No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution
We investigate whether the sky rate of fast radio bursts (FRBs) depends on Galactic latitude using the first catalog of FRBs detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project. We first select CHIME/FRB events above a specified sensitivity threshold i...
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| Veröffentlicht in: | The Astrophysical journal 2021-12, Vol.923 (1), p.2 |
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| creator | Josephy, A. Chawla, P. Curtin, A. P. Kaspi, V. M. Bhardwaj, M. Boyle, P. J. Brar, C. Cassanelli, T. Fonseca, E. Gaensler, B. M. Leung, C. Lin, H.-H. Masui, K. W. Mckinven, R. Mena-Parra, J. Michilli, D. Ng, C. Pleunis, Z. Rafiei-Ravandi, M. Rahman, M. Sanghavi, P. Scholz, P. Shin, K. Smith, K. M. Stairs, I. H. Tendulkar, S. P. Zwaniga, A. V. |
| description | We investigate whether the sky rate of fast radio bursts (FRBs) depends on Galactic latitude using the first catalog of FRBs detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project. We first select CHIME/FRB events above a specified sensitivity threshold in consideration of the radiometer equation, and then we compare these detections with the expected cumulative time-weighted exposure using Anderson–Darling and Kolmogorov–Smirnov tests. These tests are consistent with the null hypothesis that FRBs are distributed without Galactic latitude dependence (
p
-values distributed from 0.05 to 0.99, depending on completeness threshold). Additionally, we compare rates in intermediate latitudes (∣
b
∣ < 15°) with high latitudes using a Bayesian framework, treating the question as a biased coin-flipping experiment–again for a range of completeness thresholds. In these tests the isotropic model is significantly favored (Bayes factors ranging from 3.3 to 14.2). Our results are consistent with FRBs originating from an isotropic population of extragalactic sources. |
| doi_str_mv | 10.3847/1538-4357/ac33ad |
| format | Article |
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p
-values distributed from 0.05 to 0.99, depending on completeness threshold). Additionally, we compare rates in intermediate latitudes (∣
b
∣ < 15°) with high latitudes using a Bayesian framework, treating the question as a biased coin-flipping experiment–again for a range of completeness thresholds. In these tests the isotropic model is significantly favored (Bayes factors ranging from 3.3 to 14.2). Our results are consistent with FRBs originating from an isotropic population of extragalactic sources.</description><identifier>ISSN: 0004-637X</identifier><identifier>EISSN: 1538-4357</identifier><identifier>DOI: 10.3847/1538-4357/ac33ad</identifier><language>eng</language><publisher>Philadelphia: The American Astronomical Society</publisher><subject>Astrophysics ; Completeness ; High energy astrophysics ; Hydrogen ; Latitude ; Radio bursts ; Radio transient sources</subject><ispartof>The Astrophysical journal, 2021-12, Vol.923 (1), p.2</ispartof><rights>2021. The Author(s). Published by the American Astronomical Society.</rights><rights>Copyright IOP Publishing Dec 01, 2021</rights><lds50>peer_reviewed</lds50><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed><citedby>FETCH-LOGICAL-c378t-c1e3c80896bdf3a4f33c1ada01ae474003b3cc50b4e9ce8ee196f1644ba86a713</citedby><cites>FETCH-LOGICAL-c378t-c1e3c80896bdf3a4f33c1ada01ae474003b3cc50b4e9ce8ee196f1644ba86a713</cites><orcidid>0000-0001-7453-4273 ; 0000-0001-8278-1936 ; 0000-0001-8384-5049 ; 0000-0002-3382-9558 ; 0000-0002-4209-7408 ; 0000-0001-5504-229X ; 0000-0001-8537-9299 ; 0000-0003-3059-6223 ; 0000-0002-7374-7119 ; 