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Search for Very High-energy Gamma Rays from the Northern Fermi Bubble Region with HAWC
- Abeysekara, AU;
- Albert, A;
- Alfaro, R;
- Alvarez, C;
- Álvarez, JD;
- Arceo, R;
- Arteaga-Velázquez, JC;
- Solares, HA Ayala;
- Barber, AS;
- Bautista-Elivar, N;
- Becerril, A;
- Belmont-Moreno, E;
- BenZvi, SY;
- Berley, D;
- Braun, J;
- Brisbois, C;
- Caballero-Mora, KS;
- Capistrán, T;
- Carramiñana, A;
- Casanova, S;
- Castillo, M;
- Cotti, U;
- Cotzomi, J;
- de León, S Coutiño;
- De León, C;
- De la Fuente, E;
- Hernandez, R Diaz;
- Dingus, BL;
- DuVernois, MA;
- Díaz-Vélez, JC;
- Ellsworth, RW;
- Engel, K;
- Fick, B;
- Fiorino, DW;
- Fleischhack, H;
- Fraija, N;
- García-González, JA;
- Garfias, F;
- Gerhardt, M;
- Muñoz, A González;
- González, MM;
- Goodman, JA;
- Hampel-Arias, Z;
- Harding, JP;
- Hernandez, S;
- Hernandez-Almada, A;
- Hinton, J;
- Hona, B;
- Hui, CM;
- Hüntemeyer, P;
- Iriarte, A;
- Jardin-Blicq, A;
- Joshi, V;
- Kaufmann, S;
- Kieda, D;
- Lara, A;
- Lauer, RJ;
- Lee, WH;
- Lennarz, D;
- Vargas, H León;
- Linnemann, JT;
- Longinotti, AL;
- Raya, G Luis;
- Luna-García, R;
- López-Coto, R;
- Malone, K;
- Marinelli, SS;
- Martinez, O;
- Martinez-Castellanos, I;
- Martínez-Castro, J;
- Martínez-Huerta, H;
- Matthews, JA;
- Miranda-Romagnoli, P;
- Moreno, E;
- Mostafá, M;
- Nellen, L;
- Newbold, M;
- Nisa, MU;
- Noriega-Papaqui, R;
- Pelayo, R;
- Pretz, J;
- Pérez-Pérez, EG;
- Ren, Z;
- Rho, CD;
- Rivière, C;
- Rosa-González, D;
- Rosenberg, M;
- Ruiz-Velasco, E;
- Salazar, H;
- Greus, F Salesa;
- Sandoval, A;
- Schneider, M;
- Schoorlemmer, H;
- Sinnis, G;
- Smith, AJ;
- Springer, RW;
- Surajbali, P;
- Taboada, I;
- Tibolla, O;
- Tollefson, K;
- Torres, I;
- Ukwatta, TN;
- Vianello, G;
- Weisgarber, T;
- Westerhoff, S;
- Wisher, IG;
- Wood, J;
- Yapici, T;
- Yodh, GB;
- Zepeda, A;
- Zhou, H
- et al.
Abstract
We present a search for very high-energy gamma-ray emission from the Northern Fermi Bubble region using data collected with the High Altitude Water Cherenkov gamma-ray observatory. The size of the data set is 290 days. No significant excess is observed in the Northern Fermi Bubble region, so upper limits above 1 TeV are calculated. The upper limits are between and . The upper limits disfavor a proton injection spectrum that extends beyond 100 TeV without being suppressed. They also disfavor a hadronic injection spectrum derived from neutrino measurements.
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