A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415

Ian Herzog; A. Albert; R. Alfaro; C. Alvarez; A. Andrés; J. C. Arteaga-Velázquez; D. Avila Rojas; H. A. Ayala Solares; R. Babu; E. Belmont-Moreno; K. S. Caballero-Mora; T. Capistrán; S. Yun-Cárcamo; A. Carramiñana; F. Carreón; U. Cotti; J. Cotzomi; S. Coutiño de León; E. De la Fuente; D. Depaoli; C. de León; R. Diaz Hernandez; J. C. Díaz-Vélez; B. L. Dingus; M. Durocher; M. A. DuVernois; K. Engel; C. Espinoza; K. L. Fan; K. Fang; N. I. Fraija; J. A. García-González; F. Garfias; H. Goksu; M. M. González; J. A. Goodman; S. Groetsch; J. P. Harding; S. Hernandez; I. Herzog; J. Hinton; D. Huang; F. Hueyotl-Zahuantitla; P. Hüntemeyer; A. Iriarte; V. Joshi; S. Kaufmann; D. Kieda; A. Lara; J. Lee; W. H. Lee; H. León Vargas; J. Linnemann; A. L. Longinotti; G. Luis-Raya; K. Malone; J. Martínez-Castro; J. A.J. Matthews; P. Miranda-Romagnoli; J. Montes; J. A. Morales-Soto; M. Mostafá; L. Nellen; M. U. Nisa; R. Noriega-Papaqui; L. Olivera-Nieto; N. Omodei; Y. Pérez Araujo; E. G. Pérez-Pérez; A. Pratts; C. D. Rho; D. Rosa-Gonzalez; E. Ruiz-Velasco; H. Salazar; D. Salazar-Gallegos; A. Sandoval; M. Schneider; G. Schwefer; J. Serna-Franco; A. J. Smith; Y. Son; R. W. Springer; O. Tibolla; K. Tollefson; I. Torres; R. Torres-Escobedo; R. Turner; F. Ureña-Mena; E. Varela; L. Villaseñor; X. Wang; I. J. Watson; F. Werner; K. Whitaker; E. Willox; H. Wu; H. Zhou

A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415

Ian Herzog
, A. Albert
, R. Alfaro
, C. Alvarez
, A. Andrés
, J. C. Arteaga-Velázquez
, D. Avila Rojas
, H. A. Ayala Solares
, R. Babu
, E. Belmont-Moreno
, K. S. Caballero-Mora
, T. Capistrán
, S. Yun-Cárcamo
, A. Carramiñana
, F. Carreón
, U. Cotti
, J. Cotzomi
, S. Coutiño de León
, E. De la Fuente
, D. Depaoli

C. de León, R. Diaz Hernandez, J. C. Díaz-Vélez, B. L. Dingus, M. Durocher, M. A. DuVernois, K. Engel, C. Espinoza, K. L. Fan, K. Fang, N. I. Fraija, J. A. García-González, F. Garfias, H. Goksu, M. M. González, J. A. Goodman, S. Groetsch, J. P. Harding, S. Hernandez, I. Herzog, J. Hinton, D. Huang, F. Hueyotl-Zahuantitla, P. Hüntemeyer, A. Iriarte, V. Joshi, S. Kaufmann, D. Kieda, A. Lara, J. Lee, W. H. Lee, H. León Vargas, J. Linnemann, A. L. Longinotti, G. Luis-Raya, K. Malone, J. Martínez-Castro, J. A.J. Matthews, P. Miranda-Romagnoli, J. Montes, J. A. Morales-Soto, M. Mostafá, L. Nellen, M. U. Nisa, R. Noriega-Papaqui, L. Olivera-Nieto, N. Omodei, Y. Pérez Araujo, E. G. Pérez-Pérez, A. Pratts, C. D. Rho, D. Rosa-Gonzalez, E. Ruiz-Velasco, H. Salazar, D. Salazar-Gallegos, A. Sandoval, M. Schneider, G. Schwefer, J. Serna-Franco, A. J. Smith, Y. Son, R. W. Springer, O. Tibolla, K. Tollefson, I. Torres, R. Torres-Escobedo, R. Turner, F. Ureña-Mena, E. Varela, L. Villaseñor, X. Wang, I. J. Watson, F. Werner, K. Whitaker, E. Willox, H. Wu, H. Zhou

