$(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC$

(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC

This paper reports on the $\gamma$-ray properties of the 2018 Galactic nova V392 Per, spanning photon energies $\sim$0.1 GeV to 100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. In one of the most rapidly evolving $\gamma$-ray signals yet obse...

Ausführliche Beschreibung

Gespeichert in:

Bibliographische Detailangaben
Veröffentlicht in:	arXiv.org 2022-12
Hauptverfasser:	Albert, A, Alfaro, R, Alvarez, C, Arteaga-Velázquez, J C, D Avila Rojas, Ayala Solares, H A, Babu, R, Belmont-Moreno, E, Blochwitz, C, Caballero-Mora, K S, Capistrán, T, Carramiñana, A, Casanova, S, Chaparro-Amaro, O, Cotti, U, Cotzomi, J, E De la Fuente C de León S Coutiño de León, R Diaz Hernandez, Dingus, B L, DuVernois, M A, Durocher, M, Díaz-Vélez, J C, Engel, K, Espinoza, C, Fan, K L, Fang, K, Fraija, N, García-González, J A, Garfias, F, González, M M, Goodman, J A, Harding, J P, Hernandez, S, Hinton, J, Huang, D, Hueyotl-Zahuantitla, F, Hüntemeyer, P, Iriarte, A, Joshi, V, Lara, A, Lee, W 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, Omodei, N, Peisker, A, Y Pérez Araujo, Pérez-Pérez, E G, Rho, C D, Rosa-González, D, Ruiz-Velasco, E, Salazar-Gallegos, D, F Salesa Greus, Serna-Franco, A Sandoval J, Smith, A J, Son, Y, Springer, R W, Tibolla, O, Tollefson, K, Torres, I, Torres-Escobedo, R, Turner, R, Ureña-Mena, F, Villaseñor, L, Wang, X, Willox, E, A Zepeda H Zhou, Chomiuk, L, Aydi, E, Li, K L, Metzger, B D, Vurm, I
Format:	Artikel
Sprache:	eng
Schlagworte:	Emission analysis Fermi Gamma-ray Space Telescope Space telescopes
Online-Zugang:	Volltext
Tags:	Tag hinzufügen Keine Tags, Fügen Sie den ersten Tag hinzu!

container_end_page
container_issue
container_start_page
container_title	arXiv.org
container_volume
creator	Albert, A Alfaro, R Alvarez, C Arteaga-Velázquez, J C D Avila Rojas Ayala Solares, H A Babu, R Belmont-Moreno, E Blochwitz, C Caballero-Mora, K S Capistrán, T Carramiñana, A Casanova, S Chaparro-Amaro, O Cotti, U Cotzomi, J E De la Fuente C de León S Coutiño de León R Diaz Hernandez Dingus, B L DuVernois, M A Durocher, M Díaz-Vélez, J C Engel, K Espinoza, C Fan, K L Fang, K Fraija, N García-González, J A Garfias, F González, M M Goodman, J A Harding, J P Hernandez, S Hinton, J Huang, D Hueyotl-Zahuantitla, F Hüntemeyer, P Iriarte, A Joshi, V Lara, A Lee, W 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 Omodei, N Peisker, A Y Pérez Araujo Pérez-Pérez, E G Rho, C D Rosa-González, D Ruiz-Velasco, E Salazar-Gallegos, D F Salesa Greus Serna-Franco, A Sandoval J Smith, A J Son, Y Springer, R W Tibolla, O Tollefson, K Torres, I Torres-Escobedo, R Turner, R Ureña-Mena, F Villaseñor, L Wang, X Willox, E A Zepeda H Zhou Chomiuk, L Aydi, E Li, K L Metzger, B D Vurm, I
description	This paper reports on the $\gamma$-ray properties of the 2018 Galactic nova V392 Per, spanning photon energies $\sim$0.1 GeV to 100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. In one of the most rapidly evolving $\gamma$-ray signals yet observed for a nova, GeV $\gamma$ rays with a power law spectrum with index $\Gamma = 2.0 \pm 0.1$ were detected over eight days following V392 Per's optical maximum. HAWC observations constrain the TeV $\gamma$-ray signal during this time and also before and after. We observe no statistically significant evidence of TeV $\gamma$-ray emission from V392 Per, but present flux limits. Tests of the extension of the Fermi/LAT spectrum to energies above 5 TeV are disfavored by 2 standard deviations (95\%) or more. We fit V392 Per's GeV $\gamma$ rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits.
