Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope

Autores
Abdo, A. A.; Ackermann, M.; Ajello, M.; Baldini, L.; Ballet, J.; Barbiellini, G.; Bastieri, D.; Baughman, B. M.; Bechtol, K.; Bellazzini, R.; Berenji, B.; Blandford, R. D.; Bloom, E. D.; Bonamente, E.; Borgland, A. W.; Bregeon, J.; Brez, A.; Brigida, M.; Bruel, P.; Burnett, T. H.; Buson, S.; Caliandro, G. A.; Cameron, R. A.; Caraveo, P. A.; Casandjian, J. M.; Cecchi, C.; Celik, O.; Chekhtman, A.; Cheung, C. C.; Chiang, J.; Cillis, Analia Nilda; Fermi-LAT Collaboration
Año de publicación
2010
Idioma
inglés
Tipo de recurso
artículo
Estado
versión publicada
Descripción
We report observation of the supernova remnant (SNR) IC 443 (G189.1+3.0) with the Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 MeV and 50 GeV. IC 443 is a shell-type SNR with mixed morphology located off the outer Galactic plane where high-energy emission has been detected in the X-ray, GeV and TeV gamma-ray bands. Past observations suggest IC 443 has been interacting with surrounding interstellar matter. Proximity between dense shocked molecular clouds and GeV-TeV gamma-ray emission regions detected by EGRET, MAGIC, and VERITAS suggests an interpretation that cosmic-ray (CR) particles are accelerated by the SNR. With the high gamma-ray statistics and broad energy coverage provided by the LAT, we accurately characterize the gamma-ray emission produced by the CRs accelerated at IC 443. The emission region is extended in the energy band with θ68 = 0fdg27 ± 0fdg01(stat) ± 0fdg03(sys) for an assumed two-dimensional Gaussian profile and overlaps almost completely with the extended source region of VERITAS. Its centroid is displaced significantly from the known pulsar wind nebula (PWN) which suggests the PWN is not the major contributor in the present energy band. The observed spectrum changes its power-law slope continuously and continues smoothly to the MAGIC and VERITAS data points. The combined gamma-ray spectrum (200 MeV Fil: Abdo, A. A.. Spece Sciences División. Naval Research Laboratory; Estados Unidos. National Academy of Sciences; Estados Unidos
Fil: Ackermann, M.. University Of Stanford; Estados Unidos
Fil: Ajello, M.. University Of Stanford; Estados Unidos
Fil: Baldini, L.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Ballet, J.. Universite Paris Diderot; Francia
Fil: Barbiellini, G.. Universita di Trieste; Italia
Fil: Bastieri, D.. Universita Di Padova; Italia
Fil: Baughman, B. M.. Ohio State University; Estados Unidos
Fil: Bechtol, K.. University Of Stanford; Estados Unidos
Fil: Bellazzini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Berenji, B.. University Of Stanford; Estados Unidos
Fil: Blandford, R. D.. University Of Stanford; Estados Unidos
Fil: Bloom, E. D.. University Of Stanford; Estados Unidos
Fil: Bonamente, E.. Universita degli Studi di Perugia; Italia
Fil: Borgland, A. W.. University Of Stanford; Estados Unidos
Fil: Bregeon, J.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Brez, A.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Brigida, M.. Universita e del Politecnico di Bari; Italia
Fil: Bruel, P.. Ecole Polytechnique; Francia
Fil: Burnett, T. H.. University of Washington; Estados Unidos
Fil: Buson, S.. Universita Di Padova; Italia
Fil: Caliandro, G. A.. Universita e del Politecnico di Bari; Italia
Fil: Cameron, R. A.. University Of Stanford; Estados Unidos
Fil: Caraveo, P. A.. Istituto di Astrofisica Spaziale e Fisica Cosmica; Italia
Fil: Casandjian, J. M.. Université Paris Diderot - Paris 7; Francia
Fil: Cecchi, C.. Universita degli Studi di Perugia; Italia
Fil: Celik, O.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados Unidos
Fil: Chekhtman, A.. Space Science Division; Estados Unidos
Fil: Cheung, C. C.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados Unidos
Fil: Chiang, J.. University Of Stanford; Estados Unidos
Fil: Cillis, Analia Nilda. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Fermi-LAT Collaboration.
