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Table 1

List of observed pulsars, their observing parameters, and the values derived from the observations.

PSR P DM Date of t obs t samp S m int
(s) (cm-3  pc) observation (min) [μs] (mJy)

B0329+54 0.7145 26.833 05.12.2002 28 697.6 1.11 ± 0.22
11.06.2004 72 697.6 2.87 ± 0.57

1.99 ± 0.40 0.88 ± 0.06

B0355+54 0.1563 57.142 26.04.2004 9 152.6 2.17 ± 0.43

B0450+55 0.3407 14.495 05.12.2002 8 332.6 0.45 ± 0.09

B0809+74 1.2922 6.116 05.12.2002 90 1261.8 0.64 ± 0.13 1.24

B0823+26 0.5306 19.454 05.12.2002 20 518.0 0.87 ± 0.17
05.12.2002 13 518.0 0.71 ± 0.14
26.04.2004 53 518.0 0.99 ± 0.20

0.86 ± 0.17 1.1 ± 0.1

B0950+08 0.2530 2.958 26.04.2004 30 247.0 1.09 ± 0.22 1.29

B1133+16 1.1879 4.864 05.12.2002 10 1159.8 0.92 ± 0.18
05.12.2002 90 1159.8 0.88 ± 0.18
26.04.2004 120 60.0 0.73 ± 0.15
11.06.2004 47 60.0 0.79 ± 0.16

0.78 ± 0.16 2.11 ± 0.14

B2016+28 0.5579 14.172 11.06.2004 55 544.8 0.66 ± 0.13 1.15

B2020+28 0.3434 24.640 11.06.2004 35 335.2 1.09 ± 0.22 0.69

B2021+51 0.5291 22.648 05.12.2002 18 516.6 1.73 ± 0.35 0.75

B2154+40 1.5252 70.857 11.06.2004 11 1489.2 0.13 ± 0.03

B2310+42 0.3494 17.276 11.06.2004 9 341.2 0.17 ± 0.03

Notes.The first three columns list the pulsar name, its period, and the dispersion measure, respectively. Columns 4−6 hold the date of observation, its duration, and the sampling time. The last two columns present the flux density measurements of integrated pulse profiles and modulation indices intrinsic to the pulsar, respectively. When there was more than one measurement of the flux density and modulation index, we present the average value and its uncertainty.

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