doi_str_mv	10.48550/arxiv.2201.10644
format	Article
fullrecord	<record><control><sourceid>proquest</sourceid><recordid>TN_cdi_proquest_journals_2623197893</recordid><sourceformat>XML</sourceformat><sourcesystem>PC</sourcesystem><sourcerecordid>2623197893</sourcerecordid><originalsourceid>FETCH-proquest_journals_26231978933</originalsourceid><addsrcrecordid>eNqNirsKwjAUQIMgKNoPcLvgokNrctPW1k2K4qI4-FgEuWiUStNoYkX_XkE_wOlwOIexjuBBmEQRH5B95o8AkYtA8DgMa6yJUgo_CREbzHPuwjnHeIhRJJts3dudSWva9X1LL5jo3LnclHCyRkNW0McOVMDCPAg2MkVYKjuCuSJXWaVVeXffdaqszoHKI8zG26zN6icqnPJ-bLHudLLKZv7Vmlul3H1_MZUtP2mPMUqRDpNUyv-uN-qhRLM</addsrcrecordid><sourcetype>Aggregation Database</sourcetype><iscdi>true</iscdi><recordtype>article</recordtype><pqid>2623197893</pqid></control><display><type>article</type><title>(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC</title><source>Free E- Journals</source><creator>Albert, A ; Alfaro, R ; Alvarez, C ; Arteaga-Velázquez, J C ; D Avila Rojas ; Ayala Solares, H A ; Babu, R ; Belmont-Moreno, E ; Blochwitz, C ; Caballero-Mora, K S ; Capistrán, T ; Carramiñana, A ; Casanova, S ; Chaparro-Amaro, O ; Cotti, U ; Cotzomi, J ; E De la Fuente C de León S Coutiño de León ; R Diaz Hernandez ; Dingus, B L ; DuVernois, M A ; Durocher, M ; Díaz-Vélez, J C ; Engel, K ; Espinoza, C ; Fan, K L ; Fang, K ; Fraija, N ; García-González, J A ; Garfias, F ; González, M M ; Goodman, J A ; Harding, J P ; Hernandez, S ; Hinton, J ; Huang, D ; Hueyotl-Zahuantitla, F ; Hüntemeyer, P ; Iriarte, A ; Joshi, V ; Lara, A ; Lee, W 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 ; Omodei, N ; Peisker, A ; Y Pérez Araujo ; Pérez-Pérez, E G ; Rho, C D ; Rosa-González, D ; Ruiz-Velasco, E ; Salazar-Gallegos, D ; F Salesa Greus ; Serna-Franco, A Sandoval J ; Smith, A J ; Son, Y ; Springer, R W ; Tibolla, O ; Tollefson, K ; Torres, I ; Torres-Escobedo, R ; Turner, R ; Ureña-Mena, F ; Villaseñor, L ; Wang, X ; Willox, E ; A Zepeda H Zhou ; Chomiuk, L ; Aydi, E ; Li, K L ; Metzger, B D ; Vurm, I</creator><creatorcontrib>Albert, A ; Alfaro, R ; Alvarez, C ; Arteaga-Velázquez, J C ; D Avila Rojas ; Ayala Solares, H A ; Babu, R ; Belmont-Moreno, E ; Blochwitz, C ; Caballero-Mora, K S ; Capistrán, T ; Carramiñana, A ; Casanova, S ; Chaparro-Amaro, O ; Cotti, U ; Cotzomi, J ; E De la Fuente C de León S Coutiño de León ; R Diaz Hernandez ; Dingus, B L ; DuVernois, M A ; Durocher, M ; Díaz-Vélez, J C ; Engel, K ; Espinoza, C ; Fan, K L ; Fang, K ; Fraija, N ; García-González, J A ; Garfias, F ; González, M M ; Goodman, J A ; Harding, J P ; Hernandez, S ; Hinton, J ; Huang, D ; Hueyotl-Zahuantitla, F ; Hüntemeyer, P ; Iriarte, A ; Joshi, V ; Lara, A ; Lee, W 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 ; Omodei, N ; Peisker, A ; Y Pérez Araujo ; Pérez-Pérez, E G ; Rho, C D ; Rosa-González, D ; Ruiz-Velasco, E ; Salazar-Gallegos, D ; F Salesa Greus ; Serna-Franco, A Sandoval J ; Smith, A J ; Son, Y ; Springer, R W ; Tibolla, O ; Tollefson, K ; Torres, I ; Torres-Escobedo, R ; Turner, R ; Ureña-Mena, F ; Villaseñor, L ; Wang, X ; Willox, E ; A Zepeda H Zhou ; Chomiuk, L ; Aydi, E ; Li, K L ; Metzger, B D ; Vurm, I</creatorcontrib><description>This paper reports on the $\gamma$-ray properties of the 2018 Galactic nova V392 Per, spanning photon energies $\sim$0.1 GeV to 100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. In