints.keele.ac.uk/id/eprint/1436

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