Evidence that Ultra-high-energy Gamma Rays Are a Universal Feature near Powerful Pulsars
The highest-energy known gamma-ray sources are all located within 0.°5 of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; >56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the...
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| Veröffentlicht in: | Astrophysical journal. Letters 2021-04, Vol.911 (2), p.L27 |
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| creator | Albert, A. Alfaro, R. Alvarez, C. Álvarez, J. D. Angeles Camacho, J. R. Arteaga-Velázquez, J. C. Arunbabu, K. P. Rojas, D. Avila Ayala Solares, H. A. Baghmanyan, V. Belmont-Moreno, E. BenZvi, S. Y. Brisbois, C. Caballero-Mora, K. S. Capistrán, T. Carramiñana, A. Casanova, S. Cotti, U. Cotzomi, J. Coutiño de León, S. De la Fuente, E. de León, C. Diaz Hernandez, R. Dingus, B. L. DuVernois, M. A. Durocher, M. Díaz-Vélez, J. C. Ellsworth, R. W. Engel, K. Espinoza, C. Fan, K. L. Fernández Alonso, M. Fraija, N. Galván-Gámez, A. García-González, J. A. Garfias, F. Giacinti, G. González, M. M. Goodman, J. A. Harding, J. P. Hernandez, S. Hona, B. Huang, D. Hueyotl-Zahuantitla, F. Hüntemeyer, P. Iriarte, A. Jardin-Blicq, A. Joshi, V. Kieda, D. Lara, A. Lee, W. H. Lee, J. León Vargas, H. Linnemann, J. T. Longinotti, A. L. Luis-Raya, G. Lundeen, J. Malone, K. Marandon, V. Martinez, O. Martínez-Castro, J. Matthews, J. A. Miranda-Romagnoli, P. Morales-Soto, J. A. Moreno, E. Mostafá, M. Nayerhoda, A. Nellen, L. Newbold, M. Nisa, M. U. Noriega-Papaqui, R. Olivera-Nieto, L. Omodei, N. Peisker, A. Araujo, Y. Pérez Pérez-Pérez, E. G. Rho, C. D. Roh, Y. J. Rosa-González, D. Ruiz-Velasco, E. Salazar, H. Salesa Greus, F. Sandoval, A. Schneider, M. Schoorlemmer, H. Serna-Franco, J. Smith, A. J. Springer, R. W. Surajbali, P. Tanner, M. Tollefson, K. Torres, I. Torres-Escobedo, R. Turner, R. Ureña-Mena, F. Villaseñor, L. Weisgarber, T. Willox, E. Zhou, H. |
| description | The highest-energy known gamma-ray sources are all located within 0.°5 of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; >56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov Gamma-Ray Observatory, we present a joint-likelihood analysis of 10 extremely powerful pulsars to search for subthreshold UHE gamma-ray emission correlated with these locations. We report a significant detection (>3
σ
), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays and the implications of this result. The individual environment, such as the magnetic field and particle density in the surrounding area, appears to play a role in the amount of emission. |
| doi_str_mv | 10.3847/2041-8213/abf4dc |
| format | Article |
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S. ; Capistrán, T. ; Carramiñana, A. ; Casanova, S. ; Cotti, U. ; Cotzomi, J. ; Coutiño de León, S. ; De la Fuente, E. ; de León, C. ; Diaz Hernandez, R. ; Dingus, B. L. ; DuVernois, M. A. ; Durocher, M. ; Díaz-Vélez, J. C. ; Ellsworth, R. W. ; Engel, K. ; Espinoza, C. ; Fan, K. L. ; Fernández