one of the most rapidly evolving $\gamma$-ray signals yet observed for a nova, GeV $\gamma$ rays with a power law spectrum with index $\Gamma = 2.0 \pm 0.1$ were detected over eight days following V392 Per's optical maximum. HAWC observations constrain the TeV $\gamma$-ray signal during this time and also before and after. We observe no statistically significant evidence of TeV $\gamma$-ray emission from V392 Per, but present flux limits. Tests of the extension of the Fermi/LAT spectrum to energies above 5 TeV are disfavored by 2 standard deviations (95\%) or more. We fit V392 Per's GeV $\gamma$ rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits.</description><identifier>EISSN: 2331-8422</identifier><identifier>DOI: 10.48550/arxiv.2201.10644</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>Emission analysis ; Fermi Gamma-ray Space Telescope ; Space telescopes</subject><ispartof>arXiv.org, 2022-12</ispartof><rights>2022. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). Notwithstanding the ProQuest Terms and Conditions, you may use this content in accordance with the terms of the License.</rights><oa>free_for_read</oa><woscitedreferencessubscribed>false</woscitedreferencessubscribed></display><links><openurl>$$Topenurl_article</openurl><openurlfulltext>$$Topenurlfull_article</openurlfulltext><thumbnail>$$Tsyndetics_thumb_exl</thumbnail><link.rule.ids>780,784,27923</link.rule.ids></links><search><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>Alfaro, R</creatorcontrib><creatorcontrib>Alvarez, C</creatorcontrib><creatorcontrib>Arteaga-Velázquez, J C</creatorcontrib><creatorcontrib>D Avila Rojas</creatorcontrib><creatorcontrib>Ayala Solares, H A</creatorcontrib><creatorcontrib>Babu, R</creatorcontrib><creatorcontrib>Belmont-Moreno, E</creatorcontrib><creatorcontrib>Blochwitz, C</creatorcontrib><creatorcontrib>Caballero-Mora, K S</creatorcontrib><creatorcontrib>Capistrán, T</creatorcontrib><creatorcontrib>Carramiñana, A</creatorcontrib><creatorcontrib>Casanova, S</creatorcontrib><creatorcontrib>Chaparro-Amaro, O</creatorcontrib><creatorcontrib>Cotti, U</creatorcontrib><creatorcontrib>Cotzomi, J</creatorcontrib><creatorcontrib>E De la Fuente C de León S Coutiño de León</creatorcontrib><creatorcontrib>R Diaz Hernandez</creatorcontrib><creatorcontrib>Dingus, B L</creatorcontrib><creatorcontrib>DuVernois, M A</creatorcontrib><creatorcontrib>Durocher, M</creatorcontrib><creatorcontrib>Díaz-Vélez, J C</creatorcontrib><creatorcontrib>Engel, K</creatorcontrib><creatorcontrib>Espinoza, C</creatorcontrib><creatorcontrib>Fan, K L</creatorcontrib><creatorcontrib>Fang, K</creatorcontrib><creatorcontrib>Fraija, N</creatorcontrib><creatorcontrib>García-González, J A</creatorcontrib><creatorcontrib>Garfias, F</creatorcontrib><creatorcontrib>González, M M</creatorcontrib><creatorcontrib>Goodman, J A</creatorcontrib><creatorcontrib>Harding, J P</creatorcontrib><creatorcontrib>Hernandez, S</creatorcontrib><creatorcontrib>Hinton, J</creatorcontrib><creatorcontrib>Huang, D</creatorcontrib><creatorcontrib>Hueyotl-Zahuantitla, F</creatorcontrib><creatorcontrib>Hüntemeyer, P</creatorcontrib><creatorcontrib>Iriarte, A</creatorcontrib><creatorcontrib>Joshi, V</creatorcontrib><creatorcontrib>Lara, A</creatorcontrib><creatorcontrib>Lee, W 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>Omodei, N</creatorcontrib><creatorcontrib>Peisker, A</creatorcontrib><creatorcontrib>Y