dc.contributor.author | Eden, DJ | |
dc.contributor.author | Moore, TJT | |
dc.contributor.author | Currie, MJ | |
dc.contributor.author | Rigby, AJ | |
dc.contributor.author | Rosolowsky, E | |
dc.contributor.author | Su, Y | |
dc.contributor.author | Kim, K-T | |
dc.contributor.author | Parsons, H | |
dc.contributor.author | Morata, O | |
dc.contributor.author | Chen, H-R | |
dc.contributor.author | Minamidani, T | |
dc.contributor.author | Park, G | |
dc.contributor.author | Ragan, SE | |
dc.contributor.author | Urquhart, JS | |
dc.contributor.author | Rani, R | |
dc.contributor.author | Tahani, K | |
dc.contributor.author | Billington, SJ | |
dc.contributor.author | Deb, S | |
dc.contributor.author | Figura, C | |
dc.contributor.author | Fujiyoshi, T | |
dc.contributor.author | Joncas, G | |
dc.contributor.author | Liao, LW | |
dc.contributor.author | Liu, T | |
dc.contributor.author | Ma, H | |
dc.contributor.author | Tuan-Anh, P | |
dc.contributor.author | Yun, H-S | |
dc.contributor.author | Zhang, S | |
dc.contributor.author | Zhu, M | |
dc.contributor.author | Henshaw, JD | |
dc.contributor.author | Longmore, SN | |
dc.contributor.author | Kobayashi, MIN | |
dc.contributor.author | Thompson, MA | |
dc.contributor.author | Ao, Y | |
dc.contributor.author | Campbell-White, J | |
dc.contributor.author | Ching, T-C | |
dc.contributor.author | Chung, EJ | |
dc.contributor.author | Duarte-Cabral, A | |
dc.contributor.author | Fich, M | |
dc.contributor.author | Gao, Y | |
dc.contributor.author | Graves, SF | |
dc.contributor.author | Jiang, X-J | |
dc.contributor.author | Kemper, F | |
dc.contributor.author | Kuan, Y-J | |
dc.contributor.author | Kwon, W | |
dc.contributor.author | Lee, CW | |
dc.contributor.author | Lee, JE | |
dc.contributor.author | Liu, M | |
dc.contributor.author | Penaloza, CH | |
dc.contributor.author | Peretto, N | |
dc.contributor.author | Phuong, NT | |
dc.contributor.author | Pineda, JE | |
dc.contributor.author | Plume, R | |
dc.contributor.author | Puspitaningrum, E | |
dc.contributor.author | Samal, MR | |
dc.contributor.author | Soam, A | |
dc.contributor.author | Sun, Y | |
dc.contributor.author | Tang, XD | |
dc.contributor.author | Traficante, A | |
dc.contributor.author | White, GJ | |
dc.contributor.author | Yan, C-H | |
dc.contributor.author | Yang, AY | |
dc.contributor.author | Yuan, J | |
dc.contributor.author | Yue, N | |
dc.contributor.author | Bemis, A | |
dc.contributor.author | Brunt, CM | |
dc.contributor.author | Chen, Z | |
dc.contributor.author | Cho, J | |
dc.contributor.author | Clark, PC | |
dc.contributor.author | Cyganowski, CJ | |
dc.contributor.author | Friberg, P | |
dc.contributor.author | Fuller, GA | |
dc.contributor.author | Han, I | |
dc.contributor.author | Hoare, MG | |
dc.contributor.author | Izumi, N | |
dc.contributor.author | Kim, H-J | |
dc.contributor.author | Kim, J | |
dc.contributor.author | Kim, S | |
dc.contributor.author | Koch, EW | |
dc.contributor.author | Kuno, N | |
dc.contributor.author | Lacialle, KM | |
dc.contributor.author | Lai, S-P | |
dc.contributor.author | Lee, H | |
dc.contributor.author | Lee, Y-H | |
dc.contributor.author | Li, DL | |
dc.contributor.author | Liu, S-Y | |
dc.contributor.author | Mairs, S | |
dc.contributor.author | Pan, Z | |
dc.contributor.author | Qian, L | |
dc.contributor.author | Scicluna, P | |
dc.contributor.author | Shi, C-S | |
dc.contributor.author | Shi, H | |
dc.contributor.author | Srinivasan, S | |
dc.contributor.author | Tan, Q-H | |
dc.contributor.author | Thomas, HS | |
dc.contributor.author | Torii, K | |
dc.contributor.author | Trejo, A | |
dc.contributor.author | Umemoto, T | |
