Table 3: Sources observed during the first observing run only. Columns 6-9 give the peak of each line or the rms level of the spectrum, both in K.
IRAS RA (J2000) Dec. (J2000) $V_{\rm LSR}$ $d_{\rm kin}$ N2H+ (1-0) N2H+ (3-2) N2D+ (2-1) N2D+ (3-2)
Source (h m s) ($^{\circ}$ ' '') (km s-1) (kpc)        
IRAS 05490+26582 05 52 12.9 26 59 33 0.8 2.1 0.4 ${\leq} 0.9$ ${\leq} 0.19$ ${\leq} 0.3$
IRAS 18567+07001 18 59 13.6 07 04 47 29.4 2.16 0.5 ${\leq} 0.4$ ${\leq} 0.13$ ${\leq} 0.2$
IRAS 20106+35451 20 12 31.2 35 54 46 7.8 1.6 0.5 0.45 ${\leq} 0.05$ ${\leq} 0.05$
IRAS 20205+39482 20 22 21.9 39 58 05 -1.7 4.5 $\leq$0.03 ${\leq} 0.1$ ${\leq} 0.05$ ${\leq} 0.05$
IRAS 20278+35211 20 29 46.9 35 31 39 -4.5 5.0 0.3 ${\leq} 0.2$ ${\leq} 0.06$ ${\leq} 0.08$
IRAS 22134+58342 22 15 09.1 58 49 09 -18.3 2.6 1.2 1.6 ${\leq} 0.06$ ${\leq} 0.08$
IRAS 23139+59392 23 16 09.3 59 55 23 -44.7 4.8 0.9 1.5 ${\leq} 0.16$ ${\leq} 0.3$
IRAS 23151+59122 23 17 21.0 59 28 49 -54.4 5.7 ${\leq} 0.08$ ${\leq} 0.5$ ${\leq} 0.13$ ${\leq} 0.36$
IRAS 23545+65082 23 57 05.2 65 25 11 -18.4 0.8 ${\leq} 0.07$ ${\leq} 0.8$ ${\leq} 0.15$ ${\leq} 0.42$

1 $V_{\rm LSR}$ and $d_{\rm kin}$ from NH3 observations (Molinari et al. 1996). 2 $V_{\rm LSR}$ and $d_{\rm kin}$ from NH3 observations (Sridharan et al. 2002).


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