Table 1 Observational set-up

From: A link between repeating and non-repeating fast radio bursts through their energy distributions

Station

Band

Frequency (MHz)

Bandwidtha (MHz)

Bandwidth per sub-band (MHz)

SEFDb (Jy)

Completenessc (Jy ms)

Time observed (h)

Wb

P

300–364

60

8

2100

91

649.51

Wb

LWb-1

1,259–1,387

100

16

420

14

383.1

Wb

LWb-2

1,382–1,510

100

16

420

14

129.5

St

LSt

1,332.5–1,430.5

98

98

1,100/385

39/14

1,431.7

O8

LO8-1

1,360–1,488

100

16

310

10

415.7

O8

LO8-2

1,460–1,588

100

16

310

10

85.7

O8

LO8-3

1,360–1,616

200

16

310

7

9.8

O8

LO8-4

1,202–1,714

350

32

310

5

40.9

Tr

LTr-1

1,290–1,546

200

32

350

8

116.9

Tr

LTr-2

1,340–1,596

200

32

350

8

22.4

Tr

LTr-3

1,350–1,478

100

16

350

12

15.6

Tr

CTr-1

4,550–4,806

240

32

220

5

227.7

Tr

CTr-2

4,600–4,728

120

32

220

7

16.4

Total telescope time/total time on source (h)d

3,545/2,281

  1. aEffective bandwidth accounting for RFI and band edges.
  2. bFrom the EVN status page (with the exception of St, for which the two values indicate the pre- and post-upgrade sensitivity).
  3. cAssuming a 15σ detection threshold and a pulse width of 1 ms.
  4. dTotal time on source accounts for the overlap between the participating stations.
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