Figure 23 from Skynet Algorithm for Single-dish Radio Mapping. I. Contaminant-cleaning, Mapping, and Photometering Small-scale Structures

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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 23.

20 m L-band raster from Figure 5 background-subtracted, with 7 (left; Table 1) and 24 (right) beamwidth scales (the map is 24 beamwidths across). Locally modeled surfaces (Section 1.2.1, see Section 3.7) have been applied for visualization only. Hyperbolic arcsine scaling is used to emphasize fainter structures.

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