0000-0001-7348-6900 ; 0000-0002-2551-7554 ; 0000-0001-9784-8670 ; 0000-0002-6823-2073 ; 0000-0002-2088-3125 ; 0000-0001-7694-6650 ; 0000-0002-3615-3514 ; 0000-0002-4279-6946 ; 0000-0003-1842-6096 ; 0000-0003-2047-5276 ; 0000-0003-2548-2926 ; 0000-0001-9345-0307 ; 0000-0002-4795-697X ; 0000-0002-3426-7606 ; 0000-0002-8376-1563 ; 0000-0002-3616-5160 ; 0000-0002-1800-8233 ; 0000-0002-0772-9326</orcidid></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><linktopdf>$$Uhttps://iopscience.iop.org/article/10.3847/1538-4357/ac33ad/pdf$$EPDF$$P50$$Giop$$Hfree_for_read</linktopdf><link.rule.ids>314,776,780,27901,27902,38867,53842</link.rule.ids></links><search><creatorcontrib>Josephy, A.</creatorcontrib><creatorcontrib>Chawla, P.</creatorcontrib><creatorcontrib>Curtin, A. P.</creatorcontrib><creatorcontrib>Kaspi, V. M.</creatorcontrib><creatorcontrib>Bhardwaj, M.</creatorcontrib><creatorcontrib>Boyle, P. J.</creatorcontrib><creatorcontrib>Brar, C.</creatorcontrib><creatorcontrib>Cassanelli, T.</creatorcontrib><creatorcontrib>Fonseca, E.</creatorcontrib><creatorcontrib>Gaensler, B. M.</creatorcontrib><creatorcontrib>Leung, C.</creatorcontrib><creatorcontrib>Lin, H.-H.</creatorcontrib><creatorcontrib>Masui, K. W.</creatorcontrib><creatorcontrib>Mckinven, R.</creatorcontrib><creatorcontrib>Mena-Parra, J.</creatorcontrib><creatorcontrib>Michilli, D.</creatorcontrib><creatorcontrib>Ng, C.</creatorcontrib><creatorcontrib>Pleunis, Z.</creatorcontrib><creatorcontrib>Rafiei-Ravandi, M.</creatorcontrib><creatorcontrib>Rahman, M.</creatorcontrib><creatorcontrib>Sanghavi, P.</creatorcontrib><creatorcontrib>Scholz, P.</creatorcontrib><creatorcontrib>Shin, K.</creatorcontrib><creatorcontrib>Smith, K. M.</creatorcontrib><creatorcontrib>Stairs, I. H.</creatorcontrib><creatorcontrib>Tendulkar, S. P.</creatorcontrib><creatorcontrib>Zwaniga, A. V.</creatorcontrib><title>No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution</title><title>The Astrophysical journal</title><addtitle>APJ</addtitle><addtitle>Astrophys. J</addtitle><description>We investigate whether the sky rate of fast radio bursts (FRBs) depends on Galactic latitude using the first catalog of FRBs detected by the Canadian Hydrogen Intensity Mapping Experiment Fast Radio Burst (CHIME/FRB) Project. We first select CHIME/FRB events above a specified sensitivity threshold in consideration of the radiometer equation, and then we compare these detections with the expected cumulative time-weighted exposure using Anderson–Darling and Kolmogorov–Smirnov tests. These tests are consistent with the null hypothesis that FRBs are distributed without Galactic latitude dependence (
p
-values distributed from 0.05 to 0.99, depending on completeness threshold). Additionally, we compare rates in intermediate latitudes (∣
b
∣ < 15°) with high latitudes using a Bayesian framework, treating the question as a biased coin-flipping experiment–again for a range of completeness thresholds. In these tests the isotropic model is significantly favored (Bayes factors ranging from 3.3 to 14.2). Our results are consistent with FRBs originating from an isotropic population of extragalactic sources.</description><subject>Astrophysics</subject><subject>Completeness</subject><subject>High energy astrophysics</subject><subject>Hydrogen</subject><subject>Latitude</subject><subject>Radio bursts</subject><subject>Radio transient sources</subject><issn>0004-637X</issn><issn>1538-4357</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2021</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><recordid>eNp9kM9LwzAUx4MoOKd3j4FdrUv6sjY96tymMBTUgbfwmqaYOZuapsL-e1sqehFP7wef7_fxvoScc3YJUqRTPgMZCZilU9QAWByQ0c_qkIwYYyJKIH05JidNs-3HOMtGZHPv6OLTFqbShpbO0xXuUAer6RqDDW1h6I2pTTUArqTh1dAlNoE-YmEdvW591z-97emNbYK3eRusq07JUYm7xpx91zHZLBfP89to_bC6m1-tIw2pDJHmBrRkMkvyogQUJYDmWCDjaEQqGIMctJ6xXJhMG2kMz5KSJ0LkKBNMOYzJZPCtvftoTRPU1rW-6k6qOGEpgJRx1lFsoLR3TeNNqWpv39HvFWeqD0_1Sak-KTWE10kuBol19a_nP_jkDxzrrcpiUFzFqu4e_ALd-3zJ</recordid><startdate>20211201</startdate><enddate>20211201</enddate><creator>Josephy, A.