Department of Physics

Research output: Contribution to journal › Conference article › peer-review

1 Scopus citations

Abstract

The Cygnus Cocoon region is a complex region that contains an OB star cluster that is prominent in the TeV energy range. First observed by HEGRA as the unassociated TeV source TeV J2032+4130, follow-up observations with the High-Altitude Water Cherenkov (HAWC) observatory revealed additional complexity in the region. Previous work has found two sources: 3HWC J2031+415 and 3HWC J2020+403. 3HWC J2031+415 is a significant TeV gamma-ray source whose emission is a composition of 2 sources: HAWC J2030+409, associated with the Fermi-LAT Cocoon and HAWC J2031+415, a pulsar wind nebula (PWN) possibly associated with PSR J2032+4127. 3HWC J2020+403 is a single source and is associated with the supernova remnant Gamma Cygni. Using a multi-source fitting algorithm in The Multi-Mission Maximum Likelihood framework, an investigation of the TeV spectrum and very-high-energy morphology of HAWC J2031+415 is presented in this work. Additionally, X-ray observations from Suzaku are used to constrain the leptonic production of gamma rays by the PWN.

Original language	English
Article number	757
Journal	Proceedings of Science
Volume	444
State	Published - 27 Sep 2024
Event	38th International Cosmic Ray Conference, ICRC 2023 - Nagoya, Japan Duration: 26 Jul 2023 → 3 Aug 2023

Cite this

Herzog, I., Albert, A., Alfaro, R., Alvarez, C., Andrés, A., Arteaga-Velázquez, J. C., Avila Rojas, D., Ayala Solares, H. A., Babu, R., Belmont-Moreno, E., Caballero-Mora, K. S., Capistrán, T., Yun-Cárcamo, S., Carramiñana, A., Carreón, F., Cotti, U., Cotzomi, J., Coutiño de León, S., De la Fuente, E., ... Zhou, H. (2024). A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415. Proceedings of Science, 444, Article 757.

@article{5a185c4a37d048c1867a494c20e91926,

title = "A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415",

abstract = "The Cygnus Cocoon region is a complex region that contains an OB star cluster that is prominent in the TeV energy range. First observed by HEGRA as the unassociated TeV source TeV J2032+4130, follow-up observations with the High-Altitude Water Cherenkov (HAWC) observatory revealed additional complexity in the region. Previous work has found two sources: 3HWC J2031+415 and 3HWC J2020+403. 3HWC J2031+415 is a significant TeV gamma-ray source whose emission is a composition of 2 sources: HAWC J2030+409, associated with the Fermi-LAT Cocoon and HAWC J2031+415, a pulsar wind nebula (PWN) possibly associated with PSR J2032+4127. 3HWC J2020+403 is a single source and is associated with the supernova remnant Gamma Cygni. Using a multi-source fitting algorithm in The Multi-Mission Maximum Likelihood framework, an investigation of the TeV spectrum and very-high-energy morphology of HAWC J2031+415 is presented in this work. Additionally, X-ray observations from Suzaku are used to constrain the leptonic production of gamma rays by the PWN.",

author = "Ian Herzog and A. Albert and R. Alfaro and C. Alvarez and A. Andr{\'e}s and Arteaga-Vel{\'a}zquez, \{J. C.\} and \{Avila Rojas\}, D. and \{Ayala Solares\}, \{H. A.\} and R. Babu and E. Belmont-Moreno and Caballero-Mora, \{K. S.\} and T. Capistr{\'a}n and S. Yun-C{\'a}rcamo and A. Carrami{\~n}ana and F. Carre{\'o}n and U. Cotti and J. Cotzomi and \{Couti{\~n}o de Le{\'o}n\}, S. and \{De la Fuente\}, E. and D. Depaoli and \{de Le{\'o}n\}, C. and \{Diaz Hernandez\}, R. and D{\'i}az-V{\'e}lez, \{J. C.\} and Dingus, \{B. L.\} and M. Durocher and DuVernois, \{M. A.\} and K. Engel and C. Espinoza and Fan, \{K. L.\} and K. Fang and Fraija, \{N. I.\} and Garc{\'i}a-Gonz{\'a}lez, \{J. A.\} and F. Garfias and H. Goksu and Gonz{\'a}lez, \{M. M.\} and Goodman, \{J. A.\} and S. Groetsch and Harding, \{J. P.\} and S. Hernandez and I. Herzog and J. Hinton and D. Huang and F. Hueyotl-Zahuantitla and P. H{\"u}ntemeyer and A. Iriarte and V. Joshi and S. Kaufmann and D. Kieda and A. Lara and J. Lee and Lee, \{W. H.\} and \{Le{\'o}n Vargas\}, H. and J. Linnemann and Longinotti, \{A. L.\} and G. Luis-Raya and K. Malone and J. Mart{\'i}nez-Castro and Matthews, \{J. A.J.\} and P. Miranda-Romagnoli and J. Montes and Morales-Soto, \{J. A.\} and M. Mostaf{\'a} and L. Nellen and Nisa, \{M. U.\} and R. Noriega-Papaqui and L. Olivera-Nieto and N. Omodei and \{P{\'e}rez Araujo\}, Y. and P{\'e}rez-P{\'e}rez, \{E. G.\} and A. Pratts and Rho, \{C. D.\} and D. Rosa-Gonzalez and E. Ruiz-Velasco and H. Salazar and D. Salazar-Gallegos and A. Sandoval and M. Schneider and G. Schwefer and J. Serna-Franco and Smith, \{A. J.\} and Y. Son and Springer, \{R. W.\} and O. Tibolla and K. Tollefson and I. Torres and R. Torres-Escobedo and R. Turner and F. Ure{\~n}a-Mena and E. Varela and L. Villase{\~n}or and X. Wang and Watson, \{I. J.\} and F. Werner and K. Whitaker and E. Willox and H. Wu and H. Zhou",