Materia
gamma rays
supernovae
IC443
Nivel de accesibilidad
acceso abierto
Condiciones de uso
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
Repositorio
CONICET Digital (CONICET)
Institución
Consejo Nacional de Investigaciones Científicas y Técnicas
OAI Identificador
oai:ri.conicet.gov.ar:11336/19154

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oai_identifier_str oai:ri.conicet.gov.ar:11336/19154
network_acronym_str CONICETDig
repository_id_str 3498
network_name_str CONICET Digital (CONICET)
spelling Observation of Supernova Remnant IC 443 with the Fermi Large Area TelescopeAbdo, A. A.Ackermann, M.Ajello, M.Baldini, L.Ballet, J.Barbiellini, G.Bastieri, D.Baughman, B. M.Bechtol, K.Bellazzini, R.Berenji, B.Blandford, R. D.Bloom, E. D.Bonamente, E.Borgland, A. W.Bregeon, J.Brez, A.Brigida, M.Bruel, P.Burnett, T. H.Buson, S.Caliandro, G. A.Cameron, R. A.Caraveo, P. A.Casandjian, J. M.Cecchi, C.Celik, O.Chekhtman, A.Cheung, C. C.Chiang, J.Cillis, Analia NildaFermi-LAT Collaborationgamma rayssupernovaeIC443https://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1We report observation of the supernova remnant (SNR) IC 443 (G189.1+3.0) with the Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 MeV and 50 GeV. IC 443 is a shell-type SNR with mixed morphology located off the outer Galactic plane where high-energy emission has been detected in the X-ray, GeV and TeV gamma-ray bands. Past observations suggest IC 443 has been interacting with surrounding interstellar matter. Proximity between dense shocked molecular clouds and GeV-TeV gamma-ray emission regions detected by EGRET, MAGIC, and VERITAS suggests an interpretation that cosmic-ray (CR) particles are accelerated by the SNR. With the high gamma-ray statistics and broad energy coverage provided by the LAT, we accurately characterize the gamma-ray emission produced by the CRs accelerated at IC 443. The emission region is extended in the energy band with θ68 = 0fdg27 ± 0fdg01(stat) ± 0fdg03(sys) for an assumed two-dimensional Gaussian profile and overlaps almost completely with the extended source region of VERITAS. Its centroid is displaced significantly from the known pulsar wind nebula (PWN) which suggests the PWN is not the major contributor in the present energy band. The observed spectrum changes its power-law slope continuously and continues smoothly to the MAGIC and VERITAS data points. The combined gamma-ray spectrum (200 MeV <E< 2 TeV) is reproduced well by decays of neutral pions produced by a broken power-law proton spectrum with a break around 70 GeV.Fil: Abdo, A. A.. Spece Sciences División. Naval Research Laboratory; Estados Unidos. National Academy of Sciences; Estados UnidosFil: Ackermann, M.. University Of Stanford; Estados UnidosFil: Ajello, M.. University Of Stanford; Estados UnidosFil: Baldini, L.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Ballet, J.. Universite Paris Diderot; FranciaFil: Barbiellini, G.. Universita di Trieste; ItaliaFil: Bastieri, D.. Universita Di Padova; ItaliaFil: Baughman, B. M.. Ohio State University; Estados UnidosFil: Bechtol, K.. University Of Stanford; Estados UnidosFil: Bellazzini, R.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Berenji, B.. University Of Stanford; Estados UnidosFil: Blandford, R. D.. University Of Stanford; Estados UnidosFil: Bloom, E. D.. University Of Stanford; Estados UnidosFil: Bonamente, E.. Universita degli Studi di Perugia; ItaliaFil: Borgland, A. W.. University Of Stanford; Estados UnidosFil: Bregeon, J.