Decoding the cosmological baryonic fluctuations using localized fast radio bursts

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Table 1.

Basic observational data of the FRB samples with SFR_100 Myr values and uncertainties.

FRB	z_FRB	DM	SFR ^a	PS1 ^b	SCOS ^c	Reference ^b
		(pc cm⁻³)	(M_⊙/yr)
20190102C	0.291	364.4	$0 . 40_{- 0.11}^{+ 0.31}$ $0.40^{+0.31}_{-0.11}$	n	y	(1)(2)(3)(8)
20190523A	0.66	761	$0 . 09_{- 0.03}^{+ 0.03}$ $0.09^{+0.03}_{-0.03}$	y	n	(3)(4)(5)
20190608B	0.1178	339.5	$7 . 03_{- 1.15}^{+ 1.43}$ $7.03^{+1.43}_{-1.15}$	y	y	(1)(2)(5)(8)
20190714A	0.2365	504.1	$1 . 89_{- 0.72}^{+ 1.22}$ $1.89^{+1.22}_{-0.72}$	y	y	(3)(6)(8)
20191001A	0.234	507.9	$18 . 28_{- 8.95}^{+ 17.24}$ $18.28^{+17.24}_{-8.95}$	n	y	(3)(6)(7)(8)
20200430A	0.1608	380	$0 . 11_{- 0.04}^{+ 0.06}$ $0.11^{+0.06}_{-0.04}$	y	y	(3)(6)(8)
20200906A	0.3688	577.8	$4 . 93_{- 2.34}^{+ 3.46}$ $4.93^{+3.46}_{-2.34}$	y	n	(5)(8)
20210320C	0.2797	384.8	$3 . 51_{- 1.45}^{+ 2.44}$ $3.51^{+2.44}_{-1.45}$	y	y	(8)(9)(8)
20210603A	0.1772	500.147	$0 . 24_{- 0.06}^{+ 0.06}$ $0.24^{+0.06}_{-0.06}$	y	y	(10)
20211127I	0.0469	227	$35 . 83_{- 1.46}^{+ 1.02}$ $35.83^{+1.02}_{-1.46}$	n	y	(8)(11)
20211212A	0.0707	209	$0 . 73_{- 0.39}^{+ 0.62}$ $0.73^{+0.62}_{-0.39}$	y	y	(8)
20220105A	0.2785	580	$0 . 42_{- 0.19}^{+ 0.31}$ $0.42^{+0.31}_{-0.19}$	y	y	(8)
20220310F	0.477958	462.24	$4 . 25_{- 1.67}^{+ 2.45}$ $4.25^{+2.45}_{-1.67}$	y	n	(13)
20220418A	0.622	623.25	$29 . 41_{- 10.70}^{+ 18.28}$ $29.41^{+18.28}_{-10.70}$	y	n	(13)
20220914A	0.1139	631.28	$0 . 72_{- 0.15}^{+ 0.02}$ $0.72^{+0.02}_{-0.15}$	y	y	(13)(14)
20220920A	0.158239	314.99	$4 . 10_{- 1.00}^{+ 1.09}$ $4.10^{+1.09}_{-1.00}$	y	y	(13)
20221012A	0.284669	441.08	$0 . 15_{- 0.03}^{+ 0.04}$ $0.15^{+0.04}_{-0.03}$	y	y	(13)

Notes.

The star formation rate of the FRB host galaxy.

The columns (y = yes and n = no) show whether the FRB sample was used in the WISE × PS1 (PS1) or WISE × SCOS (SCOS).

References: (1) Macquart et al. (2020), (2) Day et al. (2020), (3) Cordes et al. (2022), (4) Ravi et al. (2019), (5) Bhandari et al. (2022), (6) Heintz et al. (2020), (7) Bhandari et al. (2020), (8) Gordon et al. (2023), (9) Sammons et al. (2023), (10) Cassanelli et al. (2024), (11) Glowacki et al. (2023), (12) Bhandari et al. (2020), (13) Law et al. (2024), (14) Connor et al. (2023).

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