Alonso, M. ; Fraija, N. ; Galván-Gámez, A. ; García-González, J. A. ; Garfias, F. ; Giacinti, G. ; González, M. M. ; Goodman, J. A. ; Harding, J. P. ; Hernandez, S. ; Hona, B. ; Huang, D. ; Hueyotl-Zahuantitla, F. ; Hüntemeyer, P. ; Iriarte, A. ; Jardin-Blicq, A. ; Joshi, V. ; Kieda, D. ; Lara, A. ; Lee, W. H. ; Lee, J. ; León Vargas, H. ; Linnemann, J. T. ; Longinotti, A. L. ; Luis-Raya, G. ; Lundeen, J. ; Malone, K. ; Marandon, V. ; Martinez, O. ; Martínez-Castro, J. ; Matthews, J. A. ; Miranda-Romagnoli, P. ; Morales-Soto, J. A. ; Moreno, E. ; Mostafá, M. ; Nayerhoda, A. ; Nellen, L. ; Newbold, M. ; Nisa, M. U. ; Noriega-Papaqui, R. ; Olivera-Nieto, L. ; Omodei, N. ; Peisker, A. ; Araujo, Y. Pérez ; Pérez-Pérez, E. G. ; Rho, C. D. ; Roh, Y. J. ; Rosa-González, D. ; Ruiz-Velasco, E. ; Salazar, H. ; Salesa Greus, F. ; Sandoval, A. ; Schneider, M. ; Schoorlemmer, H. ; Serna-Franco, J. ; Smith, A. J. ; Springer, R. W. ; Surajbali, P. ; Tanner, M. ; Tollefson, K. ; Torres, I. ; Torres-Escobedo, R. ; Turner, R. ; Ureña-Mena, F. ; Villaseñor, L. ; Weisgarber, T. ; Willox, E. ; Zhou, H. ; HAWC Collaboration ; Los Alamos National Lab. (LANL), Los Alamos, NM (United States)</creatorcontrib><description>The highest-energy known gamma-ray sources are all located within 0.°5 of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; >56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov Gamma-Ray Observatory, we present a joint-likelihood analysis of 10 extremely powerful pulsars to search for subthreshold UHE gamma-ray emission correlated with these locations. We report a significant detection (>3
σ
), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays and the implications of this result. The individual environment, such as the magnetic field and particle density in the surrounding area, appears to play a role in the amount of emission.</description><identifier>ISSN: 2041-8205</identifier><identifier>EISSN: 2041-8213</identifier><identifier>DOI: 10.3847/2041-8213/abf4dc</identifier><language>eng</language><publisher>Austin: IOP Publishing</publisher><subject>ASTRONOMY AND ASTROPHYSICS ; Gamma emission ; Gamma ray astronomy ; Gamma ray sources ; Gamma rays ; High altitude ; Magnetic fields ; Particle density (concentration) ; Pulsars</subject><ispartof>Astrophysical journal. 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W.</creatorcontrib><creatorcontrib>Surajbali, P.</creatorcontrib><creatorcontrib>Tanner, M.</creatorcontrib><creatorcontrib>Tollefson, K.</creatorcontrib><creatorcontrib>Torres, I.</creatorcontrib><creatorcontrib>Torres-Escobedo, R.</creatorcontrib><creatorcontrib>Turner, R.</creatorcontrib><creatorcontrib>Ureña-Mena, F.</creatorcontrib><creatorcontrib>Villaseñor, L.</creatorcontrib><creatorcontrib>Weisgarber, T.</creatorcontrib><creatorcontrib>Willox, E.</creatorcontrib><creatorcontrib>Zhou, H.</creatorcontrib><creatorcontrib>HAWC Collaboration</creatorcontrib><creatorcontrib>Los Alamos National Lab. (LANL), Los Alamos, NM (United States)</creatorcontrib><title>Evidence that Ultra-high-energy Gamma Rays Are a Universal Feature near Powerful Pulsars</title><title>Astrophysical journal. Letters</title><description>The highest-energy known gamma-ray sources are all located within 0.°5 of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; >56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov Gamma-Ray Observatory, we present a joint-likelihood analysis of 10 extremely powerful pulsars to search for subthreshold UHE gamma-ray emission correlated with these locations. We report a significant detection (>3