Pérez Araujo</creatorcontrib><creatorcontrib>Pérez-Pérez, E G</creatorcontrib><creatorcontrib>Rho, C D</creatorcontrib><creatorcontrib>Rosa-González, D</creatorcontrib><creatorcontrib>Ruiz-Velasco, E</creatorcontrib><creatorcontrib>Salazar-Gallegos, D</creatorcontrib><creatorcontrib>F Salesa Greus</creatorcontrib><creatorcontrib>Serna-Franco, A Sandoval J</creatorcontrib><creatorcontrib>Smith, A J</creatorcontrib><creatorcontrib>Son, Y</creatorcontrib><creatorcontrib>Springer, R W</creatorcontrib><creatorcontrib>Tibolla, O</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>Wang, X</creatorcontrib><creatorcontrib>Willox, E</creatorcontrib><creatorcontrib>A Zepeda H Zhou</creatorcontrib><creatorcontrib>Chomiuk, L</creatorcontrib><creatorcontrib>Aydi, E</creatorcontrib><creatorcontrib>Li, K L</creatorcontrib><creatorcontrib>Metzger, B D</creatorcontrib><creatorcontrib>Vurm, I</creatorcontrib><title>(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC</title><title>arXiv.org</title><description>This paper reports on the $\gamma$-ray properties of the 2018 Galactic nova V392 Per, spanning photon energies $\sim$0.1 GeV to 100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. In one of the most rapidly evolving $\gamma$-ray signals yet observed for a nova, GeV $\gamma$ rays with a power law spectrum with index $\Gamma = 2.0 \pm 0.1$ were detected over eight days following V392 Per's optical maximum. HAWC observations constrain the TeV $\gamma$-ray signal during this time and also before and after. We observe no statistically significant evidence of TeV $\gamma$-ray emission from V392 Per, but present flux limits. Tests of the extension of the Fermi/LAT spectrum to energies above 5 TeV are disfavored by 2 standard deviations (95\%) or more. We fit V392 Per's GeV $\gamma$ rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits.</description><subject>Emission analysis</subject><subject>Fermi Gamma-ray Space Telescope</subject><subject>Space telescopes</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><recordid>eNqNirsKwjAUQIMgKNoPcLvgokNrctPW1k2K4qI4-FgEuWiUStNoYkX_XkE_wOlwOIexjuBBmEQRH5B95o8AkYtA8DgMa6yJUgo_CREbzHPuwjnHeIhRJJts3dudSWva9X1LL5jo3LnclHCyRkNW0McOVMDCPAg2MkVYKjuCuSJXWaVVeXffdaqszoHKI8zG26zN6icqnPJ-bLHudLLKZv7Vmlul3H1_MZUtP2mPMUqRDpNUyv-uN-qhRLM</recordid><startdate>20221216</startdate><enddate>20221216</enddate><creator>Albert, A</creator><creator>Alfaro, R</creator><creator>Alvarez, C</creator><creator>Arteaga-Velázquez, J C</creator><creator>D Avila Rojas</creator><creator>Ayala Solares, H A</creator><creator>Babu, R</creator><creator>Belmont-Moreno, E</creator><creator>Blochwitz, C</creator><creator>Caballero-Mora, K S</creator><creator>Capistrán, T</creator><creator>Carramiñana, A</creator><creator>Casanova, S</creator><creator>Chaparro-Amaro, O</creator><creator>Cotti, U</creator><creator>Cotzomi, J</creator><creator>E De la Fuente C de León S Coutiño de León</creator><creator>R Diaz Hernandez</creator><creator>Dingus, B L</creator><creator>DuVernois, M A</creator><creator>Durocher, M</creator><creator>Díaz-Vélez, J C</creator><creator>Engel, K</creator><creator>Espinoza, C</creator><creator>Fan, K L</creator><creator>Fang, K</creator><creator>Fraija, N</creator><creator>García-González, J A</creator><creator>Garfias, F</creator><creator>González, M