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Skynet Algorithm for Single-dish Radio Mapping. I. Contaminant-cleaning, Mapping, and Photometering Small-scale Structures

  • Authors: J. R. Martin, D. E. Reichart, D. A. Dutton, M. P. Maples, T. A. Berger, F. D. Ghigo, J. B. Haislip, O. H. Shaban, A. S. Trotter, L. M. Barnes, M. L. Paggen, R. L. Gao, C. P. Salemi, G. I. Langston, S. Bussa, J. A. Duncan, S. White, S. A. Heatherly, J. B. Karlik, E. M. Johnson, J. E. Reichart, A. C. Foster, V. V. Kouprianov, S. Mazlin, and J. Harvey

2019 The Astrophysical Journal Supplement Series 240 12.

  • Provider: AAS Journals

Caption: Figure 33.

Top: zoom-in of the first panel of Figure 32, but in 2D. Purple dots mark observation points. Green contours mark the 0%, 25%, 50%, 75%, and 100% of peak levels of the local model. Green pluses mark observation points within the domain of the local model that were not rejected, for being too high, given the modeled noise level (Section 3.5). A locally modeled surface (Section 1.2.1; see Section 3.7) has been applied for visualization only. Middle: zoom-in of the fourth panel of Figure 32 in 2D. Bottom: zoom-in of the fifth panel of Figure 32 in 2D, which is nearly identical, despite not being contaminated with the simulated RFI.

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