</creator><creator>Chawla, P.</creator><creator>Curtin, A. 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P. ; Kaspi, V. M. ; Bhardwaj, M. ; Boyle, P. J. ; Brar, C. ; Cassanelli, T. ; Fonseca, E. ; Gaensler, B. M. ; Leung, C. ; Lin, H.-H. ; Masui, K. W. ; Mckinven, R. ; Mena-Parra, J. ; Michilli, D. ; Ng, C. ; Pleunis, Z. ; Rafiei-Ravandi, M. ; Rahman, M. ; Sanghavi, P. ; Scholz, P. ; Shin, K. ; Smith, K. M. ; Stairs, I. H. ; Tendulkar, S. P. ; Zwaniga, A. 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p
-values distributed from 0.05 to 0.99, depending on completeness threshold). Additionally, we compare rates in intermediate latitudes (∣
b
∣ < 15°) with high latitudes using a Bayesian framework, treating the question as a biased coin-flipping experiment–again for a range of completeness thresholds. In these tests the isotropic model is significantly favored (Bayes factors ranging from 3.3 to 14.2). Our results are consistent with FRBs originating from an isotropic population of extragalactic sources.</abstract><cop>Philadelphia</cop><pub>The American Astronomical Society</pub><doi>10.3847/1538-4357/ac33ad</doi><tpages>9</tpages><orcidid>https://orcid.org/0000-0001-7453-4273</orcidid><orcidid>https://orcid.org/0000-0001-8278-1936</orcidid><orcidid>https://orcid.org/0000-0001-8384-5049</orcidid><orcidid>https://orcid.org/0000-0002-3382-9558</orcidid><orcidid>https://orcid.org/0000-0002-4209-7408</orcidid><orcidid>https://orcid.org/0000-0001-5504-229X</orcidid><orcidid>https://orcid.org/0000-0001-8537-9299</orcidid><orcidid>https://orcid.org/0000-0003-3059-6223</orcidid><orcidid>https://orcid.org/0000-0002-7374-7119</orcidid><orcidid>https://orcid.org/0000-0001-7348-6900</orcidid><orcidid>https://orcid.org/0000-0002-2551-7554</orcidid><orcidid>https://orcid.org/0000-0001-9784-8670</orcidid><orcidid>https://orcid.org/0000-0002-6823-2073</orcidid><orcidid>https://orcid.org/0000-0002-2088-3125</orcidid><orcidid>https://orcid.org/0000-0001-7694-6650</orcidid><orcidid>https://orcid.org/0000-0002-3615-3514</orcidid><orcidid>https://orcid.org/0000-0002-4279-6946</orcidid><orcidid>https://orcid.org/0000-0003-1842-6096</orcidid><orcidid>https://orcid.org/0000-0003-2047-5276</orcidid><orcidid>https://orcid.org/0000-0003-2548-2926</orcidid><orcidid>https://orcid.org/0000-0001-9345-0307</orcidid><orcidid>https://orcid.org/0000-0002-4795-697X</orcidid><orcidid>https://orcid.org/0000-0002-3426-7606</orcidid><orcidid>https://orcid.org/0000-0002-8376-1563</orcidid><orcidid>https://orcid.org/0000-0002-3616-5160</orcidid><orcidid>https://orcid.org/0000-0002-1800-8233</orcidid><orcidid>https://orcid.org/0000-0002-0772-9326</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
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| ispartof | The Astrophysical journal, 2021-12, Vol.923 (1), p.2 |
| issn | 0004-637X 1538-4357 |
| language | eng |
| recordid | cdi_iop_journals_10_3847_1538_4357_ac33ad |
| source | IOP Publishing Free Content; EZB-FREE-00999 freely available EZB journals; Alma/SFX Local Collection |
| subjects | Astrophysics Completeness High energy astrophysics Hydrogen Latitude Radio bursts Radio transient sources |
| title | No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution |
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