The Canadian Galactic Plane Survey

被引:491
|
作者
Taylor, AR [1 ]
Gibson, SJ
Peracaula, M
Martin, PG
Landecker, TL
Brunt, CM
Dewdney, PE
Dougherty, SM
Gray, AD
Higgs, LA
Kerton, CR
Knee, LBG
Kothes, R
Purton, CR
Uyaniker, B
Wallace, BJ
Willis, AG
Durand, D
机构
[1] Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada
[2] Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
[3] Natl Res Council Canada, Herzberg Inst Astrophys, Domin Radio Astrophys Observ, Penticton, BC V2A 6J9, Canada
[4] Natl Res Council Canada, Herzberg Inst Astrophys, Canadian Astron Data Ctr, Victoria, BC V9E 2E7, Canada
来源
ASTRONOMICAL JOURNAL | 2003年 / 125卷 / 06期
关键词
Galaxy : general; ISM : general; ISM : structure; surveys;
D O I
10.1086/375301
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Canadian Galactic Plane Survey (CGPS) is a project to combine radio, millimeter, and infrared surveys of the Galactic plane to provide arcminute-scale images of all major components of the interstellar medium over a large portion of the Galactic disk. We describe in detail the observations for the low-frequency component of the CGPS, the radio surveys carried out at the Dominion Radio Astrophysical Observatory (DRAO), and summarize the properties of the merged database of surveys that comprises the CGPS. The DRAO Synthesis Telescope surveys have imaged a 73degrees section of the Galactic plane, using similar to85% of the telescope time between 1995 April and 2000 June. The observations provide simultaneous radio continuum images at two frequencies, 408 and 1420 MHz, and spectral-line images of the lambda = 21 cm transition of neutral atomic hydrogen. In the radio continuum at 1420 MHz, dual-polarization receivers provide images in all four Stokes parameters. The surveys cover the region 74.degrees2 < l < 147.degrees3, with latitude extent - 3.degrees6 < b < +5.degrees6 at 1420 MHz and - 6.degrees7 < b < -8.degrees7 at 408 MHz. By integration of data from single-antenna observations, the survey images provide complete information on all scales of emission structures down to the resolution limit, which is just below 1' x 1' csc delta at 1420 MHz and 3.'4 x 3.'4 csc delta at 408 MHz. The continuum images have a dynamic range of several thousand, yielding essentially noise-limited images with an rms of similar to0.3 mJy beam(-1) at 1420 MHz and similar to3 mJy beam(-1) at 408 MHz. The spectral-line data are noise limited with rms brightness temperature DeltaT(B) similar to 3 K in a 0.82 km s(-1) channel. The complete CGPS data set, including the DRAO surveys and data at similar resolution in (CO)-C-12 ( 1 - 0) and in infrared emission from dust, all imaged to an identical Galactic coordinate grid and map projection, are being made publicly available through the Canadian Astronomy Data Centre.
引用
收藏
页码:3145 / 3164
页数:20
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