Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data
The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSph...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Ackermann, M [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2015 |
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| Systematik: |
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| Übergeordnetes Werk: |
Enthalten in: Physical review letters - Ridge, NY : American Physical Society, 1958, 115(2015), 23 |
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| Übergeordnetes Werk: |
volume:115 ; year:2015 ; number:23 |
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OLC1969282959 |
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| 520 | |a The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. | ||
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PQ20160211 (DE-627)OLC1969282959 (DE-599)GBVOLC1969282959 (PRQ)p1201-bedd85444ec466e7ce68cae668970f0a6d8899c57291483e7af43070b5610a810 (KEY)0009201020150000115002300000searchingfordarkmatterannihilationfrommilkywaydwar DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Ackermann, M verfasserin aut Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. Albert, A oth Anderson, B oth Atwood, W B oth Baldini, L oth Barbiellini, G oth Bastieri, D oth Bechtol, K oth Bellazzini, R oth Bissaldi, E oth Blandford, R D oth Bloom, E D oth Bonino, R oth Bottacini, E oth Brandt, T J oth Bregeon, J oth Bruel, P oth Buehler, R oth Caliandro, G A oth Cameron, R A oth Caputo, R oth Caragiulo, M oth Caraveo, P A oth Cecchi, C oth Charles, E oth Chekhtman, A oth Chiang, J oth Chiaro, G oth Ciprini, S oth Claus, R oth Cohen-Tanugi, J oth Conrad, J oth Cuoco, A oth Cutini, S oth de Angelis, A oth de Palma, F oth Desiante, R oth Digel, S W oth Di Venere, L oth Drell, P S oth Drlica-Wagner, A oth Essig, R oth Favuzzi, C oth Fegan, S J oth Ferrara, E C oth Focke, W B oth Franckowiak, A oth Fukazawa, Y oth Funk, S oth Fusco, P oth Gargano, F oth Gasparrini, D oth Giglietto, N oth Giordano, F oth Giroletti, M oth Glanzman, T oth Godfrey, G oth Gomez-Vargas, G A oth Grenier, I A oth Guiriec, S oth Gustafsson, M oth Hays, E oth Hewitt, J W oth Horan, D oth Jogler, T oth Jóhannesson, G oth Kuss, M oth Larsson, S oth Latronico, L oth Li, J oth Li, L oth Llena Garde, M oth Longo, F oth Loparco, F oth Lubrano, P oth Malyshev, D oth Mayer, M oth Mazziotta, M N oth McEnery, J E oth Meyer, M oth Michelson, P F oth Mizuno, T oth Moiseev, A A oth Monzani, M E oth Morselli, A oth Murgia, S oth Nuss, E oth Ohsugi, T oth Orienti, M oth Orlando, E oth Ormes, J F oth Paneque, D oth Perkins, J S oth Pesce-Rollins, M oth Piron, F oth Pivato, G oth Porter, T A oth Rainò, S oth Rando, R oth D'Ammando, F oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 115(2015), 23 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:115 year:2015 number:23 http://www.ncbi.nlm.nih.gov/pubmed/26684107 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-124732 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 115 2015 23 |
