Figure 6 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 6.

Distributions of detection latitudes (empirical, solid lines) and exposure (cumulative, dashed lines). Absolute Galactic latitude is shown on the top row and decl. on the bottom. Each column corresponds to a different sensitivity cut and filtered sample of detections. Shaded regions are a 2σ band derived from an ensemble of simulated detections, where each mock sample includes the same number of bursts as the observed sample and is generated from the exposure CDF.

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