Figure 2 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 2.

Normalized band-averaged gain (intensity beam response) along meridian. Sensitivity is obtained with a composite beam model that includes primary and formed beam effects. Each point represents an average sensitivity within a synthesized beam’s 600 MHz FWHM. The dashed portion of the profile shows the lower transit. The sensitivity spike at zenith is a consequence of the beamforming technique (Ng et al. 2017).

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