M</creator><creator>Goodman, J A</creator><creator>Harding, J P</creator><creator>Hernandez, S</creator><creator>Hinton, J</creator><creator>Huang, D</creator><creator>Hueyotl-Zahuantitla, F</creator><creator>Hüntemeyer, P</creator><creator>Iriarte, A</creator><creator>Joshi, V</creator><creator>Lara, A</creator><creator>Lee, W H</creator><creator>Linnemann, J T</creator><creator>Longinotti, A L</creator><creator>Luis-Raya, G</creator><creator>Lundeen, J</creator><creator>Malone, K</creator><creator>Marandon, V</creator><creator>Martinez, O</creator><creator>Martínez-Castro, J</creator><creator>Matthews, J A</creator><creator>Miranda-Romagnoli, P</creator><creator>Morales-Soto, J A</creator><creator>Moreno, E</creator><creator>Mostafá, M</creator><creator>Nayerhoda, A</creator><creator>Nellen, L</creator><creator>Newbold, M</creator><creator>Nisa, M U</creator><creator>Noriega-Papaqui, R</creator><creator>Omodei, N</creator><creator>Peisker, A</creator><creator>Y Pérez Araujo</creator><creator>Pérez-Pérez, E G</creator><creator>Rho, C D</creator><creator>Rosa-González, D</creator><creator>Ruiz-Velasco, E</creator><creator>Salazar-Gallegos, D</creator><creator>F Salesa Greus</creator><creator>Serna-Franco, A Sandoval J</creator><creator>Smith, A J</creator><creator>Son, Y</creator><creator>Springer, R W</creator><creator>Tibolla, O</creator><creator>Tollefson, K</creator><creator>Torres, I</creator><creator>Torres-Escobedo, R</creator><creator>Turner, R</creator><creator>Ureña-Mena, F</creator><creator>Villaseñor, L</creator><creator>Wang, X</creator><creator>Willox, E</creator><creator>A Zepeda H Zhou</creator><creator>Chomiuk, L</creator><creator>Aydi, E</creator><creator>Li, K L</creator><creator>Metzger, B D</creator><creator>Vurm, I</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20221216</creationdate><title>(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC</title><author>Albert, A ; Alfaro, R ; Alvarez, C ; Arteaga-Velázquez, J C ; D Avila Rojas ; Ayala Solares, H A ; Babu, R ; Belmont-Moreno, E ; Blochwitz, C ; Caballero-Mora, K S ; Capistrán, T ; Carramiñana, A ; Casanova, S ; Chaparro-Amaro, O ; Cotti, U ; Cotzomi, J ; E De la Fuente C de León S Coutiño de León ; R Diaz Hernandez ; Dingus, B L ; DuVernois, M A ; Durocher, M ; Díaz-Vélez, J C ; Engel, K ; Espinoza, C ; Fan, K L ; Fang, K ; Fraija, N ; García-González, J A ; Garfias, F ; González, M M ; Goodman, J A ; Harding, J P ; Hernandez, S ; Hinton, J ; Huang, D ; Hueyotl-Zahuantitla, F ; Hüntemeyer, P ; Iriarte, A ; Joshi, V ; Lara, A ; Lee, W 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 ; Omodei, N ; Peisker, A ; Y Pérez Araujo ; Pérez-Pérez, E G ; Rho, C D ; Rosa-González, D ; Ruiz-Velasco, E ; Salazar-Gallegos, D ; F Salesa Greus ; Serna-Franco, A Sandoval J ; Smith, A J ; Son, Y ; Springer, R W ; Tibolla, O ; Tollefson, K ; Torres, I ; Torres-Escobedo, R ; Turner, R ; Ureña-Mena, F ; Villaseñor, L ; Wang, X ; Willox, E ; A Zepeda H Zhou ; Chomiuk, L ; Aydi, E ; Li, K L ; Metzger, B D ; Vurm, I</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_26231978933</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2022</creationdate><topic>Emission analysis</topic><topic>Fermi Gamma-ray Space Telescope</topic><topic>Space