σ
), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays and the implications of this result. 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that Ultra-high-energy Gamma Rays Are a Universal Feature near Powerful Pulsars</title><author>Albert, A. ; Alfaro, R. ; Alvarez, C. ; Álvarez, J. D. ; Angeles Camacho, J. R. ; Arteaga-Velázquez, J. C. ; Arunbabu, K. P. ; Rojas, D. Avila ; Ayala Solares, H. A. ; Baghmanyan, V. ; Belmont-Moreno, E. ; BenZvi, S. Y. ; Brisbois, C. ; Caballero-Mora, K. S. ; Capistrán, T. ; Carramiñana, A. ; Casanova, S. ; Cotti, U. ; Cotzomi, J. ; Coutiño de León, S. ; De la Fuente, E. ; de León, C. ; Diaz Hernandez, R. ; Dingus, B. L. ; DuVernois, M. A. ; Durocher, M. ; Díaz-Vélez, J. C. ; Ellsworth, R. W. ; Engel, K. ; Espinoza, C. ; Fan, K. L. ; Fernández Alonso, M. ; Fraija, N. ; Galván-Gámez, A. ; García-González, J. A. ; Garfias, F. ; Giacinti, G. ; González, M. M. ; Goodman, J. A. ; Harding, J. P. ; Hernandez, S. ; Hona, B. ; Huang, D. ; Hueyotl-Zahuantitla, F. ; Hüntemeyer, P. ; Iriarte, A. ; Jardin-Blicq, A. ; Joshi, V. ; Kieda, D. ; Lara, A. ; Lee, W. H. ; Lee, J. ; León Vargas, H. ; Linnemann, J. T. ; Longinotti, A. L. ; Luis-Raya, G. ; Lundeen, J. ; Malone, K. ; Marandon, V. ; Martinez, O. ; Martínez-Castro, J. ; Matthews, J. A. ; Miranda-Romagnoli, P. ; Morales-Soto, J. A. ; Moreno, E. ; Mostafá, M. ; Nayerhoda, A. ; Nellen, L. ; Newbold, M. ; Nisa, M. U. ; Noriega-Papaqui, R. ; Olivera-Nieto, L. ; Omodei, N. ; Peisker, A. ; Araujo, Y. Pérez ; Pérez-Pérez, E. G. ; Rho, C. D. ; Roh, Y. J. ; Rosa-González, D. ; Ruiz-Velasco, E. ; Salazar, H. ; Salesa Greus, F. ; Sandoval, A. ; Schneider, M. ; Schoorlemmer, H. ; Serna-Franco, J. ; Smith, A. J. ; Springer, R. W. ; Surajbali, P. ; Tanner, M. ; Tollefson, K. ; Torres, I. ; Torres-Escobedo, R. ; Turner, R. ; Ureña-Mena, F. ; Villaseñor, L. ; Weisgarber, T. ; Willox, E. ; Zhou, H.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c340t-9961dc8780d5a94967ffb92d850f77f4018deaca5a01e86772fae170aca571cd3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2021</creationdate><topic>ASTRONOMY AND ASTROPHYSICS</topic><topic>Gamma emission</topic><topic>Gamma ray astronomy</topic><topic>Gamma ray sources</topic><topic>Gamma rays</topic><topic>High altitude</topic><topic>Magnetic fields</topic><topic>Particle density (concentration)</topic><topic>Pulsars</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Albert, A.</creatorcontrib><creatorcontrib>Alfaro, R.</creatorcontrib><creatorcontrib>Alvarez, C.</creatorcontrib><creatorcontrib>Álvarez, J. D.</creatorcontrib><creatorcontrib>Angeles Camacho, J. R.</creatorcontrib><creatorcontrib>Arteaga-Velázquez, J. C.</creatorcontrib><creatorcontrib>Arunbabu, K. P.</creatorcontrib><creatorcontrib>Rojas, D. Avila</creatorcontrib><creatorcontrib>Ayala Solares, H. A.