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Table 2.

Overview of the parameters adopted for the simulation of surveys.

Parameter Units askap-incoh chime-frb chord fast-crafts parkes-htru
β 1.2 1.2 1.2 1.2 1.2
G K Jy−1 0.09898 1.4 3.33 16.46 0.69
tpoint s 3600 360 360 60 270
tsamp ms 1.265 1 1 0.196608 0.064
Trec K 70 50 50 20 28
νc MHz 1320 600 900 1250 1352
BW MHz 336.0 400 1200 400 340
BWch MHz 1 0.390625 0.390625 0.076 0.390625
npol 2 2 2 2 2
FoV deg2 20 164.15 200 0.031 0.5551
S/N 8 10 8 8 8
ϕ ° −26.696 49.3208 49.3208 25.6529 −32.9980
λ ° 116.637 −119.624 −119.6238 106.8566 148.2626
Mount Azimuthal Transit Transit Transit Azimuthal
α ° 0–360 0–360 0–360 0–360 0–360
δ ° −90–30 −40.679–90 −40.679–90 −14–66 −90–90
l ° −180–180 −180–180 −180–180 −180–180 −120–30
b ° −90–90 −90–90 −90–90 −90–90 −15–15
Reference 1 2 3 4 5

Parameter Units perfect puma-full ska1-low ska1-mid wsrt-apertif

β 1.2 1.2 1.2 1.2 1.2
G K Jy−1 105 166.5 10.71 17.65 0.7
tpoint s 86400 600 600 600 10800
tsamp ms 0.001 1.25 0.05 0.05 0.04096
Trec K 0.01 30 30 30 70
νc MHz 1000 650 150 7175 1370
BW MHz 800 900 200 13650 300
BWch MHz 0.001 0.390625 0.0054 0.0134 0.1953
npol 2 2 2 2 2
FoV deg2 41253 32.6 27 0.49 8.7
S/N 10−16 8 8 8 10
ϕ ° 0 0 −26.7 −30.72 52.91474
λ ° 0 0 116.67 21.41 6.603340
Mount Azimuthal Azimuthal Transit Azimuthal Equatorial
α ° 0–360 0–360 0–360 0–360 0–360
δ ° −90–90 −90–90 −90–90 −90–90 −37.1–90
l ° −180–180 −180–180 −180–180 −180–180 −180–180
b ° −90–90 −90–90 −90–90 −90–90 −90–90
Reference 6 7 7 8

Notes. Parameters include survey degradation factor β, telescope gain G, pointing time tpoint, sampling time tsamp, receiver temperature Trec, central frequency νc, bandwidth BW, channel bandwidth BWch, number of polarisations npol, field of view (FoV), minimum S/N, observatory latitude ϕ, observatory longitude λ, mount type, and then the minimum to maximum right ascension α, declination δ, Galactic longitude l, and Galactic latitude b. Greyed-out values indicate an estimated or average value, or a value obtained through private communication. We note that many future surveys have parameters that are still subject to change.

References. (1) Shannon et al. (2018); (2) CHIME/FRB Collaboration (2018); (3) Vanderlinde et al. (2019); (4) Zhang et al. (2019); (5) Keith et al. (2010); (6) Castorina et al. (2020), Slosar et al. (2019); (7) Dewdney et al. (2013); (8) Oosterloo et al. (2009), Maan & van Leeuwen (2017).

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