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PQ20160211 (DE-627)OLC1969282959 (DE-599)GBVOLC1969282959 (PRQ)p1201-bedd85444ec466e7ce68cae668970f0a6d8899c57291483e7af43070b5610a810 (KEY)0009201020150000115002300000searchingfordarkmatterannihilationfrommilkywaydwar DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Ackermann, M verfasserin aut Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. Albert, A oth Anderson, B oth Atwood, W B oth Baldini, L oth Barbiellini, G oth Bastieri, D oth Bechtol, K oth Bellazzini, R oth Bissaldi, E oth Blandford, R D oth Bloom, E D oth Bonino, R oth Bottacini, E oth Brandt, T J oth Bregeon, J oth Bruel, P oth Buehler, R oth Caliandro, G A oth Cameron, R A oth Caputo, R oth Caragiulo, M oth Caraveo, P A oth Cecchi, C oth Charles, E oth Chekhtman, A oth Chiang, J oth Chiaro, G oth Ciprini, S oth Claus, R oth Cohen-Tanugi, J oth Conrad, J oth Cuoco, A oth Cutini, S oth de Angelis, A oth de Palma, F oth Desiante, R oth Digel, S W oth Di Venere, L oth Drell, P S oth Drlica-Wagner, A oth Essig, R oth Favuzzi, C oth Fegan, S J oth Ferrara, E C oth Focke, W B oth Franckowiak, A oth Fukazawa, Y oth Funk, S oth Fusco, P oth Gargano, F oth Gasparrini, D oth Giglietto, N oth Giordano, F oth Giroletti, M oth Glanzman, T oth Godfrey, G oth Gomez-Vargas, G A oth Grenier, I A oth Guiriec, S oth Gustafsson, M oth Hays, E oth Hewitt, J W oth Horan, D oth Jogler, T oth Jóhannesson, G oth Kuss, M oth Larsson, S oth Latronico, L oth Li, J oth Li, L oth Llena Garde, M oth Longo, F oth Loparco, F oth Lubrano, P oth Malyshev, D oth Mayer, M oth Mazziotta, M N oth McEnery, J E oth Meyer, M oth Michelson, P F oth Mizuno, T oth Moiseev, A A oth Monzani, M E oth Morselli, A oth Murgia, S oth Nuss, E oth Ohsugi, T oth Orienti, M oth Orlando, E oth Ormes, J F oth Paneque, D oth Perkins, J S oth Pesce-Rollins, M oth Piron, F oth Pivato, G oth Porter, T A oth Rainò, S oth Rando, R oth D'Ammando, F oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 115(2015), 23 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:115 year:2015 number:23 http://www.ncbi.nlm.nih.gov/pubmed/26684107 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-124732 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 115 2015 23 |
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PQ20160211 (DE-627)OLC1969282959 (DE-599)GBVOLC1969282959 (PRQ)p1201-bedd85444ec466e7ce68cae668970f0a6d8899c57291483e7af43070b5610a810 (KEY)0009201020150000115002300000searchingfordarkmatterannihilationfrommilkywaydwar DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Ackermann, M verfasserin aut Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. Albert, A oth Anderson, B oth Atwood, W B oth Baldini, L oth Barbiellini, G oth Bastieri, D oth Bechtol, K oth Bellazzini, R oth Bissaldi, E oth Blandford, R D oth Bloom, E D oth Bonino, R oth Bottacini, E oth Brandt, T J oth Bregeon, J oth Bruel, P oth Buehler, R oth Caliandro, G A oth Cameron, R A oth Caputo, R oth Caragiulo, M oth Caraveo, P A oth Cecchi, C oth Charles, E oth Chekhtman, A oth Chiang, J oth Chiaro, G oth Ciprini, S oth Claus, R oth Cohen-Tanugi, J oth Conrad, J oth Cuoco, A oth Cutini, S oth de Angelis, A oth de Palma, F oth Desiante, R oth Digel, S W oth Di Venere, L oth Drell, P S oth Drlica-Wagner, A oth Essig, R oth Favuzzi, C oth Fegan, S J oth Ferrara, E C oth Focke, W B oth Franckowiak, A oth Fukazawa, Y oth Funk, S oth Fusco, P oth Gargano, F oth Gasparrini, D oth Giglietto, N oth Giordano, F oth Giroletti, M oth Glanzman, T oth Godfrey, G oth Gomez-Vargas, G A oth Grenier, I A oth Guiriec, S oth Gustafsson, M oth Hays, E oth Hewitt, J W oth Horan, D oth Jogler, T oth Jóhannesson, G oth Kuss, M oth Larsson, S oth