The Southern Galactic Plane Survey: H i Observations and Analysis
Author(s) -
N. M. McClureGriffiths,
J. M. Dickey,
B. M. Gaensler,
A. J. Green,
M. Haverkorn,
S. Strasser
Publication year - 2005
Publication title -
the astrophysical journal supplement series
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.546
H-Index - 277
eISSN - 1538-4365
pISSN - 0067-0049
DOI - 10.1086/430114
Subject(s) - galactic plane , physics , milky way , telescope , astrophysics , astronomy , radio telescope , galaxy , interstellar medium , galactic astronomy , data reduction , computer science , data mining
We describe the HI component of the Southern Galactic Plane Survey (SGPS).The SGPS is a large-scale project to image at arcminute resolution the HIspectral line and 21 cm continuum emission in parts of the plane of the MilkyWay. The survey covers Galactic longitudes 253 deg < l < 358 deg and latitudes|b| <1.5 deg (SGPS I), plus a first quadrant extension covering 5 deg < l < 20deg and |b| <1.5 deg (SGPS II). The survey combines data from the AustraliaTelescope Compact Array and the Parkes Radio Telescope for sensitivity toangular scales ranging from 2 arcminutes to several degrees. The combined datacover 325 sq-deg and have an rms sensitivity of 1.6 K. Here we describe the HIobservations and data reduction in detail, and present examples from the finaldata products. The complete dataset is publicly available through the AustraliaTelescope National Facility's HI Surveys archive. This dataset provides anunprecedented view of the neutral component of interstellar hydrogen in theinner Milky Way.
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