dc.contributor.author | Violino, G | |
dc.contributor.author | Wallstrom, S | |
dc.contributor.author | Wang, B | |
dc.contributor.author | Wu, Y | |
dc.contributor.author | Yuan, L | |
dc.contributor.author | Zhang, C | |
dc.contributor.author | Zhang, M | |
dc.contributor.author | Zhou, C | |
dc.contributor.author | Zhou, JJ | |
dc.date.accessioned | 2020-10-19T14:14:26Z | |
dc.date.issued | 2020-09-10 | |
dc.description.abstract | The latest generation of Galactic Plane surveys is enhancing our ability to study the effects of galactic environment upon the
process of star formation. We present the first data from CO Heterodyne Inner Milky Way Plane Survey 2 (CHIMPS2). CHIMPS2
is a survey that will observe the Inner Galaxy, the Central Molecular Zone (CMZ), and a section of the Outer Galaxy in 12CO,
13CO, and C18O (J = 3 → 2) emission with the Heterodyne Array Receiver Program on the James Clerk Maxwell Telescope
(JCMT). The first CHIMPS2 data presented here are a first look towards the CMZ in 12CO J = 3 → 2 and cover −3◦ ≤ ≤ 5◦
and | b | ≤ 0.
◦5 with angular resolution of 15 arcsec, velocity resolution of 1 km s−1, and rms T ∗
A = 0.58 K at these resolutions.
Such high-resolution observations of the CMZ will be a valuable data set for future studies, whilst complementing the existing
Galactic Plane surveys, such as SEDIGISM, the Herschel infrared Galactic Plane Survey, and ATLASGAL. In this paper, we
discuss the survey plan, the current observations and data, as well as presenting position–position maps of the region. The
position–velocity maps detect foreground spiral arms in both absorption and emission. | en_GB |
dc.identifier.citation | Vol 498, 5396-6951 | en_GB |
dc.identifier.doi | 10.1093/mnras/staa2734 | |
dc.identifier.uri | http://hdl.handle.net/10871/123304 | |
dc.language.iso | en | en_GB |
dc.publisher | Oxford University Press (OUP) | en_GB |
dc.rights | © 2020 The Author(s)
Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. | en_GB |
dc.subject | molecular data | en_GB |
dc.subject | surveys | en_GB |
dc.subject | stars | en_GB |
dc.subject | formation | en_GB |
dc.subject | ISM | en_GB |
dc.subject | molecules | en_GB |
dc.subject | Galaxy | en_GB |
dc.subject | centre | en_GB |
dc.title | CHIMPS2: survey description and 12CO emission in the Galactic Centre | en_GB |
dc.type | Article | en_GB |
dc.date.available | 2020-10-19T14:14:26Z | |
dc.identifier.issn | 0035-8711 | |
dc.description | This is the advance access final version. The final version is available from the publisher via the DOI in this record | en_GB |
dc.description | The reduced CHIMPS2 12CO CMZ data are available to download
from the CANFAR archive. https://www.canfar.net/citation/landing?doi=20.0004. The data are available as mosaic roughly 2◦ × 1◦ in size, as well as the individual observations.
Integrated − b and − VLSR maps, displayed in Section 5 for the
whole CMZ are provided, as well as the − VLSR maps for the
individual cubes. The data are presented in FITS format.
The raw data are also downloadable from the JCMT Science
Archive3 hosted by the Canadian Astronomy Data Centre using the
Project ID M17BL004. | en_GB |
dc.identifier.journal | Monthly Notices of the Royal Astronomical Society | en_GB |
dc.rights.uri | http://www.rioxx.net/licenses/all-rights-reserved | en_GB |
dcterms.dateAccepted | 2020-09-04 | |
rioxxterms.version | VoR | en_GB |
rioxxterms.licenseref.startdate | 2020-09-04 | |
rioxxterms.type | Journal Article/Review | en_GB |
refterms.dateFCD | 2020-10-19T12:30:06Z | |
refterms.versionFCD | AM | |
refterms.dateFOA | 2020-10-19T14:14:34Z | |
refterms.panel | B | en_GB |