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Table 4

Velocity and flux density of the peak of the MERLIN integrated spectra and the Pushchino spectra taken closest in time.

Source Date VLSR Peak Itot
Telescope (YYMMDD) (km s-1) (Jy) (Jy km s-1)

VX Sgr
Pushchino 940329 13.1 548 2696
MERLIN 940426 13.0 360 26611

Pushchino 981110 6.3 352 3208
MERLIN 990116 6.3 147 1521
Pushchino 990119 6.4 321 3027

S Per
Pushchino 930303 –37.83 22.9 232
MERLIN 940324 –37.86 63.6 222
Pushchino 940329 –37.50 51.9 188

Pushchino 981228 –37.72 69.3 311
MERLIN 990110 –37.75 45.2 286
Pushchino 930303 –37.74 63.5 371

U Ori
Pushchino 940328 –37.3 33.0 30
MERLIN 940417 –37.3 25.4 23
Pushchino 940517 –37.3 28.6 26

Pushchino 981230 –37.8 105.0 84
MERLIN 990109 –38.0 58.7 46
Pushchino 990121 –37.8 85.8 74

Pushchino 000223 –37.8 29.3 42
MERLIN 000410 –38.0 18.7 18
Pushchino 000613 –37.9 28.1 16

Pushchino 010410 –37.8 25.3 31
MERLIN 010506 –37.9 16.6 19
Pushchino 010530 –37.8 39.2 31

U Her 1994
Pushchino 940329 –14.9 21.7 30
MERLIN 940413 –15.0 22.1 44
Pushchino 940517 –14.9 32.1 56

Pushchino 000425 –15.6 186.3 406
MERLIN 000519 –15.5 209.1 254
Pushchino 000529 –15.6 182.3 267

Pushchino 010411 –15.8 93.5 118
MERLIN 010427 –15.6 52.5 62
Pushchino 010528 –15.7 73.2 96

IK Tau 1994
Pushchino 930422 31.8 34.9 89
MERLIN 940415 31.4 24.3 48
Pushchino 941109 31.7 24.7 222

Pushchino 000425 24.9 106.4 279
MERLIN 000520 24.4 117.5 360
Pushchino 000530 24.6 113.0 414

Pushchino 010409 24.2 13.4 66
MERLIN 010427 24.4 22.6 107
Pushchino 010529 24.4 23.8 118

RT Vir
Pushchino 940328 12.6 489.4 943
MERLIN 940416 12.6 394.0 590
Pushchino 940808 12.6 186.0 797

Pushchino 960319 11.9 791.0 1605
MERLIN 960405 11.8 389.0 680
MERLIN 960421 11.5 515.5 1190
MERLIN 960429 11.5 526.3 1325
MERLIN 960515 11.4 727.2 1475
MERLIN 960524 11.4 705.5 1415
MERLIN 960612 11.3 791.6 1418
Pushchino 960619 11.3 359.9 648

Notes. The integrated flux density of the whole spectrum is also given. In some cases a shift Vcorr was applied to the Pushchino data, see Figs. 32 to 41. Table continued.

(1)

Measured over the same velocity range as the Pushchino data.

(2)

The Pushchino data only cover part of the spectrum.

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