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Brez, A.. Istituto Nazionale di Fisica Nucleare; ItaliaFil: Brigida, M.. Universita e del Politecnico di Bari; ItaliaFil: Bruel, P.. Ecole Polytechnique; FranciaFil: Burnett, T. H.. University of Washington; Estados UnidosFil: Buson, S.. Universita Di Padova; ItaliaFil: Caliandro, G. A.. Universita e del Politecnico di Bari; ItaliaFil: Cameron, R. A.. University Of Stanford; Estados UnidosFil: Caraveo, P. A.. Istituto di Astrofisica Spaziale e Fisica Cosmica; ItaliaFil: Casandjian, J. M.. Université Paris Diderot - Paris 7; FranciaFil: Cecchi, C.. Universita degli Studi di Perugia; ItaliaFil: Celik, O.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados UnidosFil: Chekhtman, A.. Space Science Division; Estados UnidosFil: Cheung, C. C.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados UnidosFil: Chiang, J.. University Of Stanford; Estados UnidosFil: Cillis, Analia Nilda. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; ArgentinaFil: Fermi-LAT Collaboration.IOP Publishing2010-03-20info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/19154Abdo, A. A.; Ackermann, M.; Ajello, M.; Baldini, L.; Ballet, J.; et al.; Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope; IOP Publishing; Astrophysical Journal; 712; 1; 20-3-2010; 459-4680004-637XCONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/0004-637X/712/1/459/pdf/apj_712_1_459.pdfinfo:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1002.2198info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/712/1/459info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-sa/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2025-09-29T09:37:56Zoai:ri.conicet.gov.ar:11336/19154instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982025-09-29 09:37:56.348CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse
dc.title.none.fl_str_mv Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
title Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
spellingShingle Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
Abdo, A. A.
gamma rays
supernovae
IC443
title_short Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
title_full Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
title_fullStr Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
title_full_unstemmed Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
title_sort Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope
dc.creator.none.fl_str_mv Abdo, A. A.
Ackermann, M.
Ajello, M.
Baldini, L.
Ballet, J.
Barbiellini, G.
Bastieri, D.
Baughman, B. M.
Bechtol, K.
Bellazzini, R.
Berenji, B.
Blandford, R. D.
Bloom, E. D.
Bonamente, E.
Borgland, A. W.
Bregeon, J.
Brez, A.
Brigida, M.
Bruel, P.
Burnett, T. H.
Buson, S.
Caliandro, G. A.
Cameron, R. A.
Caraveo, P. A.
Casandjian, J. M.
Cecchi, C.
Celik, O.
Chekhtman, A.
Cheung, C. C.
Chiang, J.
Cillis, Analia Nilda
Fermi-LAT Collaboration
author Abdo, A. A.
author_facet Abdo, A. A.
Ackermann, M.
Ajello, M.
Baldini, L.
Ballet, J.
Barbiellini, G.
Bastieri, D.
Baughman, B. M.
Bechtol, K.
Bellazzini, R.
Berenji, B.
Blandford, R. D.
Bloom, E. D.
Bonamente, E.
Borgland, A. W.
Bregeon, J.
Brez, A.
Brigida, M.
Bruel, P.
Burnett, T. H.
Buson, S.
Caliandro, G. A.
Cameron, R. A.
Caraveo, P. A.
Casandjian, J. M.
Cecchi, C.
Celik, O.
Chekhtman, A.
Cheung, C. C.
Chiang, J.
Cillis, Analia Nilda
Fermi-LAT Collaboration
author_role author
author2 Ackermann, M.
Ajello, M.
Baldini, L.
Ballet, J.
Barbiellini, G.
Bastieri, D.
Baughman, B. M.
Bechtol, K.
Bellazzini, R.
Berenji, B.
Blandford, R. D.
Bloom, E. D.
Bonamente, E.
Borgland, A. W.
Bregeon, J.
Brez, A.
Brigida, M.
Bruel, P.
Burnett, T. H.
