Figure 1 from No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution

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No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution

Authors: A. Josephy, P. Chawla, A. P. Curtin, V. M. Kaspi, M. Bhardwaj, P. J. Boyle, C. Brar, T. Cassanelli, E. Fonseca, B. M. Gaensler, C. Leung, H.-H. Lin, K. W. Masui, R. Mckinven, J. Mena-Parra, D. Michilli, C. Ng, Z. Pleunis, M. Rafiei-Ravandi, M. Rahman, P. Sanghavi, P. Scholz, K. Shin, K. M. Smith, I. H. Stairs, S. P. Tendulkar, and A. V. Zwaniga

2021 The Astrophysical Journal 923 2.

Provider: AAS Journals

Caption: Figure 1.

Cumulative exposure (dashed) and cumulative source positions (solid) as a function of absolute Galactic latitude (black) and as a function of decl. (blue). Note that the slope increase above decl. ∼70° is due to doubled exposure from the secondary “lower” transit. Only the cuts described in Section 2 have been applied to the original Catalog 1 sample of bursts.

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