Latronico, L oth Li, J oth Li, L oth Llena Garde, M oth Longo, F oth Loparco, F oth Lubrano, P oth Malyshev, D oth Mayer, M oth Mazziotta, M N oth McEnery, J E oth Meyer, M oth Michelson, P F oth Mizuno, T oth Moiseev, A A oth Monzani, M E oth Morselli, A oth Murgia, S oth Nuss, E oth Ohsugi, T oth Orienti, M oth Orlando, E oth Ormes, J F oth Paneque, D oth Perkins, J S oth Pesce-Rollins, M oth Piron, F oth Pivato, G oth Porter, T A oth Rainò, S oth Rando, R oth D'Ammando, F oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 115(2015), 23 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:115 year:2015 number:23 http://www.ncbi.nlm.nih.gov/pubmed/26684107 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-124732 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 115 2015 23 |
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PQ20160211 (DE-627)OLC1969282959 (DE-599)GBVOLC1969282959 (PRQ)p1201-bedd85444ec466e7ce68cae668970f0a6d8899c57291483e7af43070b5610a810 (KEY)0009201020150000115002300000searchingfordarkmatterannihilationfrommilkywaydwar DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Ackermann, M verfasserin aut Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. Albert, A oth Anderson, B oth Atwood, W B oth Baldini, L oth Barbiellini, G oth Bastieri, D oth Bechtol, K oth Bellazzini, R oth Bissaldi, E oth Blandford, R D oth Bloom, E D oth Bonino, R oth Bottacini, E oth Brandt, T J oth Bregeon, J oth Bruel, P oth Buehler, R oth Caliandro, G A oth Cameron, R A oth Caputo, R oth Caragiulo, M oth Caraveo, P A oth Cecchi, C oth Charles, E oth Chekhtman, A oth Chiang, J oth Chiaro, G oth Ciprini, S oth Claus, R oth Cohen-Tanugi, J oth Conrad, J oth Cuoco, A oth Cutini, S oth de Angelis, A oth de Palma, F oth Desiante, R oth Digel, S W oth Di Venere, L oth Drell, P S oth Drlica-Wagner, A oth Essig, R oth Favuzzi, C oth Fegan, S J oth Ferrara, E C oth Focke, W B oth Franckowiak, A oth Fukazawa, Y oth Funk, S oth Fusco, P oth Gargano, F oth Gasparrini, D oth Giglietto, N oth Giordano, F oth Giroletti, M oth Glanzman, T oth Godfrey, G oth Gomez-Vargas, G A oth Grenier, I A oth Guiriec, S oth Gustafsson, M oth Hays, E oth Hewitt, J W oth Horan, D oth Jogler, T oth Jóhannesson, G oth Kuss, M oth Larsson, S oth Latronico, L oth Li, J oth Li, L oth Llena Garde, M oth Longo, F oth Loparco, F oth Lubrano, P oth Malyshev, D oth Mayer, M oth Mazziotta, M N oth McEnery, J E oth Meyer, M oth Michelson, P F oth Mizuno, T oth Moiseev, A A oth Monzani, M E oth Morselli, A oth Murgia, S oth Nuss, E oth Ohsugi, T oth Orienti, M oth Orlando, E oth Ormes, J F oth Paneque, D oth Perkins, J S oth Pesce-Rollins, M oth Piron, F oth Pivato, G oth Porter, T A oth Rainò, S oth Rando, R oth D'Ammando, F oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 115(2015), 23 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:115 year:2015 number:23 http://www.ncbi.nlm.nih.gov/pubmed/26684107 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-124732 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 115 2015 23 |
