Deep Synoptic Array Science: Discovery of the Host Galaxy of FRB 20220912A
We report the detection and interferometric localization of the repeating fast radio burst (FRB) source FRB 20220912A during commissioning observations with the Deep Synoptic Array (DSA-110). Two bursts were detected from FRB 20220912A, one each on 2022 October 18 and 2022 October 25. The best-fit p...
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| Veröffentlicht in: | Astrophysical journal. Letters 2023-05, Vol.949 (1), p.L3 |
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| creator | Ravi, Vikram Catha, Morgan Chen, Ge Connor, Liam Faber, Jakob T. Lamb, James W. Hallinan, Gregg Harnach, Charlie Hellbourg, Greg Hobbs, Rick Hodge, David Hodges, Mark Law, Casey Rasmussen, Paul Sharma, Kritti Sherman, Myles B. Shi, Jun Simard, Dana Squillace, Reynier Weinreb, Sander Woody, David P. Yadlapalli, Nitika Ahumada, Tomas Dong, Dillon Fremling, Christoffer Huang, Yuping Karambelkar, Viraj Miller, Jessie M. |
| description | We report the detection and interferometric localization of the repeating fast radio burst (FRB) source FRB 20220912A during commissioning observations with the Deep Synoptic Array (DSA-110). Two bursts were detected from FRB 20220912A, one each on 2022 October 18 and 2022 October 25. The best-fit position is (R.A. J2000, decl. J2000) = (23:09:04.9, +48:42:25.4), with a 90% confidence error ellipse with radii ±2″ and ±1″ in R.A. and decl., respectively. The two bursts are polarized, and we find a Faraday rotation measure that is consistent with the low value of +0.6 rad m
−2
reported by CHIME/FRB. The DSA-110 localization overlaps with the galaxy PSO J347.2702+48.7066 at a redshift
z
= 0.0771, which we identify as the likely host. PSO J347.2702+48.7066 has a stellar mass of approximately 10
10
M
⊙
, modest internal dust extinction, and a star formation rate likely in excess of 0.1
M
⊙
yr
−1
. The host-galaxy contribution to the dispersion measure is likely ≲50 pc cm
−3
. The FRB 20220912A source is therefore likely viewed along a tenuous plasma column through the host galaxy. |
| doi_str_mv | 10.3847/2041-8213/acc4b6 |
| format | Article |
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−2
reported by CHIME/FRB. The DSA-110 localization overlaps with the galaxy PSO J347.2702+48.7066 at a redshift
z
= 0.0771, which we identify as the likely host. PSO J347.2702+48.7066 has a stellar mass of approximately 10
10
M
⊙
, modest internal dust extinction, and a star formation rate likely in excess of 0.1
M
⊙
yr
−1
. The host-galaxy contribution to the dispersion measure is likely ≲50 pc cm
−3
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−2
reported by CHIME/FRB. The DSA-110 localization overlaps with the galaxy PSO J347.2702+48.7066 at a redshift
z
= 0.0771, which we identify as the likely host. PSO J347.2702+48.7066 has a stellar mass of approximately 10
10
M
⊙
, modest internal dust extinction, and a star formation rate likely in excess of 0.1
M
⊙
yr
−1
. The host-galaxy contribution to the dispersion measure is likely ≲50 pc cm
−3
. The FRB 20220912A source is therefore likely viewed along a tenuous plasma column through the host galaxy.</description><subject>Arrays</subject><subject>Compact objects</subject><subject>Faraday effect</subject><subject>Galaxies</subject><subject>Localization</subject><subject>Radio bursts</subject><subject>Radio interferometry</subject><subject>Radio telescopes</subject><subject>Radio transient sources</subject><subject>Red shift</subject><subject>Star & galaxy formation</subject><subject>Star formation</subject><subject>Star formation rate</subject><subject>Stellar mass</subject><issn>2041-8205</issn><issn>2041-8213</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2023</creationdate><recordtype>article</recordtype><sourceid>O3W</sourceid><sourceid>DOA</sourceid><recordid>eNp1kM9LwzAcxYsoOKd3jwHxZl1-N_E2N7cpA8HtHtI00Za51LQT-9_brjIvevqGx_t-vi8vii4RvCWCJiMMKYoFRmSkjaEpP4oGB-n48IbsNDqrqgJCDDkSg-hpam0JVs3Wl3VuwDgE3YCVye3W2DswzSvjP21ogHegfrNg4asazPVGf-2l2cs9wBBjKBEen0cnTm8qe_Ezh9F69rCeLOLl8_xxMl7GhlJex0lKBNFOJCTNmCAcO8SMkTohMuHcCmhsItPM4ZQZSwxlBmaEOaYzJDGxZBg99tjM60KVIX_XoVFe52ov-PCqdGj_srGKES5gRjXXyNAEupQLY9u0jkmkU-da1lXPKoP_2NmqVoXfhW2bXmGBqGRYMNa6YO8ywVdVsO5wFUHVla-6dlXXtOrLb1eu-5Xcl79MXRYbJalUSC2JKrMuwM0fvn-x34Plj1w</recordid><startdate>20230501</startdate><enddate>20230501</enddate><creator>Ravi, Vikram</creator><creator>Catha, Morgan</creator><creator>Chen, Ge</creator><creator>Connor, Liam</creator><creator>Faber, Jakob T.