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Table 1

Past surveys dedicated to the periodicity (PS) and single-pulse (SPS) pulsar searches in nearby galaxies.

Galaxy d Telescope Fcntr Δν Tsamp Tint Smin [PS] Speak [SPS] Reference
(Mpc) (MHz) (MHz) (μs) (hrs) (Jy) (Jy)

M 33 0.84 Arecibo 430 10 102.4 3.0 0.2 × 10-3 0.5 1
1440 100 64 (100) 2.0 (3.0) 5.3 × 10-6 0.1 2
NGC 253, NGC 300, Fornax 3.0, 2.0, 16.9 Parkes 435 32 420 3.0 (...) 0.09 1
NGC 6300, NGC 7793 16.9, 3.5
Leo I (dSph galaxy) 0.25 GBT 350 100 81.92 20.0 ~2.0 × 10-4 ~0.04 3
IC 10 0.66 820 200 204.8 16.0 1.5 × 10-5 0.02 4
Willman 1, Boo dw, UMi dw 0.046, 0.062, 0.075 GBT (Arecibo) 820 (327) 50 (50) 81.92 (128) 3.3, 4.4, 5.3 (...) 0.5 (1.54), 0.3 (1), 1.6 (5), each × 103 5
Dra dw, Scl dw, Sex dw 0.078, 0.093, 0.099 3.6, 2.8, 3.25 2.3 (7), 2.3 (7.1), 2.3 (7.1), each × 103
CVn I, Leo I-II, UMa II 0.23, 0.28, 0.23, 0.25 6.2, 21.9, 10.9, 2.0 4 (12), 6 (19), 4 (12), 19 (57), each × 103
And II, III, VI, XI-XIV 0.9 1.4, 1.1, 2.5, 3.9, 3.7, 3.0, 2.0 64 (198), each × 103
Leo T, Leo A 0.4, 0.78 4.2, 6.1 13 (40), 44 (136), each × 103
IC 1613, LGS 3, Peg dw 0.9, 0.93, 0.93 3.5, 3.9, 2.5 63 (195), 67 (207), 67 (207), each × 103
M 31 0.8 WSRT 328 10 409.6 32.0 0.3 × 10-3 2.8 6

Notes. Tabulated are: galaxy, its distance, the telescope, central frequency, bandwidth in MHz, sampling time in μs, total dwell time in hours, and the obtained average (for PS), and peak (for SPS) flux densities in Jy.

Reference. (1) McLaughlin & Cordes (2003); (2) Bhat et al. (2011); (3) Rubio-Herrera & Maccarone (2013); (4) Noori et al. (2014); (5) Kondratiev et al. (2013) and Kondratiev (priv. comm.); (6) Rubio-Herrera et al. (2013).

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