Table 2: "FIR-maser'' observations.
Sourcea RA Dec $V_{\rm sys}$ $S_{100~\mu \rm m}^{b}$ V-range rms Channel Epochc
              width  
  (J2000) (J2000) (cz) (Jy) (km s-1 (mJy) (km s-1)  
IC 10 d 00 20 27.0 $\:~$59 17 29 -350 71        
NGC 253 d 00 47 33.1 -25 17 18 240 1045        
NGC 660 01 43 01.6 $\:~$13 38 35 850 104 620, 1100 7 1.1 0601
          0, 1780 10 4.2 0302
NGC 891 02 22 33.4 $\:~$42 20 57 525 148 320, 900 20 1.1 0601
NGC 972 02 34 12.9 $\:~$29 18 48 1540 65 700, 2470 9 4.3 0302
          860, 2080 20 1.1 0302
NGC 1055 02 41 45.4 $\:~$00 26 35 1000 60 800, 1250 17 1.1 1203
          450, 1600 17 1.1 0404
Maffei 2 02 41 55.1 $\:~$59 36 11 -35 227 -250, 210 12 1.1 0601
          -250, 200 15 1.1 0302
NGC 1068 d 02 42 40.7 -00 00 48 1135 240        
NGC 1084 02 46 00.0 -07 34 37 1405 55 930, 1940 20 1.1 0103
IC 342 d 03 46 48.6 $\:~$68 05 46 40 128 -190, 300 12 1.1 0601
          -150, 300 9 1.1 0302
UGC 02855 03 48 22.6 $\:~$70 07 57 1200 79 980, 1460 9 1.1 0601
NGC 1569 04 30 46.8 $\:~$64 51 02 100 52 -100, 190 12 1.1 0601
NGC 2146 d 06 18 39.6 $\:~$78 21 19 900 187 500, 1190 7 1.1 0302
NGC 2403 07 37 37.6 $\:~$71 19 32 130 56 -100, 400 9 1.1 0601
NGC 2559 08 17 06.0 -27 27 27 1560 66 1080, 2090 20 1.1 0103
NGC 2903 09 32 10.1 $\:~$21 30 04 550 104 100, 1100 7 4.2 0701
NGC 3034 d 09 55 52.2 $\:~$69 40 47 200 1145        
NGC 3079 d 10 01 57.8 $\:~$55 40 47 1120 89        
NGC 3521 11 05 48.6 -00 02 09 850 85 320, 1340 29 1.1 0302
NGC 3556 d 11 11 31.2 $\:~$55 40 25 700 61 see Table 3      
NGC 3627 11 20 15.0 $\:~$12 59 30 725 106 300, 1250 8 4.2 0701
NGC 3628 11 20 17.0 $\:~$13 35 20 842 103 400, 1380 7 4.2 0701
Arp 299 d 11 28 31.9 $\:~$58 33 45 3120 111 see Table 3      
NGC 4038 12 01 52.8 -18 51 54 1640 76 1020, 2300 28 1.1 0502
NGC 4088 12 05 34.2 $\:~$50 32 21 750 52 280, 1280 16 1.1 0302
NGC 4102 12 06 23.1 $\:~$52 42 39 850 69 600, 1100 17 1.1 0601
NGC 4254 12 18 49.5 $\:~$14 25 00 2400 72 2000, 2930 6 4.3 0701
NGC 4303 12 21 54.9 $\:~$04 28 25 1565 62 1080, 2100 13 1.1 0302
NGC 4321 12 22 54.9 $\:~$15 49 20 1570 58 1100, 2100 12 1.1 0302
NGC 4414 12 26 27.1 $\:~$31 13 24 700 68 230, 1250 17 1.1 0302
NGC 4490 12 30 36.1 $\:~$41 38 34 560 78 60, 1100 17 1.1 0302
NGC 4501 12 31 59.1 $\:~$14 25 14 2278 55 1800, 2800 10 1.1 0103
NGC 4527 12 34 08.5 $\:~$02 39 10 1735 64 1240, 2260 15 1.1 0302
NGC 4631 12 42 07.9 $\:~$32 32 26 600 120 200, 1100 7 4.2 0701
NGC 4666 12 45 08.7 -00 27 41 1500 77 1050, 2050 10 1.1 0103
NGC 4736 12 50 53.0 $\:~$41 07 13 300 105 -150, 820 5 4.2 0701
NGC 4826 12 56 43.7 $\:~$21 40 52 400 76 -80, 940 11 1.1 0103
NGC 5005 13 10 56.3 $\:~$37 03 33 950 59 450 1470 13 1.1 0302
NGC 5055 13 15 49.3 $\:~$42 01 49 500 101 30, 1030 12 1.1 0302
NGC 5194 d 13 29 52.7 $\:~$47 11 42 450 123        
NGC 5236 13 37 00.7 -29 51 58 500 213 50, 1050 34 1.1 0302
Arp 220 15 34 57.1 $\:~$23 30 11 5430 118 5220, 5700 10 1.1 0601
NGC 6000 15 49 49.6 -29 23 11 2200 59 1970, 2400 25 1.1 0601
NGC 6946 20 34 52.4 $\:~$60 09 14 50 128 -170, 300 11 1.1 0601
NGC 7331 22 37 04.0 $\:~$34 24 56 820 82 600, 1070 14 1.1 0601
          330, 1070 12 1.1 0302
a Source names in italics: previously detected sources; bold-faced: newly detected sources.
b Flux densities are taken from the IRAS Point Source Catalog (Fullmer & Lonsdale 1989).
c Month (first two digits) and year (last two digits).
d IC 10: see Henkel et al. (1986); NGC 253: Ho et al. (1987); NGC 1068: Claussen et al. (1984); IC 342: Tarchi et al. (2002a) and Sect. 3.5; NGC 2146: Tarchi et al. (2002b) and Sect. 3.5; NGC 3034 (M 82): Claussen et al. (1984); NGC 3079: Henkel et al. (1984), Haschick & Baan (1985); NGC 3556 and Arp 299: this paper; NGC 5194 (M 51): Ho et al. (1987).

Source LaTeX | All tables | In the text

Article Contents
1 Introduction and sample selection
2 Observations
3 Results
4 Discussion
5 Conclusions
References
List of tables
List of figures