telescopes</topic><toplevel>online_resources</toplevel><creatorcontrib>Albert, A</creatorcontrib><creatorcontrib>Alfaro, R</creatorcontrib><creatorcontrib>Alvarez, C</creatorcontrib><creatorcontrib>Arteaga-Velázquez, J C</creatorcontrib><creatorcontrib>D Avila Rojas</creatorcontrib><creatorcontrib>Ayala Solares, H A</creatorcontrib><creatorcontrib>Babu, R</creatorcontrib><creatorcontrib>Belmont-Moreno, E</creatorcontrib><creatorcontrib>Blochwitz, C</creatorcontrib><creatorcontrib>Caballero-Mora, K S</creatorcontrib><creatorcontrib>Capistrán, T</creatorcontrib><creatorcontrib>Carramiñana, A</creatorcontrib><creatorcontrib>Casanova, S</creatorcontrib><creatorcontrib>Chaparro-Amaro, O</creatorcontrib><creatorcontrib>Cotti, U</creatorcontrib><creatorcontrib>Cotzomi, J</creatorcontrib><creatorcontrib>E De la Fuente C de León S Coutiño de León</creatorcontrib><creatorcontrib>R Diaz Hernandez</creatorcontrib><creatorcontrib>Dingus, B L</creatorcontrib><creatorcontrib>DuVernois, M A</creatorcontrib><creatorcontrib>Durocher, M</creatorcontrib><creatorcontrib>Díaz-Vélez, J C</creatorcontrib><creatorcontrib>Engel, K</creatorcontrib><creatorcontrib>Espinoza, C</creatorcontrib><creatorcontrib>Fan, K L</creatorcontrib><creatorcontrib>Fang, K</creatorcontrib><creatorcontrib>Fraija, N</creatorcontrib><creatorcontrib>García-González, J A</creatorcontrib><creatorcontrib>Garfias, F</creatorcontrib><creatorcontrib>González, M M</creatorcontrib><creatorcontrib>Goodman, J A</creatorcontrib><creatorcontrib>Harding, J P</creatorcontrib><creatorcontrib>Hernandez, S</creatorcontrib><creatorcontrib>Hinton, J</creatorcontrib><creatorcontrib>Huang, D</creatorcontrib><creatorcontrib>Hueyotl-Zahuantitla, F</creatorcontrib><creatorcontrib>Hüntemeyer, P</creatorcontrib><creatorcontrib>Iriarte, A</creatorcontrib><creatorcontrib>Joshi, V</creatorcontrib><creatorcontrib>Lara, A</creatorcontrib><creatorcontrib>Lee, W 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>Omodei, N</creatorcontrib><creatorcontrib>Peisker, A</creatorcontrib><creatorcontrib>Y Pérez Araujo</creatorcontrib><creatorcontrib>Pérez-Pérez, E G</creatorcontrib><creatorcontrib>Rho, C D</creatorcontrib><creatorcontrib>Rosa-González, D</creatorcontrib><creatorcontrib>Ruiz-Velasco, E</creatorcontrib><creatorcontrib>Salazar-Gallegos, D</creatorcontrib><creatorcontrib>F Salesa Greus</creatorcontrib><creatorcontrib>Serna-Franco, A Sandoval J</creatorcontrib><creatorcontrib>Smith, A J</creatorcontrib><creatorcontrib>Son, Y</creatorcontrib><creatorcontrib>Springer, R W</creatorcontrib><creatorcontrib>Tibolla, O</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>Wang, X</creatorcontrib><creatorcontrib>Willox, E</creatorcontrib><creatorcontrib>A Zepeda H Zhou</creatorcontrib><creatorcontrib>Chomiuk, L</creatorcontrib><creatorcontrib>Aydi, E</creatorcontrib><creatorcontrib>Li, K L</creatorcontrib><creatorcontrib>Metzger, B D</creatorcontrib><creatorcontrib>Vurm, I</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Collection</collection><collection>ProQuest Central (Alumni Edition)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection (ProQuest)</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central Korea</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering Collection</collection></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>Arteaga-Velázquez, J C</au><au>D Avila Rojas</au><au>Ayala Solares, H