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Table 2

Results of the VLA H2O maser observations of our program stars.

Name CGCS V LSR Searched VLSR Maser VLSR V peak S peak S I RMS noise
range (km s-1) range (km s-1) (km s-1) (Jy) (10-21 W m-2) (mJy)

IRAS 06017+1011 1158 −13.0 −54.6 ... +28.3 −24.0 ... −15.1 −24.0 4.2 6.5 5.3
−18.4 0.15
−15.1 0.14
BM Gem 1653 +76.1 +34.0 ... +118.2 <0.015 5.1
IRAS 07221-0431 1698 +79.0 +36.9 ... +121.1 <0.023 7.8
IRAS 08002-3803 2011 0.0 −42.1 ... +42.1 <0.045 15.0
IRAS 18006-3213 3935 +176.7 +134.6 ... +218.8 <0.033 11.0
NC83 4222 −6.7 −48.3 ... +34.6 −8.2 ... +5.6 −8.2 5.2 6.9 7.3
+1.7 0.03
+3.6 0.06
+5.6 0.13
HD 189605 4595 +58.2 +16.1 ... +100.3 <0.024 7.9
V778 Cyg 4923 −17.0 −58.3 ... +24.6 −25.0 ... −14.2 −25.0...−20.1 0.05–0.07 100 22.0
−19.5 0.22
−16.8 90.4
−14.2 0.21
V1415 Cyg 5548 0.0 −81.7 ... +81.6 −34.3 ... −21.1 −26.4 0.31 2.1 3.5
EU And 5848 −36.0 −77.5 ... +5.4 −42.0 ... −34.1 −42.0 3.6 16 5.2
−39.3 0.62
−34.1 7.4

Notes. The central velocity and the searched velocity range, as well as the RMS noise level are listed. For positive detections, the velocity (Vpeak) and intensity (Speak) of each peak are listed, together with the integrated flux (SI). For nondetection sources, the upper limit (3σ RMS noise) is listed.

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