A Survey of the polarized emission from the Galactic plane at 1420 MHz with arcminute angular resolution

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Table 1:

DRAO Synthesis Telescope survey characteristics.
Coverage	${66^{\circ}} < {\ell} < {175^{\circ}}, {-3^{\circ}} < {b} < {5^{\circ}}$ ;
	${101^{\circ}} < {\ell} < {116^{\circ}}, {5.0^{\circ}} < {b} < {17\hbox{$.\!\!^\circ$ }5}$
Individual field size	107 $.\mkern-4mu^\prime$ 2 diameter to 50%
	150 $.\mkern-4mu^\prime$ 0 diameter to 25.7%
Field used in mosaicking	150 $^\prime$ diameter
Field centre spacing	112 $^\prime$ on triangular grid
Observation dates	1995.3 to 2004.4
Survey area	1060 square degrees
Observing rate	150 square degrees per year
Bandwidth	30 MHz in four bands of
	7.5 MHz each
Centre frequencies	1407.2, 1414.1, 1427.7,
	and 1434.6 MHz
Angular resolution	$58'' \times 58''$ cosec $\delta$
System temperature	60 K, 1995.3 to 2003.4;
	45 K, 2003.4 to 2004.4
Sensitivity (mosaicked data)	0.30 mJy/beam rms 1995.3 to 2003.4
	${76}\thinspace{\rm {sin{\thinspace}(declination)}}$ mK;
	0.23 mJy/beam rms 2003.4 to 2004.4
	${58}\thinspace{\rm {sin{\thinspace}(declination)}}$ mK

Source LaTeX | All tables | In the text

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