Erratum: Search for dark matter gamma-ray emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory (Journal of Cosmology and Astroparticle Physics (2018) 6 (43) DOI: 10.1088/1475-7516/2018/06/043)

A. Albert, R. Alfaro, C. Alvarez, J. D. Álvarez, R. Arceo, J. C. Arteaga-Velázquez, D. Avila Rojas, H. A. Ayala Solares, A. Becerril, E. Belmont-Moreno, S. Y. Benzvi, A. Bernal, C. Brisbois, K. S. Caballero-Mora, T. Capistrán, A. Carramiñana, S. Casanova, M. Castillo, U. Cotti, J. CotzomiS. Coutiño De León, C. De León, S. Dichiara, B. L. Dingus, M. A. Duvernois, J. C. Díaz-Vélez, C. Eckner, K. Engel, O. Enríquez-Rivera, C. Espinoza, D. W. Fiorino, N. Fraija, E. De La Fuente, A. Galván-Gámez, J. A. García-González, F. Garfias, A. González Muñoz, M. M. González, J. A. Goodman, Z. Hampel-Arias, J. P. Harding, S. Hernandez, A. Hernandez-Almada, B. Hona, P. Hüntemeyer, A. Iriarte, A. Jardin-Blicq, V. Joshi, S. Kaufmann, G. J. Kunde, D. Lennarz, H. León Vargas, J. T. Linnemann, A. L. Longinotti, G. Luis Raya, R. Luna-García, K. Malone, S. S. Marinelli, O. Martinez, J. Martínez-Castro, H. Martínez-Huerta, J. A. Matthews, P. Miranda-Romagnoli, E. Moreno, M. Mostafa, A. Nayerhoda, L. Nellen, M. Newbold, M. U. Nisa, R. Noriega-Papaqui, R. Pelayo, J. Pretz, E. G. Pérez-Pérez, Z. Ren, C. D. Rho, C. Riviére, D. Rosa-González, M. Rosenberg, E. Ruiz-Velasco, E. Ruiz-Velasco, H. Salazar, F. Salesa Greus, A. Sandoval, M. Schneider, M. Seglar Arroyo, G. Sinnis, A. J. Smith, R. W. Springer, P. Surajbali, I. Taboada, O. Tibolla, K. Tollefson, I. Torres, T. N. Ukwatta, L. Villaseñor, T. Weisgarber, S. Westerhoff, J. Wood, T. Yapici, G. Zaharijas, A. Zepeda, H. Zhou

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Abstract

We'd like to submit an erratum on our paper Search for Dark Matter Gamma-ray Emission from the Andromeda Galaxy with the High-Altitude Water Cherenkov Observatory (JCAP06(2018)043). The original figure 6 (bottom) is incorrect. The y-axis says \dN/dE" and the green curve is correct, but the limit data points are actually the upper limits on the normalization of the power law (K), not dN/dE. Figure 1 is the corrected plot where we plot E2dN=dE for both the limit data points and the green comparison model curve. (Figure Presented).

Original languageEnglish
Article numberE01
JournalJournal of Cosmology and Astroparticle Physics
Volume2019
Issue number4
DOIs
StatePublished - 8 Apr 2019

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