Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe

Research output: Contribution to journal › Journal article › Research › peer-review

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Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe. / Bhandari, Shivani; Heintz, Kasper E.; Aggarwal, Kshitij; Marnoch, Lachlan; Day, Cherie K.; Sydnor, Jessica; Burke-Spolaor, Sarah; Law, Casey J.; Prochaska, J. Xavier; Tejos, Nicolas; Bannister, Keith W.; Butler, Bryan J.; Deller, Adam T.; Ekers, R. D.; Flynn, Chris; Fong, Wen-fai; James, Clancy W.; Lazio, T. Joseph W.; Luo, Rui; Mahony, Elizabeth K.; Ryder, Stuart D.; Sadler, Elaine M.; Shannon, Ryan M.; Han, Jinlin; Lee, Kejia; Zhang, Bing.

In: Astronomical Journal, Vol. 163, No. 2, 69, 01.02.2022.

Research output: Contribution to journal › Journal article › Research › peer-review

Harvard

Bhandari, S, Heintz, KE, Aggarwal, K, Marnoch, L, Day, CK, Sydnor, J, Burke-Spolaor, S, Law, CJ, Prochaska, JX, Tejos, N, Bannister, KW, Butler, BJ, Deller, AT, Ekers, RD, Flynn, C, Fong, W, James, CW, Lazio, TJW, Luo, R, Mahony, EK, Ryder, SD, Sadler, EM, Shannon, RM, Han, J, Lee, K & Zhang, B 2022, 'Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe', Astronomical Journal, vol. 163, no. 2, 69. https://doi.org/10.3847/1538-3881/ac3aec

APA

Bhandari, S., Heintz, K. E., Aggarwal, K., Marnoch, L., Day, C. K., Sydnor, J., Burke-Spolaor, S., Law, C. J., Prochaska, J. X., Tejos, N., Bannister, K. W., Butler, B. J., Deller, A. T., Ekers, R. D., Flynn, C., Fong, W., James, C. W., Lazio, T. J. W., Luo, R., ... Zhang, B. (2022). Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe. Astronomical Journal, 163(2), [69]. https://doi.org/10.3847/1538-3881/ac3aec

Vancouver

Bhandari S, Heintz KE, Aggarwal K, Marnoch L, Day CK, Sydnor J et al. Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe. Astronomical Journal. 2022 Feb 1;163(2). 69. https://doi.org/10.3847/1538-3881/ac3aec

Author

Bhandari, Shivani ; Heintz, Kasper E. ; Aggarwal, Kshitij ; Marnoch, Lachlan ; Day, Cherie K. ; Sydnor, Jessica ; Burke-Spolaor, Sarah ; Law, Casey J. ; Prochaska, J. Xavier ; Tejos, Nicolas ; Bannister, Keith W. ; Butler, Bryan J. ; Deller, Adam T. ; Ekers, R. D. ; Flynn, Chris ; Fong, Wen-fai ; James, Clancy W. ; Lazio, T. Joseph W. ; Luo, Rui ; Mahony, Elizabeth K. ; Ryder, Stuart D. ; Sadler, Elaine M. ; Shannon, Ryan M. ; Han, Jinlin ; Lee, Kejia ; Zhang, Bing. / Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe. In: Astronomical Journal. 2022 ; Vol. 163, No. 2.

Bibtex

@article{601829e435864c8ca9162b5eda1b012f,
title = "Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe",
abstract = "We present the localization and host galaxies of one repeating and two apparently nonrepeating fast radio bursts (FRBs). FRB 20180301A was detected and localized with the Karl G. Jansky Very Large Array to a star-forming galaxy at z = 0.3304. FRB20191228A and FRB20200906A were detected and localized by the Australian Square Kilometre Array Pathfinder to host galaxies at z = 0.2430 and z = 0.3688, respectively. We combine these with 13 other well-localized FRBs in the literature, and analyze the host galaxy properties. We find no significant differences in the host properties of repeating and apparently nonrepeating FRBs. FRB hosts are moderately star forming, with masses slightly offset from the star-forming main sequence. Star formation and low-ionization nuclear emission-line region emission are major sources of ionization in FRB host galaxies, with the former dominant in repeating FRB hosts. FRB hosts do not track stellar mass and star formation as seen in field galaxies (more than 95% confidence). FRBs are rare in massive red galaxies, suggesting that progenitor formation channels are not solely dominated by delayed channels which lag star formation by gigayears. The global properties of FRB hosts are indistinguishable from core-collapse supernovae and short gamma-ray bursts hosts, and the spatial offset (from galaxy centers) of FRBs is mostly inconsistent with that of the Galactic neutron star population (95% confidence). The spatial offsets of FRBs (normalized to the galaxy effective radius) also differ from those of globular clusters in late- and early-type galaxies with 95% confidence.",
keywords = "GLOBULAR-CLUSTER SYSTEM, STAR-FORMATION, ENVIRONMENT, STELLAR, MASS, DWARF",
author = "Shivani Bhandari and Heintz, {Kasper E.} and Kshitij Aggarwal and Lachlan Marnoch and Day, {Cherie K.} and Jessica Sydnor and Sarah Burke-Spolaor and Law, {Casey J.} and Prochaska, {J. Xavier} and Nicolas Tejos and Bannister, {Keith W.} and Butler, {Bryan J.} and Deller, {Adam T.} and Ekers, {R. D.} and Chris Flynn and Wen-fai Fong and James, {Clancy W.} and Lazio, {T. Joseph W.} and Rui Luo and Mahony, {Elizabeth K.} and Ryder, {Stuart D.} and Sadler, {Elaine M.} and Shannon, {Ryan M.} and Jinlin Han and Kejia Lee and Bing Zhang",
year = "2022",
month = feb,
day = "1",
doi = "10.3847/1538-3881/ac3aec",
language = "English",
volume = "163",
journal = "The Astronomical Journal",
issn = "0004-6256",
publisher = "Institute of Physics Publishing, Inc",
number = "2",

