Subarcsecond resolution observations of warm water toward three deeply embedded low-mass protostars

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Table 2

Parameters for the sources from elliptical Gaussian fits to their continuum emission.

	IRAS2A	IRAS4A-NW	IRAS4A-SE

Flux (±)^a	0.24 (0.002) Jy	0.88 (0.025) Jy	1.46 (0.021) Jy
RA (±)^b	03:28:55.57 (0004)	03:29:10.44 (002)	03:29:10.53 (0005)
Dec (±)^b	31:14:37.03 (0004)	31:13:32.16 (002)	31:13:30.92 (0006)
Extent^c

Notes. Errors given are the statistical errors from the fitting routine.

^(a)

Statistical error from fit, the calibration dominates the uncertainty in the flux determination.

^(b)

J2000 epoch. Statistical error from fit.

^(c)

Major × Minor axis and position angle for elliptical Gaussian profile in (u,v) plane. The statistical error of the extent is typically 0.5−3%.

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