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Table 11

Main observational parameters for SGR (top) and FRB (bottom) ToOs at the SRT.

Source Date νobs BW Δν tsampl Backend tobs S
(GHz) (MHz) (MHz) (μs) (s) (mJy)

SGR J1745-2900 20130506 7.3 680 680 40000 TP 7200 0.1
SGR J1935+2154 20140731 6.4 412 1 6338 DFB 5598 <0.08
20140807 0.35 105 0.25 3169 DFB 1800 ...
SGR J1819-1600 20151126 1.55 500 2 250 DFB 8424 <0.07
20151126 6.5 924 2 500 DFB 7835 <0.04
20151206 1.55 500 4 250 DFB 5500 <0.08
20151206 6.6 924 2 650 DFB 5500 <0.05
SGR J0755-2933 20160319 6.6 924 2 250 DFB 3766 <0.06

Source Date ν obs BW Δν t sampl Backend t obs S
(GHz) (MHz) (MHz) (μs) (s) (Jy)

FRB150418 20150421 1.55 500 2 125 DFB 3534 <0.54 × (W/ 3.5)-0.5
20150421 0.35 105 0.25 128 ROACH1 4363 ...
FRB151206 20151207 1.5 500 1 500 DFB 12177 <0.31 × (W/ 2.7)-0.5
20151207 1.5 500 1 500 SARDARA 10126 ...
20160506 1.5 500 1 250 DFB 10480 <0.31 × (W/ 2.7)-0.5
20160506 0.35 105 0.25 256 ROACH1 10480 ...
FRB121102 20160309 6.6 924 2 250 DFB 19792 <0.07 × (W/ 2.8)-0.5
FRB151230 20160510 1.55 500 1 250 DFB 10350 <0.24 × (W/ 4.6)-0.5
FRB160102 20160507 1.55 500 1 250 DFB 7200 <0.28 × (W/ 3.3)-0.5
FRB160102 20160507 0.35 105 1 256 ROACH1 7200 ...

Notes.

(†)

For L-band observations the flux density was estimated by multiplying the nominal Tsys by two to roughly take into account the adverse RFI environment. Observations at P band were too badly affected by RFI and a reliable flux density estimate could not be obtained. For FRB flux density estimates we explicitly indicate the dependance on the pulse duration W, normalized over the actual width of the observed pulse (expressed in ms).

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