</creator><creator>Lamb, James W.</creator><creator>Hallinan, Gregg</creator><creator>Harnach, Charlie</creator><creator>Hellbourg, Greg</creator><creator>Hobbs, Rick</creator><creator>Hodge, David</creator><creator>Hodges, Mark</creator><creator>Law, Casey</creator><creator>Rasmussen, Paul</creator><creator>Sharma, Kritti</creator><creator>Sherman, Myles B.</creator><creator>Shi, Jun</creator><creator>Simard, Dana</creator><creator>Squillace, Reynier</creator><creator>Weinreb, Sander</creator><creator>Woody, David P.</creator><creator>Yadlapalli, Nitika</creator><creator>Ahumada, Tomas</creator><creator>Dong, Dillon</creator><creator>Fremling, Christoffer</creator><creator>Huang, Yuping</creator><creator>Karambelkar, Viraj</creator><creator>Miller, Jessie M.</creator><general>The American Astronomical Society</general><general>IOP Publishing</general><scope>O3W</scope><scope>TSCCA</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>8FD</scope><scope>H8D</scope><scope>KL.</scope><scope>L7M</scope><scope>DOA</scope><orcidid>https://orcid.org/0000-0003-2758-159X</orcidid><orcidid>https://orcid.org/0000-0002-7587-6352</orcidid><orcidid>https://orcid.org/0000-0002-4477-3625</orcidid><orcidid>https://orcid.org/0000-0002-5959-1285</orcidid><orcidid>https://orcid.org/0000-0001-8840-922X</orcidid><orcidid>https://orcid.org/0000-0002-7252-5485</orcidid><orcidid>https://orcid.org/0000-0002-4119-9963</orcidid><orcidid>https://orcid.org/0000-0002-8873-8784</orcidid><orcidid>https://orcid.org/0000-0001-6748-5290</orcidid><orcidid>https://orcid.org/0000-0003-4267-6108</orcidid><orcidid>https://orcid.org/0000-0003-3255-4617</orcidid><orcidid>https://orcid.org/0000-0001-9584-2531</orcidid><orcidid>https://orcid.org/0000-0002-4223-103X</orcidid><orcidid>https://orcid.org/0000-0003-1647-7762</orcidid><orcidid>https://orcid.org/0000-0003-2867-4544</orcidid><orcidid>https://orcid.org/0000-0002-6573-7316</orcidid><orcidid>https://orcid.org/0000-0002-7083-4049</orcidid></search><sort><creationdate>20230501</creationdate><title>Deep Synoptic Array Science: Discovery of the Host Galaxy of FRB 20220912A</title><author>Ravi, Vikram ; Catha, Morgan ; Chen, Ge ; Connor, Liam ; Faber, Jakob T. ; Lamb, James W. ; Hallinan, Gregg ; Harnach, Charlie ; Hellbourg, Greg ; Hobbs, Rick ; Hodge, David ; Hodges, Mark ; Law, Casey ; Rasmussen, Paul ; Sharma, Kritti ; Sherman, Myles B. ; Shi, Jun ; Simard, Dana ; Squillace, Reynier ; Weinreb, Sander ; Woody, David P. ; Yadlapalli, Nitika ; Ahumada, Tomas ; Dong, Dillon ; Fremling, Christoffer ; Huang, Yuping ; Karambelkar, Viraj ; Miller, Jessie M.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c446t-7b383af873bd58362f15cc9a739766e80ce79bdf2b5ce3c45c0d35f5ad1923e3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2023</creationdate><topic>Arrays</topic><topic>Compact objects</topic><topic>Faraday effect</topic><topic>Galaxies</topic><topic>Localization</topic><topic>Radio bursts</topic><topic>Radio interferometry</topic><topic>Radio telescopes</topic><topic>Radio transient sources</topic><topic>Red shift</topic><topic>Star & galaxy formation</topic><topic>Star formation</topic><topic>Star formation rate</topic><topic>Stellar mass</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Ravi, Vikram</creatorcontrib><creatorcontrib>Catha, Morgan</creatorcontrib><creatorcontrib>Chen, Ge</creatorcontrib><creatorcontrib>Connor, Liam</creatorcontrib><creatorcontrib>Faber, Jakob T.</creatorcontrib><creatorcontrib>Lamb, James W.</creatorcontrib><creatorcontrib>Hallinan, Gregg</creatorcontrib><creatorcontrib>Harnach, Charlie</creatorcontrib><creatorcontrib>Hellbourg, Greg</creatorcontrib><creatorcontrib>Hobbs, Rick</creatorcontrib><creatorcontrib>Hodge, David</creatorcontrib><creatorcontrib>Hodges, Mark</creatorcontrib><creatorcontrib>Law, Casey</creatorcontrib><creatorcontrib>Rasmussen, Paul</creatorcontrib><creatorcontrib>Sharma, Kritti</creatorcontrib><creatorcontrib>Sherman, Myles B.