2025ApJS..280....6C

Query : 2025ApJS..280....6C

2025ApJS..280....6C - Astrophys. J., Suppl. Ser., 280, 6 (2025/September-0)

A Catalog of Local Universe Fast Radio Bursts from CHIME/FRB and the KKO.

CHIME/FRB COLLABORATION, AMIRI M., AMOUYAL D., ANDERSEN B.C., ANDREW S., BANDURA K., BHARDWAJ M., BOYLE P.J., BRAR C., CASSITY A., CHATTERJEE S., CURTIN A.P., DOBBS M., DONG F.A., DONG Y., EADIE G.M., EFTEKHARI T., FONG W.-F., FONSECA E., GAENSLER B.M., HALPERN M., HESSELS J.W.T., HOPKINS H., IBIK A.L., JOSEPH R.C., KACZMAREK J., KAHINGA L., KASPI V., KHAIRY K., KILPATRICK C.D., LANMAN A.E., LAZDA M., LEUNG C., MAIN R., MAS-RIBAS L., MASUI K.W., MCKINVEN R., MENA-PARRA J., MEYERS B.W., MICHILLI D., MILUTINOVIC N., NIMMO K., NOBLE G., PANDHI A., PATIL S.S., PEARLMAN A.B., PETROFF E., PLEUNIS Z., PROCHASKA J.X., RAFIEI-RAVANDI M., RAHMAN M., RENARD A., SAMMONS M.W., SAND K.R., SCHOLZ P., SHAH V., SHIN K., SIEGEL S.R., SIMHA S., SMITH K., STAIRS I., VANDERLINDE K., WANG H., WULF D. and ZEGMOTT T.J.

Abstract (from CDS):

We present the first catalog of fast radio burst (FRB) host galaxies from CHIME/FRB Outriggers, selected uniformly in the radio and the optical by localizing 81 new bursts to 2″ × ∼ 60″ accuracy using CHIME and the k'niʔatn k'l ⌣ stk'masqt Outrigger station, located 66 km from CHIME. Of the 81 localized bursts, we use the probabilistic association of transients to their hosts algorithm to securely identify 21 new FRB host galaxies, and compile spectroscopic redshifts for 19 systems, 15 of which are newly obtained via spectroscopic observations. The most nearby source is FRB 20231229A, at a distance of 90 Mpc. One burst in our sample is from a previously reported repeating source in a galaxy merger (FRB 20190303A). Three new FRB host galaxies (FRBs 20230203A, 20230703A, and 20231206A) are found toward X-ray and optically selected galaxy clusters, potentially doubling the sample of known galaxy cluster FRBs. A search for radio counterparts reveals that FRB 20231128A is associated with a luminous persistent radio source (PRS) candidate with high significance (Pcc ∼ 10–2). If its compactness is confirmed, it would be the nearest known compact PRS at z = 0.1079. Our catalog significantly increases the statistics of the Macquart relation at low redshifts (z < 0.2). In the near future, the completed CHIME/FRB Outriggers array will produce hundreds of FRBs localized with very long baseline interferometry (VLBI). This will significantly expand the known sample and pave the way for future telescopes relying on VLBI for FRB localization.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Radio transient sources

Simbad objects: 44

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Number of rows : 44
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 FRB 20231011A G 01 12 57.86 +41 44 56.8           ~ 8 0
2 Z 521-78 GiG 01 45 51.8097960912 +35 06 39.190328820   14.8   14.27   ~ 38 0
3 FRB 20231229A G 01 45 52.28 +35 06 46.5           ~ 8 0
4 FRB 20180916B rB 01 58 00.750 +65 43 00.30           ~ 457 0
5 FRB 20231201A G 03 38 21.43 +26 49 03.6           ~ 7 0
6 FRB 20230730A G 03 38 39.49 +33 09 33.5           ~ 7 0
7 FRB 20231202A rB 04 20 07.29 +38 37 59.8           ~ 1 0
8 FRB 20231020A rB 04 43 48.698 +71 56 27.51           ~ 1 0
9 FRB 20231025C rB 04 47 54.54 +33 14 16.8           ~ 1 0
10 FRB 20231230A G 04 51 11.43 +02 23 38.3           ~ 8 0
11 FRB 20201124A rB 05 07 57.600 +26 11 24.00           ~ 307 0
12 FRB 20231123A G 05 30 29.58 +04 28 31.9           ~ 8 0
13 FRB 20181119D rB 05 31 58.6980 +33 08 52.588           ~ 933 0
14 M 1 SNR 05 34 31.8 +22 01 03           ~ 6516 1
15 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
16 FRB 20230311A G 06 04 26.32 +55 56 45.4           ~ 7 0
17 FRB 20230222A G 07 07 50.49 +11 13 28.3           ~ 8 0
18 ACO 576 ClG 07 21 24.1 +55 44 20           ~ 312 1
19 FRB 20231206A G 07 29 46.28 +56 15 22.6           ~ 7 0
20 PSR B0919+06 Psr 09 22 13.85000 +06 38 19.0000           ~ 329 1
21 FRB 20200120E rB 09 57 56.7 +68 49 32           ~ 219 0
22 FRB 20230203A G 10 06 38.78 +35 41 38.8           ~ 8 0
23 NSC J100649+353929 ClG 10 06 49.29 +35 39 28.5           ~ 2 0
24 FRB 20230703A G 12 18 29.87 +48 43 47.7           ~ 7 0
25 NSCS J121847+484410 ClG 12 18 47.00 +48 44 09.2           ~ 1 0
26 FRB 20231128A G 13 18 18.77 +42 59 33.8           ~ 7 0
27 ILT J131819.22+425958.9 Rad 13 18 19.22 +42 59 58.9           ~ 3 0
28 FRB 20191106C rB 13 18 +43.0           ~ 22 0
29 M 3 GlC 13 42 11.62 +28 22 38.2     6.39     ~ 2593 0
30 FRB 20190303A G 13 51 59.77 +48 06 57.6           ~ 58 0
31 FRB 20230410A rB 14 19 08.389 +25 27 26.26           ~ 1 0
32 FRB 20230222B G 15 54 57.39 +30 53 55.3           ~ 8 0
33 FRB 20190520B rB 16 02 04.270 -11 17 17.32           ~ 211 0
34 FRB 20231005A G 16 24 06.72 +35 26 55.4           ~ 8 0
35 PSR B1642-03 Psr 16 45 02.0330 -03 17 57.200           ~ 394 0
36 FRB 20231223C G 17 18 10.72 +29 29 52.6           ~ 8 0
37 ILT J175629.78+414836.4 Rad 17 56 29.78 +41 48 36.5           ~ 1 0
38 FRB 20230926A G 17 56 29.97 +41 48 51.5           ~ 8 0
39 FRB 20231025B G 18 03 09.14 +63 59 20.7           ~ 7 0
40 FRB 20240209A rB 19 19 33.0 +86 03 52           ~ 21 0
41 NAME Sgr 1935+2154 * 19 34 55.68 +21 53 48.2           ~ 820 1
42 FRB 20231007B rB 20 30 07.61 +72 53 32.5           ~ 1 0
43 FRB 20231017A G 23 07 01.03 +36 39 09.6           ~ 7 0
44 FRB 20220912A rB 23 09 04.9 +48 42 25           ~ 126 0

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