2022ApJ...931...88C


Query : 2022ApJ...931...88C

2022ApJ...931...88C - Astrophys. J., 931, 88-88 (2022/June-1)

Redshift Estimation and Constraints on Intergalactic and Interstellar Media from Dispersion and Scattering of Fast Radio Bursts.

CORDES J.M., OCKER S.K. and CHATTERJEE S.

Abstract (from CDS):

A sample of 14 FRBs with measured redshifts and scattering times is used to assess contributions to dispersion and scattering from the intergalactic medium (IGM), galaxy halos, and the disks of host galaxies. The IGM and galaxy halos contribute significantly to dispersion measures (DMs) but evidently not to scattering, which is then dominated by host galaxies. This enables the usage of scattering times for estimating DM contributions from host galaxies and also for a combined scattering-dispersion redshift estimator. Redshift estimation is calibrated using the scattering of Galactic pulsars after taking into account different scattering geometries for Galactic and intergalactic lines of sight. The DM-only estimator has a bias of ∼0.1 and rms error of ∼0.15 in the redshift estimate for an assumed ad hoc value of 50 pc cm–3 for the host galaxy's DM contribution. The combined redshift estimator shows less bias by a factor of 4 to 10 and a 20%-40% smaller rms error. We find that values for the baryonic fraction of the ionized IGM figm ≃ 0.85 ± 0.05 optimize redshift estimation using dispersion and scattering. Our study suggests that 2 of the 14 candidate galaxy associations (FRB 20190523A and FRB 20190611B) should be reconsidered.

Abstract Copyright: © 2022. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Radio pulsars - Radio transient sources - Radio bursts - Intergalactic medium - Interstellar scattering - Interstellar medium - Baryon density - Interstellar plasma

Simbad objects: 32

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Number of rows : 32
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 SDSS J015800.28+654253.0 G 01 58 00.28512 +65 42 53.0964           ~ 17 0
2 FRB 20180916B rB 01 58 00.750 +65 43 00.30           ~ 457 0
3 FRB 20191221A rB 02 57 21.600 +79 43 12.00           ~ 34 0
4 NAME Magellanic Clouds GrG 03 00 -71.0           ~ 7988 0
5 FRB 20201124A rB 05 07 57.600 +26 11 24.00           ~ 307 0
6 NAME FRB 20201124A Host Galaxy G 05 08 03.49512 +26 03 37.9008           ~ 24 0
7 FRB 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
8 NAME FRB 121102 host galaxy G 05 31 58.698 +33 08 52.60           ~ 35 0
9 NAME Gal Anticenter reg 05 46 +28.9           ~ 1024 0
10 M 81 Sy2 09 55 33.1726556496 +69 03 55.062505368   7.89 6.94     ~ 4725 3
11 FRB 20200120E rB 09 57 56.7 +68 49 32           ~ 219 0
12 NAME FRB 190714 host galaxy G 12 15 55.00 -13 01 16.0           ~ 7 0
13 FRB 190714 rB 12 15 55.1 -13 01 16           ~ 64 0
14 PSO J207.0643+72.4708 G 13 48 15.4 +72 28 15           ~ 6 0
15 FRB 190523 rB 13 48 15.6 +72 28 11           ~ 109 0
16 NAME FRB 200430 host galaxy G 15 18 49.53 +12 22 35.8           ~ 7 0
17 FRB 200430 rB 15 18 49.54 +12 22 36.8           ~ 59 0
18 FRB 20190520B rB 16 02 04.270 -11 17 17.32           ~ 211 0
19 FRB 190611 rB 21 22 58.91 -79 23 51.3           ~ 82 0
20 NAME FRB 190611 host galaxy G 21 22 58.91 -79 23 51.3           ~ 7 0
21 NAME FRB 190102 host galaxy G 21 29 39.58 -79 28 32.5           ~ 10 0
22 FRB 190102 rB 21 29 39.76 -79 28 32.5           ~ 83 0
23 FRB 191001 rB 21 33 24.373 -54 44 51.40           ~ 64 0
24 NAME FRB 191001 host galaxy G 21 33 24.444240 -54 44 54.65400           ~ 11 0
25 FRB 180924 rB 21 44 25.255 -40 54 00.10           ~ 140 0
26 NAME FRB 180924 host galaxy G 21 44 25.29 -40 54 01.1           ~ 16 0
27 FRB 181112 rB 21 49 23.630 -52 58 15.39           ~ 131 0
28 DES J214923.66-525815.2 G 21 49 23.660 -52 58 15.28         21.51 ~ 9 0
29 NAME FRB 190711 host galaxy G 21 57 40.6 -80 21 29           ~ 5 0
30 FRB 20190711A rB 21 57 40.7 -80 21 29           ~ 114 0
31 FRB 190608 rB 22 16 04.74 -07 53 53.6           ~ 102 0
32 NAME FRB 190608 host galaxy Sy1 22 16 04.8973879488 -07 53 55.925178972   18.22 17.79     ~ 18 0

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