The HI Parkes All Sky Survey:: southern observations, calibration and robust imaging

被引:512
作者
Barnes, DG
Staveley-Smith, L
de Blok, WJG
Oosterloo, T
Stewart, IM
Wright, AE
Banks, GD
Bhathal, R
Boyce, PJ
Calabretta, MR
Disney, MJ
Drinkwater, MJ
Ekers, RD
Freeman, KC
Gibson, BK
Green, AJ
Haynes, RF
Hekkert, PTL
Henning, PA
Jerjen, B
Juraszek, S
Kesteven, MJ
Kilborn, VA
Knezek, PM
Koribalski, B
Kraan-Korteweg, RC
Malin, DE
Marquarding, M
Minchin, RF
Mould, JR
Price, RM
Putman, ME
Ryder, SD
Sadler, EM
Schröder, A
Stootman, F
Webster, RL
Wilson, WE
Ye, T
机构
[1] CSIRO, Australia Telescope Natl Facil, Epping, NSW 1710, Australia
[2] Swinburne Univ Technol, Ctr Astrophys & Supercomp, Hawthorn, Vic 3122, Australia
[3] Netherlands Fdn Res Astron, NL-7990 AA Dwingeloo, Netherlands
[4] Univ Leicester, Dept Phys & Astron, Leicester LE1 7RH, Leics, England
[5] Univ Wales, Dept Phys & Astron, Cardiff CF24 3YB, S Glam, Wales
[6] Univ Western Sydney Macarthur, Dept Phys, Campbelltown, NSW 2560, Australia
[7] Univ Bristol, Dept Phys, Bristol BS8 1TL, Avon, England
[8] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia
[9] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia
[10] Univ Sydney, Sch Phys, Sydney, NSW 2006, Australia
[11] Univ New Mexico, Inst Astrophys, Albuquerque, NM 87131 USA
[12] Space Telescope Sci Inst, Baltimore, MD 21218 USA
[13] Univ Guanajuato, Dept Astron, Guanajuato 36000, Mexico
[14] Anglo Australian Observ, Epping, NSW 1710, Australia
[15] Observ Cote Azur, F-06304 Nice 4, France
关键词
instrumentation : detectors; methods : observational; methods : statistical; techniques : image processing; surveys; radio lines : galaxies;
D O I
10.1046/j.1365-8711.2001.04102.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The acquisition of HI Parkes All Shy Survey (HIPASS) southern sky data commenced at the Australia Telescope National Facility's Parkes 64-m telescope in 1997 February, and was completed in 2000 March. HIPASS is the deepest HI survey yet of the sky south of declination +2 degrees, and is sensitive to emission out to 170 h(75)(-1) Mpc. The characteristic root mean square noise in the survey images is 13.3 mJy. This paper describes the survey observations, which comprise 23 020 eight-degree scans of 9-min duration, and details the techniques used to calibrate and image the data. The processing algorithms are successfully designed to be statistically robust to the presence of interference signals, and are particular to imaging point (or nearly point) sources. Specifically, a major improvement in image quality is obtained by designing a median-gridding algorithm which uses the median estimator in place of the mean estimator.
引用
收藏
页码:486 / 498
页数:13
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