Buson, S.
Caliandro, G. A.
Cameron, R. A.
Caraveo, P. A.
Casandjian, J. M.
Cecchi, C.
Celik, O.
Chekhtman, A.
Cheung, C. C.
Chiang, J.
Cillis, Analia Nilda
Fermi-LAT Collaboration
author2_role author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
author
dc.subject.none.fl_str_mv gamma rays
supernovae
IC443
topic gamma rays
supernovae
IC443
purl_subject.fl_str_mv https://purl.org/becyt/ford/1.3
https://purl.org/becyt/ford/1
dc.description.none.fl_txt_mv We report observation of the supernova remnant (SNR) IC 443 (G189.1+3.0) with the Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 MeV and 50 GeV. IC 443 is a shell-type SNR with mixed morphology located off the outer Galactic plane where high-energy emission has been detected in the X-ray, GeV and TeV gamma-ray bands. Past observations suggest IC 443 has been interacting with surrounding interstellar matter. Proximity between dense shocked molecular clouds and GeV-TeV gamma-ray emission regions detected by EGRET, MAGIC, and VERITAS suggests an interpretation that cosmic-ray (CR) particles are accelerated by the SNR. With the high gamma-ray statistics and broad energy coverage provided by the LAT, we accurately characterize the gamma-ray emission produced by the CRs accelerated at IC 443. The emission region is extended in the energy band with θ68 = 0fdg27 ± 0fdg01(stat) ± 0fdg03(sys) for an assumed two-dimensional Gaussian profile and overlaps almost completely with the extended source region of VERITAS. Its centroid is displaced significantly from the known pulsar wind nebula (PWN) which suggests the PWN is not the major contributor in the present energy band. The observed spectrum changes its power-law slope continuously and continues smoothly to the MAGIC and VERITAS data points. The combined gamma-ray spectrum (200 MeV <E< 2 TeV) is reproduced well by decays of neutral pions produced by a broken power-law proton spectrum with a break around 70 GeV.
Fil: Abdo, A. A.. Spece Sciences División. Naval Research Laboratory; Estados Unidos. National Academy of Sciences; Estados Unidos
Fil: Ackermann, M.. University Of Stanford; Estados Unidos
Fil: Ajello, M.. University Of Stanford; Estados Unidos
Fil: Baldini, L.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Ballet, J.. Universite Paris Diderot; Francia
Fil: Barbiellini, G.. Universita di Trieste; Italia
Fil: Bastieri, D.. Universita Di Padova; Italia
Fil: Baughman, B. M.. Ohio State University; Estados Unidos
Fil: Bechtol, K.. University Of Stanford; Estados Unidos
Fil: Bellazzini, R.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Berenji, B.. University Of Stanford; Estados Unidos
Fil: Blandford, R. D.. University Of Stanford; Estados Unidos
Fil: Bloom, E. D.. University Of Stanford; Estados Unidos
Fil: Bonamente, E.. Universita degli Studi di Perugia; Italia
Fil: Borgland, A. W.. University Of Stanford; Estados Unidos
Fil: Bregeon, J.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Brez, A.. Istituto Nazionale di Fisica Nucleare; Italia
Fil: Brigida, M.. Universita e del Politecnico di Bari; Italia
Fil: Bruel, P.. Ecole Polytechnique; Francia
Fil: Burnett, T. H.. University of Washington; Estados Unidos
Fil: Buson, S.. Universita Di Padova; Italia
Fil: Caliandro, G. A.. Universita e del Politecnico di Bari; Italia
Fil: Cameron, R. A.. University Of Stanford; Estados Unidos
Fil: Caraveo, P. A.. Istituto di Astrofisica Spaziale e Fisica Cosmica; Italia
Fil: Casandjian, J. M.. Université Paris Diderot - Paris 7; Francia
Fil: Cecchi, C.. Universita degli Studi di Perugia; Italia
Fil: Celik, O.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados Unidos
Fil: Chekhtman, A.. Space Science Division; Estados Unidos
Fil: Cheung, C. C.. National Aeronautics And Space Administration. Goddart Institute For Space Studies; Estados Unidos
Fil: Chiang, J.. University Of Stanford; Estados Unidos
Fil: Cillis, Analia Nilda. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina
Fil: Fermi-LAT Collaboration.