</creatorcontrib><creatorcontrib>Shi, Jun</creatorcontrib><creatorcontrib>Simard, Dana</creatorcontrib><creatorcontrib>Squillace, Reynier</creatorcontrib><creatorcontrib>Weinreb, Sander</creatorcontrib><creatorcontrib>Woody, David P.</creatorcontrib><creatorcontrib>Yadlapalli, Nitika</creatorcontrib><creatorcontrib>Ahumada, Tomas</creatorcontrib><creatorcontrib>Dong, Dillon</creatorcontrib><creatorcontrib>Fremling, Christoffer</creatorcontrib><creatorcontrib>Huang, Yuping</creatorcontrib><creatorcontrib>Karambelkar, Viraj</creatorcontrib><creatorcontrib>Miller, Jessie M.</creatorcontrib><creatorcontrib>The Deep Synoptic Array team</creatorcontrib><collection>IOP Publishing Free Content</collection><collection>IOPscience (Open Access)</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Advanced Technologies Database with Aerospace</collection><collection>DOAJ Directory of Open Access Journals</collection><jtitle>Astrophysical journal. 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Letters</jtitle><stitle>APJL</stitle><addtitle>Astrophys. J. Lett</addtitle><date>2023-05-01</date><risdate>2023</risdate><volume>949</volume><issue>1</issue><spage>L3</spage><pages>L3-</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>We report the detection and interferometric localization of the repeating fast radio burst (FRB) source FRB 20220912A during commissioning observations with the Deep Synoptic Array (DSA-110). Two bursts were detected from FRB 20220912A, one each on 2022 October 18 and 2022 October 25. The best-fit position is (R.A. J2000, decl. J2000) = (23:09:04.9, +48:42:25.4), with a 90% confidence error ellipse with radii ±2″ and ±1″ in R.A. and decl., respectively. The two bursts are polarized, and we find a Faraday rotation measure that is consistent with the low value of +0.6 rad m
−2
reported by CHIME/FRB. The DSA-110 localization overlaps with the galaxy PSO J347.2702+48.7066 at a redshift
z
= 0.0771, which we identify as the likely host. PSO J347.2702+48.7066 has a stellar mass of approximately 10
10
M
⊙
, modest internal dust extinction, and a star formation rate likely in excess of 0.1
M
⊙
yr
−1
. The host-galaxy contribution to the dispersion measure is likely ≲50 pc cm
−3
. The FRB 20220912A source is therefore likely viewed along a tenuous plasma column through the host galaxy.</abstract><cop>Austin</cop><pub>The American Astronomical Society</pub><doi>10.3847/2041-8213/acc4b6</doi><tpages>8</tpages><orcidid>https://orcid.org/0000-0003-2758-159X</orcidid><orcidid>https://orcid.org/0000-0002-7587-6352</orcidid><orcidid>https://orcid.org/0000-0002-4477-3625</orcidid><orcidid>https://orcid.org/0000-0002-5959-1285</orcidid><orcidid>https://orcid.org/0000-0001-8840-922X</orcidid><orcidid>https://orcid.org/0000-0002-7252-5485</orcidid><orcidid>https://orcid.org/0000-0002-4119-9963</orcidid><orcidid>https://orcid.org/0000-0002-8873-8784</orcidid><orcidid>https://orcid.org/0000-0001-6748-5290</orcidid><orcidid>https://orcid.org/0000-0003-4267-6108</orcidid><orcidid>https://orcid.org/0000-0003-3255-4617</orcidid><orcidid>https://orcid.org/0000-0001-9584-2531</orcidid><orcidid>https://orcid.org/0000-0002-4223-103X</orcidid><orcidid>https://orcid.org/0000-0003-1647-7762</orcidid><orcidid>https://orcid.org/0000-0003-2867-4544</orcidid><orcidid>https://orcid.org/0000-0002-6573-7316</orcidid><orcidid>https://orcid.org/0000-0002-7083-4049</orcidid><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
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| ispartof | Astrophysical journal. Letters, 2023-05, Vol.949 (1), p.L3 |
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| source | IOP Publishing Free Content; DOAJ Directory of Open Access Journals; Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; IOPscience extra; Alma/SFX Local Collection |
| subjects | Arrays Compact objects Faraday effect Galaxies Localization Radio bursts Radio interferometry Radio telescopes Radio transient sources Red shift Star & galaxy formation Star formation Star formation rate Stellar mass |
| title | Deep Synoptic Array Science: Discovery of the Host Galaxy of FRB 20220912A |
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