</creatorcontrib><creatorcontrib>Baghmanyan, V.</creatorcontrib><creatorcontrib>Belmont-Moreno, E.</creatorcontrib><creatorcontrib>BenZvi, S. Y.</creatorcontrib><creatorcontrib>Brisbois, C.</creatorcontrib><creatorcontrib>Caballero-Mora, K. S.</creatorcontrib><creatorcontrib>Capistrán, T.</creatorcontrib><creatorcontrib>Carramiñana, A.</creatorcontrib><creatorcontrib>Casanova, S.</creatorcontrib><creatorcontrib>Cotti, U.</creatorcontrib><creatorcontrib>Cotzomi, J.</creatorcontrib><creatorcontrib>Coutiño de León, S.</creatorcontrib><creatorcontrib>De la Fuente, E.</creatorcontrib><creatorcontrib>de León, C.</creatorcontrib><creatorcontrib>Diaz Hernandez, R.</creatorcontrib><creatorcontrib>Dingus, B. L.</creatorcontrib><creatorcontrib>DuVernois, M. A.</creatorcontrib><creatorcontrib>Durocher, M.</creatorcontrib><creatorcontrib>Díaz-Vélez, J. C.</creatorcontrib><creatorcontrib>Ellsworth, R. W.</creatorcontrib><creatorcontrib>Engel, K.</creatorcontrib><creatorcontrib>Espinoza, C.</creatorcontrib><creatorcontrib>Fan, K. L.</creatorcontrib><creatorcontrib>Fernández Alonso, M.</creatorcontrib><creatorcontrib>Fraija, N.</creatorcontrib><creatorcontrib>Galván-Gámez, A.</creatorcontrib><creatorcontrib>García-González, J. A.</creatorcontrib><creatorcontrib>Garfias, F.</creatorcontrib><creatorcontrib>Giacinti, G.</creatorcontrib><creatorcontrib>González, M. M.</creatorcontrib><creatorcontrib>Goodman, J. A.</creatorcontrib><creatorcontrib>Harding, J. P.</creatorcontrib><creatorcontrib>Hernandez, S.</creatorcontrib><creatorcontrib>Hona, B.</creatorcontrib><creatorcontrib>Huang, D.</creatorcontrib><creatorcontrib>Hueyotl-Zahuantitla, F.</creatorcontrib><creatorcontrib>Hüntemeyer, P.</creatorcontrib><creatorcontrib>Iriarte, A.</creatorcontrib><creatorcontrib>Jardin-Blicq, A.</creatorcontrib><creatorcontrib>Joshi, V.</creatorcontrib><creatorcontrib>Kieda, D.</creatorcontrib><creatorcontrib>Lara, A.</creatorcontrib><creatorcontrib>Lee, W. H.</creatorcontrib><creatorcontrib>Lee, J.</creatorcontrib><creatorcontrib>León Vargas, H.</creatorcontrib><creatorcontrib>Linnemann, J. T.</creatorcontrib><creatorcontrib>Longinotti, A. L.</creatorcontrib><creatorcontrib>Luis-Raya, G.</creatorcontrib><creatorcontrib>Lundeen, J.</creatorcontrib><creatorcontrib>Malone, K.</creatorcontrib><creatorcontrib>Marandon, V.</creatorcontrib><creatorcontrib>Martinez, O.</creatorcontrib><creatorcontrib>Martínez-Castro, J.</creatorcontrib><creatorcontrib>Matthews, J. A.</creatorcontrib><creatorcontrib>Miranda-Romagnoli, P.</creatorcontrib><creatorcontrib>Morales-Soto, J. A.</creatorcontrib><creatorcontrib>Moreno, E.</creatorcontrib><creatorcontrib>Mostafá, M.</creatorcontrib><creatorcontrib>Nayerhoda, A.</creatorcontrib><creatorcontrib>Nellen, L.</creatorcontrib><creatorcontrib>Newbold, M.</creatorcontrib><creatorcontrib>Nisa, M. U.</creatorcontrib><creatorcontrib>Noriega-Papaqui, R.</creatorcontrib><creatorcontrib>Olivera-Nieto, L.</creatorcontrib><creatorcontrib>Omodei, N.</creatorcontrib><creatorcontrib>Peisker, A.</creatorcontrib><creatorcontrib>Araujo, Y. Pérez</creatorcontrib><creatorcontrib>Pérez-Pérez, E. G.</creatorcontrib><creatorcontrib>Rho, C. D.