note = "Publisher Copyright: {\textcopyright} Copyright owned by the author(s) under the terms of the Creative Commons.; 38th International Cosmic Ray Conference, ICRC 2023 ; Conference date: 26-07-2023 Through 03-08-2023",

year = "2024",

month = sep,

day = "27",

language = "English",

volume = "444",

journal = "Proceedings of Science",

issn = "1824-8039",

publisher = "Sissa Medialab Srl",

}

Herzog, I, Albert, A, Alfaro, R, Alvarez, C, Andrés, A, Arteaga-Velázquez, JC, Avila Rojas, D, Ayala Solares, HA, Babu, R, Belmont-Moreno, E, Caballero-Mora, KS, Capistrán, T, Yun-Cárcamo, S, Carramiñana, A, Carreón, F, Cotti, U, Cotzomi, J, Coutiño de León, S, De la Fuente, E, Depaoli, D, de León, C, Diaz Hernandez, R, Díaz-Vélez, JC, Dingus, BL, Durocher, M, DuVernois, MA, Engel, K, Espinoza, C, Fan, KL, Fang, K, Fraija, NI, García-González, JA, Garfias, F, Goksu, H, González, MM, Goodman, JA, Groetsch, S, Harding, JP, Hernandez, S, Herzog, I, Hinton, J, Huang, D, Hueyotl-Zahuantitla, F, Hüntemeyer, P, Iriarte, A, Joshi, V, Kaufmann, S, Kieda, D, Lara, A, Lee, J, Lee, WH, León Vargas, H, Linnemann, J, Longinotti, AL, Luis-Raya, G, Malone, K, Martínez-Castro, J, Matthews, JAJ, Miranda-Romagnoli, P, Montes, J, Morales-Soto, JA, Mostafá, M, Nellen, L, Nisa, MU, Noriega-Papaqui, R, Olivera-Nieto, L, Omodei, N, Pérez Araujo, Y, Pérez-Pérez, EG, Pratts, A, Rho, CD, Rosa-Gonzalez, D, Ruiz-Velasco, E, Salazar, H, Salazar-Gallegos, D, Sandoval, A, Schneider, M, Schwefer, G, Serna-Franco, J, Smith, AJ, Son, Y, Springer, RW, Tibolla, O, Tollefson, K, Torres, I, Torres-Escobedo, R, Turner, R, Ureña-Mena, F, Varela, E, Villaseñor, L, Wang, X, Watson, IJ, Werner, F, Whitaker, K, Willox, E, Wu, H & Zhou, H 2024, 'A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415', Proceedings of Science, vol. 444, 757.

TY - JOUR

T1 - A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415

AU - Herzog, Ian

AU - Albert, A.

AU - Alfaro, R.

AU - Alvarez, C.

AU - Andrés, A.

AU - Arteaga-Velázquez, J. C.

AU - Avila Rojas, D.

AU - Ayala Solares, H. A.

AU - Babu, R.

AU - Belmont-Moreno, E.

AU - Caballero-Mora, K. S.

AU - Capistrán, T.

AU - Yun-Cárcamo, S.

AU - Carramiñana, A.

AU - Carreón, F.

AU - Cotti, U.

AU - Cotzomi, J.

AU - Coutiño de León, S.

AU - De la Fuente, E.

AU - Depaoli, D.

AU - de León, C.

AU - Diaz Hernandez, R.

AU - Díaz-Vélez, J. C.

AU - Dingus, B. L.

AU - Durocher, M.

AU - DuVernois, M. A.

AU - Engel, K.

AU - Espinoza, C.

AU - Fan, K. L.

AU - Fang, K.

AU - Fraija, N. I.

AU - García-González, J. A.

AU - Garfias, F.