}

RIS

TY - JOUR

T1 - Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe

AU - Bhandari, Shivani

AU - Heintz, Kasper E.

AU - Aggarwal, Kshitij

AU - Marnoch, Lachlan

AU - Day, Cherie K.

AU - Sydnor, Jessica

AU - Burke-Spolaor, Sarah

AU - Law, Casey J.

AU - Prochaska, J. Xavier

AU - Tejos, Nicolas

AU - Bannister, Keith W.

AU - Butler, Bryan J.

AU - Deller, Adam T.

AU - Ekers, R. D.

AU - Flynn, Chris

AU - Fong, Wen-fai

AU - James, Clancy W.

AU - Lazio, T. Joseph W.

AU - Luo, Rui

AU - Mahony, Elizabeth K.

AU - Ryder, Stuart D.

AU - Sadler, Elaine M.

AU - Shannon, Ryan M.

AU - Han, Jinlin

AU - Lee, Kejia

AU - Zhang, Bing

PY - 2022/2/1

Y1 - 2022/2/1

N2 - We present the localization and host galaxies of one repeating and two apparently nonrepeating fast radio bursts (FRBs). FRB 20180301A was detected and localized with the Karl G. Jansky Very Large Array to a star-forming galaxy at z = 0.3304. FRB20191228A and FRB20200906A were detected and localized by the Australian Square Kilometre Array Pathfinder to host galaxies at z = 0.2430 and z = 0.3688, respectively. We combine these with 13 other well-localized FRBs in the literature, and analyze the host galaxy properties. We find no significant differences in the host properties of repeating and apparently nonrepeating FRBs. FRB hosts are moderately star forming, with masses slightly offset from the star-forming main sequence. Star formation and low-ionization nuclear emission-line region emission are major sources of ionization in FRB host galaxies, with the former dominant in repeating FRB hosts. FRB hosts do not track stellar mass and star formation as seen in field galaxies (more than 95% confidence). FRBs are rare in massive red galaxies, suggesting that progenitor formation channels are not solely dominated by delayed channels which lag star formation by gigayears. The global properties of FRB hosts are indistinguishable from core-collapse supernovae and short gamma-ray bursts hosts, and the spatial offset (from galaxy centers) of FRBs is mostly inconsistent with that of the Galactic neutron star population (95% confidence). The spatial offsets of FRBs (normalized to the galaxy effective radius) also differ from those of globular clusters in late- and early-type galaxies with 95% confidence.

AB - We present the localization and host galaxies of one repeating and two apparently nonrepeating fast radio bursts (FRBs). FRB 20180301A was detected and localized with the Karl G. Jansky Very Large Array to a star-forming galaxy at z = 0.3304. FRB20191228A and FRB20200906A were detected and localized by the Australian Square Kilometre Array Pathfinder to host galaxies at z = 0.2430 and z = 0.3688, respectively. We combine these with 13 other well-localized FRBs in the literature, and analyze the host galaxy properties. We find no significant differences in the host properties of repeating and apparently nonrepeating FRBs. FRB hosts are moderately star forming, with masses slightly offset from the star-forming main sequence. Star formation and low-ionization nuclear emission-line region emission are major sources of ionization in FRB host galaxies, with the former dominant in repeating FRB hosts. FRB hosts do not track stellar mass and star formation as seen in field galaxies (more than 95% confidence). FRBs are rare in massive red galaxies, suggesting that progenitor formation channels are not solely dominated by delayed channels which lag star formation by gigayears. The global properties of FRB hosts are indistinguishable from core-collapse supernovae and short gamma-ray bursts hosts, and the spatial offset (from galaxy centers) of FRBs is mostly inconsistent with that of the Galactic neutron star population (95% confidence). The spatial offsets of FRBs (normalized to the galaxy effective radius) also differ from those of globular clusters in late- and early-type galaxies with 95% confidence.

KW - GLOBULAR-CLUSTER SYSTEM

KW - STAR-FORMATION

KW - ENVIRONMENT

KW - STELLAR

KW - MASS

KW - DWARF

U2 - 10.3847/1538-3881/ac3aec

DO - 10.3847/1538-3881/ac3aec

M3 - Journal article

VL - 163

JO - The Astronomical Journal

JF - The Astronomical Journal

SN - 0004-6256

IS - 2

M1 - 69

ER -

ID: 302383295