</creatorcontrib><creatorcontrib>Roh, Y. J.</creatorcontrib><creatorcontrib>Rosa-González, D.</creatorcontrib><creatorcontrib>Ruiz-Velasco, E.</creatorcontrib><creatorcontrib>Salazar, H.</creatorcontrib><creatorcontrib>Salesa Greus, F.</creatorcontrib><creatorcontrib>Sandoval, A.</creatorcontrib><creatorcontrib>Schneider, M.</creatorcontrib><creatorcontrib>Schoorlemmer, H.</creatorcontrib><creatorcontrib>Serna-Franco, J.</creatorcontrib><creatorcontrib>Smith, A. J.</creatorcontrib><creatorcontrib>Springer, R. W.</creatorcontrib><creatorcontrib>Surajbali, P.</creatorcontrib><creatorcontrib>Tanner, M.</creatorcontrib><creatorcontrib>Tollefson, K.</creatorcontrib><creatorcontrib>Torres, I.</creatorcontrib><creatorcontrib>Torres-Escobedo, R.</creatorcontrib><creatorcontrib>Turner, R.</creatorcontrib><creatorcontrib>Ureña-Mena, F.</creatorcontrib><creatorcontrib>Villaseñor, L.</creatorcontrib><creatorcontrib>Weisgarber, T.</creatorcontrib><creatorcontrib>Willox, E.</creatorcontrib><creatorcontrib>Zhou, H.</creatorcontrib><creatorcontrib>HAWC Collaboration</creatorcontrib><creatorcontrib>Los Alamos National Lab. (LANL), Los Alamos, NM (United States)</creatorcontrib><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>OSTI.GOV - Hybrid</collection><collection>OSTI.GOV</collection><jtitle>Astrophysical journal. Letters</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Albert, A.</au><au>Alfaro, R.</au><au>Alvarez, C.</au><au>Álvarez, J. D.</au><au>Angeles Camacho, J. R.</au><au>Arteaga-Velázquez, J. C.</au><au>Arunbabu, K. P.</au><au>Rojas, D. Avila</au><au>Ayala Solares, H. A.</au><au>Baghmanyan, V.</au><au>Belmont-Moreno, E.</au><au>BenZvi, S. Y.</au><au>Brisbois, C.</au><au>Caballero-Mora, K. S.</au><au>Capistrán, T.</au><au>Carramiñana, A.</au><au>Casanova, S.</au><au>Cotti, U.</au><au>Cotzomi, J.</au><au>Coutiño de León, S.</au><au>De la Fuente, E.</au><au>de León, C.</au><au>Diaz Hernandez, R.</au><au>Dingus, B. L.</au><au>DuVernois, M. A.</au><au>Durocher, M.</au><au>Díaz-Vélez, J. C.</au><au>Ellsworth, R. W.</au><au>Engel, K.</au><au>Espinoza, C.</au><au>Fan, K. L.</au><au>Fernández Alonso, M.</au><au>Fraija, N.</au><au>Galván-Gámez, A.</au><au>García-González, J. A.</au><au>Garfias, F.</au><au>Giacinti, G.</au><au>González, M. M.</au><au>Goodman, J. A.</au><au>Harding, J. P.</au><au>Hernandez, S.</au><au>Hona, B.</au><au>Huang, D.</au><au>Hueyotl-Zahuantitla, F.</au><au>Hüntemeyer, P.</au><au>Iriarte, A.</au><au>Jardin-Blicq, A.</au><au>Joshi, V.</au><au>Kieda, D.</au><au>Lara, A.</au><au>Lee, W. H.</au><au>Lee, J.</au><au>León Vargas, H.</au><au>Linnemann, J. T.</au><au>Longinotti, A. L.</au><au>Luis-Raya, G.</au><au>Lundeen, J.</au><au>Malone, K.</au><au>Marandon, V.</au><au>Martinez, O.</au><au>Martínez-Castro, J.</au><au>Matthews, J. A.</au><au>Miranda-Romagnoli, P.</au><au>Morales-Soto, J. A.</au><au>Moreno, E.</au><au>Mostafá, M.</au><au>Nayerhoda, A.</au><au>Nellen, L.</au><au>Newbold, M.</au><au>Nisa, M. U.</au><au>Noriega-Papaqui, R.</au><au>Olivera-Nieto, L.</au><au>Omodei, N.</au><au>Peisker, A.</au><au>Araujo, Y. Pérez</au><au>Pérez-Pérez, E. G.</au><au>Rho, C. D.