AU - Goksu, H.

AU - González, M. M.

AU - Goodman, J. A.

AU - Groetsch, S.

AU - Harding, J. P.

AU - Hernandez, S.

AU - Herzog, I.

AU - Hinton, J.

AU - Huang, D.

AU - Hueyotl-Zahuantitla, F.

AU - Hüntemeyer, P.

AU - Iriarte, A.

AU - Joshi, V.

AU - Kaufmann, S.

AU - Kieda, D.

AU - Lara, A.

AU - Lee, J.

AU - Lee, W. H.

AU - León Vargas, H.

AU - Linnemann, J.

AU - Longinotti, A. L.

AU - Luis-Raya, G.

AU - Malone, K.

AU - Martínez-Castro, J.

AU - Matthews, J. A.J.

AU - Miranda-Romagnoli, P.

AU - Montes, J.

AU - Morales-Soto, J. A.

AU - Mostafá, M.

AU - Nellen, L.

AU - Nisa, M. U.

AU - Noriega-Papaqui, R.

AU - Olivera-Nieto, L.

AU - Omodei, N.

AU - Pérez Araujo, Y.

AU - Pérez-Pérez, E. G.

AU - Pratts, A.

AU - Rho, C. D.

AU - Rosa-Gonzalez, D.

AU - Ruiz-Velasco, E.

AU - Salazar, H.

AU - Salazar-Gallegos, D.

AU - Sandoval, A.

AU - Schneider, M.

AU - Schwefer, G.

AU - Serna-Franco, J.

AU - Smith, A. J.

AU - Son, Y.

AU - Springer, R. W.

AU - Tibolla, O.

AU - Tollefson, K.

AU - Torres, I.

AU - Torres-Escobedo, R.

AU - Turner, R.

AU - Ureña-Mena, F.

AU - Varela, E.

AU - Villaseñor, L.

AU - Wang, X.

AU - Watson, I. J.

AU - Werner, F.

AU - Whitaker, K.

AU - Willox, E.

AU - Wu, H.

AU - Zhou, H.

PY - 2024/9/27

Y1 - 2024/9/27

N2 - The Cygnus Cocoon region is a complex region that contains an OB star cluster that is prominent in the TeV energy range. First observed by HEGRA as the unassociated TeV source TeV J2032+4130, follow-up observations with the High-Altitude Water Cherenkov (HAWC) observatory revealed additional complexity in the region. Previous work has found two sources: 3HWC J2031+415 and 3HWC J2020+403. 3HWC J2031+415 is a significant TeV gamma-ray source whose emission is a composition of 2 sources: HAWC J2030+409, associated with the Fermi-LAT Cocoon and HAWC J2031+415, a pulsar wind nebula (PWN) possibly associated with PSR J2032+4127. 3HWC J2020+403 is a single source and is associated with the supernova remnant Gamma Cygni. Using a multi-source fitting algorithm in The Multi-Mission Maximum Likelihood framework, an investigation of the TeV spectrum and very-high-energy morphology of HAWC J2031+415 is presented in this work. Additionally, X-ray observations from Suzaku are used to constrain the leptonic production of gamma rays by the PWN.

AB - The Cygnus Cocoon region is a complex region that contains an OB star cluster that is prominent in the TeV energy range. First observed by HEGRA as the unassociated TeV source TeV J2032+4130, follow-up observations with the High-Altitude Water Cherenkov (HAWC) observatory revealed additional complexity in the region. Previous work has found two sources: 3HWC J2031+415 and 3HWC J2020+403. 3HWC J2031+415 is a significant TeV gamma-ray source whose emission is a composition of 2 sources: HAWC J2030+409, associated with the Fermi-LAT Cocoon and HAWC J2031+415, a pulsar wind nebula (PWN) possibly associated with PSR J2032+4127. 3HWC J2020+403 is a single source and is associated with the supernova remnant Gamma Cygni. Using a multi-source fitting algorithm in The Multi-Mission Maximum Likelihood framework, an investigation of the TeV spectrum and very-high-energy morphology of HAWC J2031+415 is presented in this work. Additionally, X-ray observations from Suzaku are used to constrain the leptonic production of gamma rays by the PWN.

UR - https://www.scopus.com/pages/publications/85185576658

M3 - Conference article

AN - SCOPUS:85185576658

SN - 1824-8039

VL - 444

JO - Proceedings of Science

JF - Proceedings of Science

M1 - 757

T2 - 38th International Cosmic Ray Conference, ICRC 2023

Y2 - 26 July 2023 through 3 August 2023

ER -

A Spectral, Morphological, and Emission Analysis of Gamma Ray Source HAWC J2031+415

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