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PQ20160211 (DE-627)OLC1969282959 (DE-599)GBVOLC1969282959 (PRQ)p1201-bedd85444ec466e7ce68cae668970f0a6d8899c57291483e7af43070b5610a810 (KEY)0009201020150000115002300000searchingfordarkmatterannihilationfrommilkywaydwar DE-627 ger DE-627 rakwb eng 550 DNB UA 1000 AVZ rvk Ackermann, M verfasserin aut Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data 2015 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. Albert, A oth Anderson, B oth Atwood, W B oth Baldini, L oth Barbiellini, G oth Bastieri, D oth Bechtol, K oth Bellazzini, R oth Bissaldi, E oth Blandford, R D oth Bloom, E D oth Bonino, R oth Bottacini, E oth Brandt, T J oth Bregeon, J oth Bruel, P oth Buehler, R oth Caliandro, G A oth Cameron, R A oth Caputo, R oth Caragiulo, M oth Caraveo, P A oth Cecchi, C oth Charles, E oth Chekhtman, A oth Chiang, J oth Chiaro, G oth Ciprini, S oth Claus, R oth Cohen-Tanugi, J oth Conrad, J oth Cuoco, A oth Cutini, S oth de Angelis, A oth de Palma, F oth Desiante, R oth Digel, S W oth Di Venere, L oth Drell, P S oth Drlica-Wagner, A oth Essig, R oth Favuzzi, C oth Fegan, S J oth Ferrara, E C oth Focke, W B oth Franckowiak, A oth Fukazawa, Y oth Funk, S oth Fusco, P oth Gargano, F oth Gasparrini, D oth Giglietto, N oth Giordano, F oth Giroletti, M oth Glanzman, T oth Godfrey, G oth Gomez-Vargas, G A oth Grenier, I A oth Guiriec, S oth Gustafsson, M oth Hays, E oth Hewitt, J W oth Horan, D oth Jogler, T oth Jóhannesson, G oth Kuss, M oth Larsson, S oth Latronico, L oth Li, J oth Li, L oth Llena Garde, M oth Longo, F oth Loparco, F oth Lubrano, P oth Malyshev, D oth Mayer, M oth Mazziotta, M N oth McEnery, J E oth Meyer, M oth Michelson, P F oth Mizuno, T oth Moiseev, A A oth Monzani, M E oth Morselli, A oth Murgia, S oth Nuss, E oth Ohsugi, T oth Orienti, M oth Orlando, E oth Ormes, J F oth Paneque, D oth Perkins, J S oth Pesce-Rollins, M oth Piron, F oth Pivato, G oth Porter, T A oth Rainò, S oth Rando, R oth D'Ammando, F oth ... oth Enthalten in Physical review letters Ridge, NY : American Physical Society, 1958 115(2015), 23 (DE-627)129503959 (DE-600)208853-8 (DE-576)014907267 0031-9007 nnns volume:115 year:2015 number:23 http://www.ncbi.nlm.nih.gov/pubmed/26684107 http://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-124732 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_21 GBV_ILN_22 GBV_ILN_40 GBV_ILN_47 GBV_ILN_55 GBV_ILN_59 GBV_ILN_60 GBV_ILN_70 GBV_ILN_130 GBV_ILN_2004 GBV_ILN_2016 GBV_ILN_2095 GBV_ILN_2192 GBV_ILN_2279 GBV_ILN_2286 UA 1000 AR 115 2015 23 |
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Ackermann, M @@aut@@ Albert, A @@oth@@ Anderson, B @@oth@@ Atwood, W B @@oth@@ Baldini, L @@oth@@ Barbiellini, G @@oth@@ Bastieri, D @@oth@@ Bechtol, K @@oth@@ Bellazzini, R @@oth@@ Bissaldi, E @@oth@@ Blandford, R D @@oth@@ Bloom, E D @@oth@@ Bonino, R @@oth@@ Bottacini, E @@oth@@ Brandt, T J @@oth@@ Bregeon, J @@oth@@ Bruel, P @@oth@@ Buehler, R @@oth@@ Caliandro, G A @@oth@@ Cameron, R A @@oth@@ Caputo, R @@oth@@ Caragiulo, M @@oth@@ Caraveo, P A @@oth@@ Cecchi, C @@oth@@ Charles, E @@oth@@ Chekhtman, A @@oth@@ Chiang, J @@oth@@ Chiaro, G @@oth@@ Ciprini, S @@oth@@ Claus, R @@oth@@ Cohen-Tanugi, J @@oth@@ Conrad, J @@oth@@ Cuoco, A @@oth@@ Cutini, S @@oth@@ de Angelis, A @@oth@@ de Palma, F @@oth@@ Desiante, R @@oth@@ Digel, S W @@oth@@ Di Venere, L @@oth@@ Drell, P S @@oth@@ Drlica-Wagner, A @@oth@@ Essig, R @@oth@@ Favuzzi, C @@oth@@ Fegan, S J @@oth@@ Ferrara, E C @@oth@@ Focke, W B @@oth@@ Franckowiak, A @@oth@@ Fukazawa, Y @@oth@@ Funk, S @@oth@@ Fusco, P @@oth@@ Gargano, F @@oth@@ Gasparrini, D @@oth@@ Giglietto, N @@oth@@ Giordano, F @@oth@@ Giroletti, M @@oth@@ Glanzman, T @@oth@@ Godfrey, G @@oth@@ Gomez-Vargas, G A @@oth@@ Grenier, I A @@oth@@ Guiriec, S @@oth@@ Gustafsson, M @@oth@@ Hays, E @@oth@@ Hewitt, J W @@oth@@ Horan, D @@oth@@ Jogler, T @@oth@@ Jóhannesson, G @@oth@@ Kuss, M @@oth@@ Larsson, S @@oth@@ Latronico, L @@oth@@ Li, J @@oth@@ Li, L @@oth@@ Llena Garde, M @@oth@@ Longo, F @@oth@@ Loparco, F @@oth@@ Lubrano, P @@oth@@ Malyshev, D @@oth@@ Mayer, M @@oth@@ Mazziotta, M N @@oth@@ McEnery, J E @@oth@@ Meyer, M @@oth@@ Michelson, P F @@oth@@ Mizuno, T @@oth@@ Moiseev, A A @@oth@@ Monzani, M E @@oth@@ Morselli, A @@oth@@ Murgia, S @@oth@@ Nuss, E @@oth@@ Ohsugi, T @@oth@@ Orienti, M @@oth@@ Orlando, E @@oth@@ Ormes, J F @@oth@@ Paneque, D @@oth@@ Perkins, J S @@oth@@ Pesce-Rollins, M @@oth@@ Piron, F @@oth@@ Pivato, G @@oth@@ Porter, T A @@oth@@ Rainò, S @@oth@@ Rando, R @@oth@@ D'Ammando, F @@oth@@ ... @@oth@@ |
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searching for dark matter annihilation from milky way dwarf spheroidal galaxies with six years of fermi large area telescope data |
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Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data |
| abstract |
The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. |
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The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. |
| abstract_unstemmed |
The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. We report on γ-ray observations of Milky Way dSphs based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis. None of the dSphs are significantly detected in γ rays, and we present upper limits on the DM annihilation cross section from a combined analysis of 15 dSphs. These constraints are among the strongest and most robust to date and lie below the canonical thermal relic cross section for DM of mass ≲100 GeV annihilating via quark and τ-lepton channels. |
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Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1969282959</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20220224042708.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">160211s2015 xx ||||| 00| ||eng c</controlfield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20160211</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1969282959</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1969282959</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)p1201-bedd85444ec466e7ce68cae668970f0a6d8899c57291483e7af43070b5610a810</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0009201020150000115002300000searchingfordarkmatterannihilationfrommilkywaydwar</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">550</subfield><subfield code="q">DNB</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">UA 1000</subfield><subfield code="q">AVZ</subfield><subfield code="2">rvk</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Ackermann, M</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Searching for Dark Matter Annihilation from Milky Way Dwarf Spheroidal Galaxies with Six Years of Fermi Large Area Telescope Data</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2015</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">The dwarf spheroidal satellite galaxies (dSphs) of the Milky Way are some of the most dark matter (DM) dominated objects known. 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