description We report observation of the supernova remnant (SNR) IC 443 (G189.1+3.0) with the Fermi Gamma-ray Space Telescope Large Area Telescope (LAT) in the energy band between 200 MeV and 50 GeV. IC 443 is a shell-type SNR with mixed morphology located off the outer Galactic plane where high-energy emission has been detected in the X-ray, GeV and TeV gamma-ray bands. Past observations suggest IC 443 has been interacting with surrounding interstellar matter. Proximity between dense shocked molecular clouds and GeV-TeV gamma-ray emission regions detected by EGRET, MAGIC, and VERITAS suggests an interpretation that cosmic-ray (CR) particles are accelerated by the SNR. With the high gamma-ray statistics and broad energy coverage provided by the LAT, we accurately characterize the gamma-ray emission produced by the CRs accelerated at IC 443. The emission region is extended in the energy band with θ68 = 0fdg27 ± 0fdg01(stat) ± 0fdg03(sys) for an assumed two-dimensional Gaussian profile and overlaps almost completely with the extended source region of VERITAS. Its centroid is displaced significantly from the known pulsar wind nebula (PWN) which suggests the PWN is not the major contributor in the present energy band. The observed spectrum changes its power-law slope continuously and continues smoothly to the MAGIC and VERITAS data points. The combined gamma-ray spectrum (200 MeV <E< 2 TeV) is reproduced well by decays of neutral pions produced by a broken power-law proton spectrum with a break around 70 GeV.
publishDate 2010
dc.date.none.fl_str_mv 2010-03-20
dc.type.none.fl_str_mv info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
http://purl.org/coar/resource_type/c_6501
info:ar-repo/semantics/articulo
format article
status_str publishedVersion
dc.identifier.none.fl_str_mv http://hdl.handle.net/11336/19154
Abdo, A. A.; Ackermann, M.; Ajello, M.; Baldini, L.; Ballet, J.; et al.; Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope; IOP Publishing; Astrophysical Journal; 712; 1; 20-3-2010; 459-468
0004-637X
CONICET Digital
CONICET
url http://hdl.handle.net/11336/19154
identifier_str_mv Abdo, A. A.; Ackermann, M.; Ajello, M.; Baldini, L.; Ballet, J.; et al.; Observation of Supernova Remnant IC 443 with the Fermi Large Area Telescope; IOP Publishing; Astrophysical Journal; 712; 1; 20-3-2010; 459-468
0004-637X
CONICET Digital
CONICET
dc.language.none.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv info:eu-repo/semantics/altIdentifier/url/http://iopscience.iop.org/0004-637X/712/1/459/pdf/apj_712_1_459.pdf
info:eu-repo/semantics/altIdentifier/url/https://arxiv.org/abs/1002.2198
info:eu-repo/semantics/altIdentifier/doi/10.1088/0004-637X/712/1/459
dc.rights.none.fl_str_mv info:eu-repo/semantics/openAccess
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
eu_rights_str_mv openAccess
rights_invalid_str_mv https://creativecommons.org/licenses/by-nc-sa/2.5/ar/
dc.format.none.fl_str_mv application/pdf
application/pdf
application/pdf
dc.publisher.none.fl_str_mv IOP Publishing
publisher.none.fl_str_mv IOP Publishing
dc.source.none.fl_str_mv reponame:CONICET Digital (CONICET)
instname:Consejo Nacional de Investigaciones Científicas y Técnicas
reponame_str CONICET Digital (CONICET)
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instname_str Consejo Nacional de Investigaciones Científicas y Técnicas
repository.name.fl_str_mv CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicas
repository.mail.fl_str_mv dasensio@conicet.gov.ar; lcarlino@conicet.gov.ar
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