A</au><au>Babu, R</au><au>Belmont-Moreno, E</au><au>Blochwitz, C</au><au>Caballero-Mora, K S</au><au>Capistrán, T</au><au>Carramiñana, A</au><au>Casanova, S</au><au>Chaparro-Amaro, O</au><au>Cotti, U</au><au>Cotzomi, J</au><au>E De la Fuente C de León S Coutiño de León</au><au>R Diaz Hernandez</au><au>Dingus, B L</au><au>DuVernois, M A</au><au>Durocher, M</au><au>Díaz-Vélez, J C</au><au>Engel, K</au><au>Espinoza, C</au><au>Fan, K L</au><au>Fang, K</au><au>Fraija, N</au><au>García-González, J A</au><au>Garfias, F</au><au>González, M M</au><au>Goodman, J A</au><au>Harding, J P</au><au>Hernandez, S</au><au>Hinton, J</au><au>Huang, D</au><au>Hueyotl-Zahuantitla, F</au><au>Hüntemeyer, P</au><au>Iriarte, A</au><au>Joshi, V</au><au>Lara, A</au><au>Lee, W 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>Omodei, N</au><au>Peisker, A</au><au>Y Pérez Araujo</au><au>Pérez-Pérez, E G</au><au>Rho, C D</au><au>Rosa-González, D</au><au>Ruiz-Velasco, E</au><au>Salazar-Gallegos, D</au><au>F Salesa Greus</au><au>Serna-Franco, A Sandoval J</au><au>Smith, A J</au><au>Son, Y</au><au>Springer, R W</au><au>Tibolla, O</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>Wang, X</au><au>Willox, E</au><au>A Zepeda H Zhou</au><au>Chomiuk, L</au><au>Aydi, E</au><au>Li, K L</au><au>Metzger, B D</au><au>Vurm, I</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC</atitle><jtitle>arXiv.org</jtitle><date>2022-12-16</date><risdate>2022</risdate><eissn>2331-8422</eissn><abstract>This paper reports on the $\gamma$-ray properties of the 2018 Galactic nova V392 Per, spanning photon energies $\sim$0.1 GeV to 100 TeV by combining observations from the Fermi Gamma-ray Space Telescope and the HAWC Observatory. In one of the most rapidly evolving $\gamma$-ray signals yet observed for a nova, GeV $\gamma$ rays with a power law spectrum with index $\Gamma = 2.0 \pm 0.1$ were detected over eight days following V392 Per's optical maximum. HAWC observations constrain the TeV $\gamma$-ray signal during this time and also before and after. We observe no statistically significant evidence of TeV $\gamma$-ray emission from V392 Per, but present flux limits. Tests of the extension of the Fermi/LAT spectrum to energies above 5 TeV are disfavored by 2 standard deviations (95\%) or more. We fit V392 Per's GeV $\gamma$ rays with hadronic acceleration models, incorporating optical observations, and compare the calculations with HAWC limits.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><doi>10.48550/arxiv.2201.10644</doi><oa>free_for_read</oa></addata></record>
fulltext	fulltext
identifier	EISSN: 2331-8422
ispartof	arXiv.org, 2022-12
issn	2331-8422
language	eng
recordid	cdi_proquest_journals_2623197893
source	Free E- Journals
subjects	Emission analysis Fermi Gamma-ray Space Telescope Space telescopes
title	(\gamma\)-ray Emission from Classical Nova V392 Per: Measurements from Fermi and HAWC
url	https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-01-09T13%3A17%3A54IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=(%5Cgamma%5C)-ray%20Emission%20from%20Classical%20Nova%20V392%20Per:%20Measurements%20from%20Fermi%20and%20HAWC&rft.jtitle=arXiv.org&rft.au=Albert,%20A&rft.date=2022-12-16&rft.eissn=2331-8422&rft_id=info:doi/10.48550/arxiv.2201.10644&rft_dat=%3Cproquest%3E2623197893%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2623197893&rft_id=info:pmid/&rfr_iscdi=true