</au><au>Roh, Y. J.</au><au>Rosa-González, D.</au><au>Ruiz-Velasco, E.</au><au>Salazar, H.</au><au>Salesa Greus, F.</au><au>Sandoval, A.</au><au>Schneider, M.</au><au>Schoorlemmer, H.</au><au>Serna-Franco, J.</au><au>Smith, A. J.</au><au>Springer, R. W.</au><au>Surajbali, P.</au><au>Tanner, M.</au><au>Tollefson, K.</au><au>Torres, I.</au><au>Torres-Escobedo, R.</au><au>Turner, R.</au><au>Ureña-Mena, F.</au><au>Villaseñor, L.</au><au>Weisgarber, T.</au><au>Willox, E.</au><au>Zhou, H.</au><aucorp>HAWC Collaboration</aucorp><aucorp>Los Alamos National Lab. (LANL), Los Alamos, NM (United States)</aucorp><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Evidence that Ultra-high-energy Gamma Rays Are a Universal Feature near Powerful Pulsars</atitle><jtitle>Astrophysical journal. Letters</jtitle><date>2021-04-01</date><risdate>2021</risdate><volume>911</volume><issue>2</issue><spage>L27</spage><pages>L27-</pages><issn>2041-8205</issn><eissn>2041-8213</eissn><abstract>The highest-energy known gamma-ray sources are all located within 0.°5 of extremely powerful pulsars. This raises the question of whether ultra-high-energy (UHE; >56 TeV) gamma-ray emission is a universal feature expected near pulsars with a high spin-down power. Using four years of data from the High Altitude Water Cherenkov Gamma-Ray Observatory, we present a joint-likelihood analysis of 10 extremely powerful pulsars to search for subthreshold UHE gamma-ray emission correlated with these locations. We report a significant detection (>3
σ
), indicating that UHE gamma-ray emission is a generic feature of powerful pulsars. We discuss the emission mechanisms of the gamma rays and the implications of this result. 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| fulltext | fulltext |
| identifier | ISSN: 2041-8205 |
| ispartof | Astrophysical journal. Letters, 2021-04, Vol.911 (2), p.L27 |
| issn | 2041-8205 2041-8213 |
| language | eng |
| recordid | cdi_osti_scitechconnect_1804429 |
| source | Open Access: IOP Publishing Free Content; Institute of Physics IOPscience extra; Free E-Journal (出版社公開部分のみ）; Alma/SFX Local Collection |
| subjects | ASTRONOMY AND ASTROPHYSICS Gamma emission Gamma ray astronomy Gamma ray sources Gamma rays High altitude Magnetic fields Particle density (concentration) Pulsars |
| title | Evidence that Ultra-high-energy Gamma Rays Are a Universal Feature near Powerful Pulsars |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2024-12-28T08%3A31%3A16IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest_osti_&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.genre=article&rft.atitle=Evidence%20that%20Ultra-high-energy%20Gamma%20Rays%20Are%20a%20Universal%20Feature%20near%20Powerful%20Pulsars&rft.jtitle=Astrophysical%20journal.%20Letters&rft.au=Albert,%20A.&rft.aucorp=HAWC%20Collaboration&rft.date=2021-04-01&rft.volume=911&rft.issue=2&rft.spage=L27&rft.pages=L27-&rft.issn=2041-8205&rft.eissn=2041-8213&rft_id=info:doi/10.3847/2041-8213/abf4dc&rft_dat=%3Cproquest_osti_%3E2518773022%3C/proquest_osti_%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2518773022&rft_id=info:pmid/&rfr_iscdi=true |